Leica TPS1100 User Manual

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Leica TPS1100 Professional Series
User Manual
Version 2.2
English
Page 2
Electronic total stations
Congratulations on your purchase of a TPS1100 Professional Series instrument.
This manual contains important safety directions (refer to chapter "Safety directions") as well as instructions for setting up the product
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Product identification
The instrument model and the serial number of your product are indicated on the label in the battery compartment. Enter the model and serial number in your manual and always refer to this information when you need to contact your agency or authorized service workshop. Type: Serial number:
TPS1100 - User Manual 2.2.1en
Software version: Language:
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Product identification
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Symbols used in this manual
The symbols used in this User Manual have the following meanings:
DANGER:
Indicates an imminently hazardous situation which, if not avoided, will result in death or serious injury.
WARNING:
Indicates a potentially hazardous situation or an unintended use which, if not avoided, could result in death or serious injury.
CAUTION:
Indicates a potentially hazardous situation or an unintended use which, if not avoided, may result in minor or moderate injury and / or appreciable material, financial and environmental damage.
Important paragraphs which must be adhered to in practice as they enable the product to be used in a technically correct and efficient manner.
Symbols used in this manual
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View of chapters
Contents
Introduction
Description of the system
Preparation, setting up
Checking and adjusting
System functions
System parameters
Data format
Care and transport
Safety directions
Technical specifications
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10
12
22
29
49
97
108
119
121
143
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Index
156
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View of chapters
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Contents
Introduction ................................................. 10
Validity ....................................................................... 11
Documentation ...........................................................11
Instrument descriptions ............................................. 12
Description of the system........................... 12
Distance measurement ............................................. 13
Extended Range (Option) .......................................... 14
Automatic Target Recognition ATR / LOCK ................ 15
Quick Prism Search with PowerSearch ...................... 15
Guide Light EGL ........................................................ 16
RCS (Remote Controlled Surveying) .......................... 17
System concept ......................................................... 18
Leica Survey Office PC software package .................. 20
Batteries and chargers ............................................... 21
Preparation, setting up ............................... 22
Unpacking ................................................................. 22
Charging the battery .................................................. 23
Inserting / replacing battery ........................................ 24
Insert PC-card ........................................................... 26
Setting up the instrument with optical plummet or laser
plummet .................................................................... 27
Levelling-up with the electronic bubble ....................... 28
Contents
Checking and adjusting .............................. 29
Electronically ............................................................. 29
Compensator (electronic bubble) ................................... 32
V-index error ................................................................... 34
Line of sight .................................................................... 36
Tilting axis ....................................................................... 38
Combined error determination ........................................ 40
Deactivating the instrument-error correction ................... 40
ATR collimation............................................................... 41
Mechanically ............................................................. 44
Tripod ............................................................................. 44
Bull's eye bubble on instrument ...................................... 44
Bull's eye bubble on the tribrach ..................................... 44
Optical plummet ............................................................. 45
Laser plummet ................................................................ 46
Reflector-free EDM ......................................................... 47
System functions ........................................ 49
Data configuration ..................................................... 49
Data job (D JOB) and meas. job (M JOB) ....................... 49
Creating a new job (NEW) .............................................. 50
Codelist .......................................................................... 50
Creating a new codelist (NEW) ....................................... 51
Copying a codelist (COPY) ............................................. 51
Data management .......................................................... 51
Importing point data (IMPOR) ......................................... 53
Displaying and importing point data (VIEW) ................... 54
Displaying and editing GSI data (SEARC) ...................... 54
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Contents (continued)
Placeholder (wild cards) in searching for points .............. 55
Manual input of coordinates (INPUT) .............................. 56
Converting data .............................................................. 56
Formatting the PC-card (FORMT) ................................... 59
Inspecting the PC-card (PROOF) ................................... 60
Setting the recording mask (RMask) ............................... 60
Setting the display mask (DMask) ................................... 61
GSI-parameters .............................................................. 62
Measurement functions ............................................. 66
Setting and entering the Hz direction (SetHz) ................. 67
Distance measurement ................................................... 67
Selecting the EDM measuring program,
target type and reflector .................................................. 68
Switch between IR/RL .................................................... 69
Switch between Standard/Tracking ................................. 70
Switch between Fast measurement/Rapid ...................... 70
Tracking .......................................................................... 70
Setting / defining prisms ................................................. 70
EDM test ......................................................................... 71
Distance corrections, ppm .............................................. 71
Reduced distance corrections ppm ................................. 73
Measurement & recording (REC) .................................... 73
Measuring distances and angles separately
(DIST + REC) ................................................................. 74
Measuring distances and angles together
with storage (ALL) .......................................................... 75
Storing station data (REC) .............................................. 75
Changing face (I<>II) ...................................................... 75
Last point number (L.Pt.) ................................................ 76
Deleting the GSI block (Del B) ........................................ 76
Manual distance entry ..................................................... 76
Positioning the last point stored (LAST) .......................... 77
V-angle modes ............................................................... 77
Offset .............................................................................. 78
Switching between display masks (>DISP) ..................... 78
Individual point number (INDIV / RUN) ........................... 79
Coding ............................................................................ 79
Quick Coding (QCod+ / QCod-) ..................................... 81
Check Orientation ........................................................... 82
GSI communication parameters ..................................... 83
Communication ......................................................... 83
Interface parameters (GeoCOM) .................................... 83
RCS communication parameters .................................... 84
On-line mode .................................................................. 84
Automatic Target Recognition .................................... 85
Functionality ................................................................... 85
ATR-Mode (ATR+ / ATR-) ............................................... 86
LOCK-Mode (LOCK+ / LOCK-) ....................................... 86
L.UNT-Mode (L.INT+ / L.GO) .......................................... 87
LAST mode (LAST) ........................................................ 88
Hz / V ............................................................................. 88
Automatic Reflector Search ....................................... 89
RCS Searching Window ................................................. 90
Definition of a Working Area (WORKA) .......................... 91
Activate/Deactivate Working Area (WORK+/WORK-) ..... 92
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Contents
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Contents (continued)
General functions ...................................................... 92
Instrument designation and software version (INFO) ...... 92
Electronic bubble (LEVEL) .............................................. 92
Illumination ..................................................................... 93
Accessories .................................................................... 94
Loading a configuration file (LOAD) ................................ 95
Loading a system-parameter file ..................................... 96
System parameters ..................................... 97
General parameters .................................................. 97
Load application ............................................................. 97
Load system language ................................................... 97
Date ................................................................................ 98
Date form. ....................................................................... 98
Time ............................................................................... 98
Alpha mode .................................................................... 98
Time form. ...................................................................... 98
Key beep ........................................................................ 98
Configuration parameters .......................................... 99
Autoexec. ....................................................................... 99
Language ....................................................................... 99
Dist. Unit ......................................................................... 99
Dist. Dec. ........................................................................ 99
Angle Unit ....................................................................... 99
Angle Dec. ...................................................................... 99
Temp. Unit .................................................................... 100
Press. Unit .................................................................... 100
Coord. Seq. .................................................................. 100
Hz system ..................................................................... 100
Face I ........................................................................... 100
Compensator ................................................................ 101
Hz-Corr. ........................................................................ 101
Sect. Beep .................................................................... 102
Sect. Angle ................................................................... 102
Release V-angle ........................................................... 102
V-Display ...................................................................... 103
Power mode ................................................................. 103
Power Time .................................................................. 103
Dist. Delay .................................................................... 103
PPM entry ..................................................................... 104
Info / Atrib ..................................................................... 104
Auto Dist ....................................................................... 105
Measurement parameters ....................................... 105
Pt. Id. mode .................................................................. 105
Offs. Mode .................................................................... 105
Increment ..................................................................... 106
Work settings .......................................................... 107
Meas Job ...................................................................... 107
Data Job ....................................................................... 107
Codelist ........................................................................ 107
Quick-Code .................................................................. 107
Data format ................................................ 108
Introduction ............................................................. 108
Contents
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Contents (continued)
Format with 8 or 16 characters ................................ 108
Block concept .......................................................... 109
Structure of a block ................................................. 109
Measurement block .................................................. 110
Code block ...............................................................110
Terminator of a data block ........................................ 110
Structure of a word ................................................... 111
Word index (positions 1 - 2) ........................................... 111
Information relating to data (positions 3 - 6) .................. 112
Data (positions 7 - 15/23) ............................................. 113
Separating character (position 16/24) ........................... 114
Block number ............................................................... 114
Units of measurement .................................................. 115
Example of data format ............................................ 115
Format of a theodolite measurement block ................... 116
Format of a code block ................................................. 118
Care and transport .....................................119
Transport ................................................................. 119
Maintainance for motorized drives ............................. 119
Storage ................................................................... 120
Cleaning and drying ................................................. 120
Safety directions ....................................... 121
Intended use of instrument ...................................... 121
Permitted uses ............................................................. 121
Prohibited uses ............................................................. 121
Limits of use ............................................................ 122
Responsibilities ....................................................... 123
Hazards of use ........................................................ 123
Main hazards of use ..................................................... 123
Laser classification .................................................. 127
Integrated distancer (infrared laser) ............................. 128
Integrated distancer (visible laser) ............................... 129
Automatic target recognition (ATR) ............................... 134
PowerSearch ................................................................ 136
Guide light EGL ............................................................ 137
Laser plummet .............................................................. 138
Electromagnetic Compatibility (EMC) ....................... 140
FCC statement (applicable in U.S.) .......................... 142
Technical specifications ........................... 143
EGL Guide Light ...................................................... 148
Automatic Target Recognition ATR .......................... 149
PowerSearch .......................................................... 150
Application programs ............................................... 150
Scale correction (ppm) ............................................ 151
Atmospheric correction DD1 ......................................... 152
Reduction to mean sea level DD2 ................................ 153
Projection distortion DD3 .............................................. 153
Atmospheric corrections .......................................... 154
Reduction formulae ................................................. 155
Index ........................................................... 156
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Introduction
6
TPS1100 stands for Total Station Positioning System. The TPS1100
instruments are available as various models with differing classes of accuracy. New technologies have enabled the measuring sequence to be largely automated, bringing advantages such as shorter measuring times, simpler operation and more efficient use. Further elements in the basic equipment are described below.
The R versions have a laser with a visible red beam. The EDM can be switched between two operational modes: measurements with normal infrared or with the visible red laser respectively. With the red laser, reflectors are not required for measuring distances. With infrared, distances of up to seven kilometres can be measured.
All TPS1100 instruments are routinely supplied with a laser plummet located in the vertical axis. The TPS1100 can therefore be set up quickly and accurately over the ground point with the help of the red laser dot.
The A-versions have an automatic target recognition (ATR), which permits rapid, fatigue-free measuring. In ATR mode the fine­pointing is automatic. In LOCK mode an already-targeted point is tracked automatically. For TPS1100 plus instruments an optional PowerSearch module is
available which allows an automatic prism detection within a short period of time.
The EGL guide light is an optional accessory for assistance with targeting. It is located within the telescope and it flashes, so that the person carrying the reflector can
place this in the line of sight of the instrument. The RCS1100 remote control system is an additional option, which allows the remote control of all total stations. The instrument can be controlled either directly on the instrument or at the RCS1100. Especially the A-versions enable the surveyor to work alone. The measurements can also be triggered, inspected and controlled from the target area.
Leica Geosystems offers applications programs for many dif­ferent tasks in surveying. Just choose the software which best meets your needs.
Within the special GeoBasic programming environment, you can create your own application-specific programs for the TPS1100 instruments.
Introduction
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Validity Documentation
The PC cards familiar in the computer industry are also used as the medium for storing data in the TPS1100. The data structures are compatible with those in existing Lei­ca Geosystems total stations.
Leica Survey Office is a PC-program package which supports the TPS1100 and RCS1100 instruments and which enables data to be exchanged between software and hardware components.
This manual applies to all TPS1100 Professional Series instruments.
Differences between the various models are clearly set out and assigned.
General text applies to all types.
For purposes of pictorial illustration, we have selected a TCA model of the TPS1100 Professional Series with EGL options. The illustrations are valid for all models.
Printed short instructions for the system and for the applications are available as well as the present user manual. The enclosed CD ROM contains the entire documentation in electronic form.
User manual: This includes all directions for using the instrument and provides an overview of the system together with important instructions and safety directions.
System Field Manual: This describes the functions of the system in standard use (in instrument case).
Application Programs Field
Manual 1 + 2:
This describes the functions of the programs in standard use (in instrument case).
Application Programs Reference
Manual:
All programs are described in de­tail.
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Introduction
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Description of the system
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Instrument descriptions
1
2
3456
12 13 15
1110
14 18 1917 20
16
1 Carrying handle
7
8
9
2 Optical sight 3 Telescope with integrated EDM,
ATR, EGL and PowerSearch 4 EGL flashing diode (yellow) 5 EGL flashing diode (red) 6 Coaxial optics for angle- and
distance measurement;
Exit port of visible laser beam
(only R-model instruments)
7 PowerSearch sensor
8 Vertical drive screw 9 Focusing ring
10 PC-card housing
11 Horizontal drive screw 12 Footscrew (tribrach) 13 Display 14Tribrach securing knob 15 Keyboard 16 Batteryholder 17 Battery 18 Bull's-eye bubble 19 Laser emission indicator lamp -
only XR-instruments (yellow)
20 Interchangeable eyepiece
1100Z01
Description of the system
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Distance measurement
A laser distancer (EDM) is incorporated into the instruments of the new TPS1100 series. In all versions, the distance can be determined by using an invisible infrared beam which emerges coaxially from the telescope objective.
Very short distances may be
measured reflectorless in Infrared-mode (e.g. to well reflecting targets like traffic signs). In this case the distances are corrected with the addition constant defined for the active reflector.
For applications without reflector, the TCR and TCRA version also use a visible red laser beam which emerges in the same manner. A special arrangement of the EDM, and appropriate arrangement of the beam paths, enable ranges of over five kilometres to be attained with standard prisms; miniprisms, 360° reflectors, and reflector tapes can also be used, and measurement is also possible without a reflector.
When a distance
measurement is triggered, the EDM measures to the object which is in the beam path at that moment.
When measurements are being made using the Reflectorless Red Laser EDM, the results may be influenced by objects passing between the EDM and the intended target surface. This will occur because reflectorless measurements are made to the first surface returning sufficient energy to allow the measurement to take place. For example, if the intended target surface is the surface of a road, but a vehicle passes between the EDM and the target surface as DIST or ALL is pressed, the measurement may be made to the side of the vehicle. The result will be the distance to the vehicle, not to the road surface. If you are using the Long Range Red Laser EDM while measuring to a prism, and an object passes within
30 m of the EDM as DIST or ALL is pressed, the distance measurement may be similarly effected.
In practice, because the measuring time is very short, the surveyor can always find a way of avoiding critical situations.
Wrong result
Correct result
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1100Z461100Z47
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Description of the system
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Extended Range (Option)
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The optional "Extended Range (XR)"­laser is a visible red laser with in-creased measurement range. The coaxial XR - laser makes it possible to measure distances over 170 m (560 ft) reflectorless and over 10 km (6.2 miles) to one prism (refer to the chapter "Technical specifications").
The operation of an XR - instrument is equivalent to a conventional TPS with red laser. Please consider the following points when measuring with the XR - laser (RL & Long Range).
The objective lens should
always be clean. Dirt on the lens (dust, fingerprints, ...) can lead to reduced accuracy.
Reflectorless
Be sure that the laser beam
is not reflected by anything close to the line of sight (e.g. highly reflective objects).
the EDM measures to the object which is in the beam path at that moment. In case of temporary obstruction (e.g. a passing vehicle) or heavy rain, fog or snow, the EDM may measure to the obstruction.
the red laser beam from the line of sight might lead to less accurate measurements. This is because the laser beam might not be reflected from the point at which the crosshairs are pointing.
Therefore, it is recommended to ver­ify that the XR - laser is well colli­mated with the telescope line of sight (refer to the chapter "Checking and adjusting"). This should be done at regular intervals.
target simultaneously.
When a distance measurement is triggered,
When measuring longer dis­tances, any divergence of
Do not measure with two instruments to the same
Long Range to prisms
WARNING:
Due to laser safety
regulations and measuring accuracy, using the Long Range Pro­gram is only allowed to prisms that are more than 1000 m (3300 ft) away.
Whenever possible accurate
measurements to prisms should be made with the standard program (IR).
Long Range to reflector tape
The Long Range Program can also measure to reflector tape. To guaran­tee the accuracy the laser beam must be perpendicular to the reflector tape and the XR - laser must be well adjusted (refer to the chapter "Checking and adjusting").
Description of the system
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Automatic Target Recognition ATR / LOCK
Quick Prism Search with PowerSearch
TCA and TCRA instruments are motorized and equipped with Automatic Target Recognition (ATR) coaxially in the telescope. The guide light (EGL), mounted on the telescope, is optional.
ATR mode
These instruments permit automatic angle and distance measurements to normal prisms and reduce the tedium of precise visual sighting to prisms. The prism is sighted with the optical sight only. Initiating a distance measurement will turn the instrument with the help of the motors to sight the prism-centre automatically. The angles V and Hz are measured to the centre of the prism completion of the distance measurement.
As with all other instrument
errors, the collimation error of the automatic target recognition (ATR) must be redetermined periodically (Refer to chapter "Checking and Adjusting").
LOCK mode
Lock mode will enable TCA instruments to follow a moving prism. Distances can be measured whenever the prism stops for a short time ("Stop and Go mode").
If the assistant changes the
location too quickly, the target may be lost. Make sure that the speed does not exceed the figure given in the technical data.
The PowerSearch sensor consists of a transmitter (1) and a receiver (2). Both are installed in the lower part of the telescope.
1
2
When PowerSearch is activated, the instrument starts to rotate around its standing axis.The transmitter emits a vertical laser swath.
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10
1100Z55
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Description of the system
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Guide Light EGL
6
If the laser swath detects a prism, the reflection is detected by the receiver
0
and the rotation of the instrument is stopped. Afterwards a fine aiming in
The optionally available Guide Light EGL consists of two coloured flashing lights in the telescope of the total station.
1100Z03
vertical direction is performed by the ATR.
PowerSearch can be started at any time by pressing the PowerSearch
12
function key (PS) in the menu PROG.
If RCS mode is activated, then PowerSearch can be switched on during an ATR prism search.
Working range: 5-200 m Swath divergence Hz: 0.025 gon Swath divergence V: ±20 gon
1 Flashing red diode 2 Flashing yellow diode
All TPS1100 instruments can be equipped with this Guide Light. The person at the prism can be guided by the flashing lights directly to the line of sight. It becomes much easier to
1100Z02
6 m (20 ft)
6 m (20 ft)
100 m (330 ft)
set out points.
Description of the system
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RCS (Remote Controlled Surveying)
At a target distance of 100 metres (330 ft) a red/yellow flashing cone of light with a width of 6m (20 ft) is formed on each side. As a result, guiding to the line of sight of the instrument is much easier and faster.
Between the two cones of light a sector about 30mm wide is created. Within this sector both colours are flashing simultaneously. In this case the prism is already right in the line of sight.
Operating range:
5 - 150 m (15 -500 ft)
Divergence:
10 m (33ft) at 100m (330 ft)
The RCS option (Remote Controlled Surveying) permits all models to be controlled from the target area. Especially qualified for this purpose are the TCA and TCRA instruments.
RCS 1100
Combined operation, partly at the TPS1100 and partly at the prism, is also possible. As a result, surveys can be performed solo. It is also possible to monitor the operation on the RCS 1100 and / or to enter the coding on the RCS 1100.
All functions of the TPS1100, including the applications programs, are available on the RCS 1100. The display and the use of the keys are as for the TPS1100.
For further information, refer to the RCS1100 user manual.
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Description of the system
Page 18
System concept
6
All of TPS 1100 models use the same software architecture and the
0
same concept for data storage and data flow.
Software architecture
The software of the TPS1100 can be divided into two groups:
1100Z04
Systemsoftware, Applications
• The system software, which
covers the basic functions
• The applications software, which
supports survey- specific
Data
Survey Office
applications and procedures.
The software permits up to three The system software forms a coherent unit, whereas the applications software can be compiled in accordance with the individual requirements of the user. Using the Leica Survey Office software provided, both the system
languages to remain stored
simultaneously and one of them to be
selected. The range of language
versions available is constantly being
expanded. If you need a particular
language version, please ask your
agency about its availability. software and the applications software can be loaded across the serial interface by the user, who is in a position to install improved software versions.
Description of the system
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System concept, continued
Storage concept and data flow
1100Z05
Survey data is generally stored on a SRAM or ATA flash card corresponding to PCMCIA standards (referred to here as a PC card). The data are stored in MS-DOS file format. Data is exchanged with a PC through either a PCMCIA drive on that PC, or an OMNI drive (optional), or the serial interface (cable link between instrument and PC). The Leica Survey Office software supplied with the instrument includes a program for transferring data across the serial interface.
Instead of using the PC card, the data can be output in GSI format at the serial data interface.
When data is transferred
across the serial interface for storage in an external PC, no data from the applications is output in the report file. Fixed-point coordinates can be read only from the PC card.
GeoBasic
The GeoBasic development environment permits the professional development of additional applications for the TPS1100.
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Description of the system
Page 20
Leica Survey Office PC software package
6
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The Leica Survey Office software includes a series of help programs which support you in your work with the TPS1100 total station.
Installing in the PC
The installation program for Leica Survey Office is located on the TPS1100 CD-ROM supplied with the present handbook. Please note that Survey Office can only be installed on the following operating systems: MS Windows 95/98/Me and MS Windows NT4.0/2000/XP.
To install the program, first call up the program "setup.exe" from the directory \SurveyOffice\ English\Disk1\ on the CD-ROM, and carry out the instructions given. For further information, refer to the handbook or to the on-line help provided by your operating system.
Range of programs
After the installation is complete, the following programs are available:
Data Exchange Manager:
Exchange of data between the instrument and the PC.
Codelists Manager:
Creates code lists.
Software Upload:
Loading and deleting systems software, applications programs, systems texts and applications texts.
Coordinate Editor:
Editing of coordinates.
Optionally, additional programs can be installed.
For additional information about Leica Survey Office, please refer to the comprehensive on-line help.
Description of the system
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Batteries and chargers
GEB111
GEB121
Your Leica Geosystems instrument is powered by rechargeable battery modules. The Pro battery (GEB121) is recommended for the TPS1100 Professional Series. The basic battery (GEB111) is an optional alter­native.
Use only the Leica Geosy­stems batteries, chargers and accessories, or accessories recommended by Leica Geo­systems.
Vehicle battery cable
Power cable
Charging cable Adapter plate
1100Z06
GDI121
Charger GKL122
The Professional charger (GKL122) will charge up to four batteries, either from a 230V or 115V power source using a power plug or from the 12V or 24V source provided by the cigarette lighter in a vehicle. At any one time, either two Pro / Basic batteries can be charged or, by using the adapter plate (GDI121), four Pro / Basic batteries.
Charger GKL23
Adapter plate
1100Z07
GDI121
The adapter plate GDI121 can be connected to the Pro charger (GKL122) or to the GKL23 charger, and enables two Pro / Basic batteries to be charged simultaneously.
6
10
1100Z08
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Description of the system
Page 22
Preparation, setting up
6
0
2
Unpacking
Take the instrument out of the transport container and check that it is complete:
1
1100Z09B
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
1 PC cable (optional) 2 Eyepiece for steep sights / Zenith
eyepiece (optional)
3 Counterweight for eyepiece for
steep sights (optional) 4 Charger GKL111 (optional) 5 PC card (optional) 6 Pocket knife (optional) 7 Auxiliary lens (optional) 8 Spare battery (optional) 9 Power plug for GKL111 (optional)
10 Spacing bracket (optional)
11 Height meter (optional) 12 Mini prism rod (optional) 13 Tool set, comprising 2 adjusting
pins, 1 Allen key each for adjusting
bull's-eye bubble and EDM. 14 Instrument 15 Mini prism + holder (optional) 16 Short instructions/ target plate
(only for reflectorless measuring
instruments) 17 Protective cover, sunshade 18 Tip for mini prism (optional)
Preparing to measure, setting up
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Charging the battery
Charger GKL111
The battery chargers GKL111 or GKL122 are used to charge the batteries. Please refer to the corresponding battery charger user manual for more information.
Charger GKL122
Adapter plate
1100Z10
GDI121
WARNING:
The battery chargers are
intended for indoor use only. Use the battery charger in a dry room only, never outdoors. Charge batteries in an ambient temperature between 0°C and 35°C ( 32°F to 95°F ). We recommend a temperature of 0°C to +20°C (32°F to 68°F) for storing the batteries.
1100Z07
To attain full battery capacitance, it is essential to subject new GEB111 / GEB121 batteries to between three and five complete charge/discharge cycles.
6
10
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Preparing to measure, setting up
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Inserting / replacing battery
6
Insert battery correctly (note pole markings on the inside
0
2
1. Remove battery holder.
1100Z481100Z49
3. Insert battery into battery holder.
1100Z50
1100Z12
of the battery cover). Check and insert battery holder true to side into the housing.
2. Remove battery and replace. 4. Insert battery holder into instrument.
Preparing to measure, setting up
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External power supply for total station
To meet the conditions stipulated for electromagnetic acceptability when powering the TPS1100 from an external source, the supply cable used must be equipped with a ferrite core.
The Lemo plug with the ferrite core always has to be
attached at the instrument side.
The cables supplied along with your instrument include a ferrite core as standard. If you are using older cables without ferrite core, it's necessary to attach ferrite cores to the cable. If you need additional ferrite cores, please contact your local Leica Geo­systems agency. The spare-part number of the ferrite core is 703 707.
1100Z57
6
10
12
1100Z58
For assembling open up one ferrite core and clip it around the supply cable, about 2cm away from the Lemo plug, before using the supply cable for the first time together with a TPS1100 instrument.
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25
Preparing to measure, setting up
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Insert PC-card
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2
1
5
4
2
3
1. Open PC-card housing.
1100Z51
2. Insert PC-card with TPS- arrow
1100Z52
3. Closing PC-card housing.
1100Z53
symbol facing up.
When closing the PC-card housing the connector
must face upwards!!
Preparing to measure, setting up
26
TPS1100 - User Manual 2.2.1en
Page 27
Setting up the instrument with optical plummet or laser plummet
1
1
2
1
2
5/8"-thread
Tribrach GDF121 or GDF122
Tripod GST120
2
3
6
6
10
12
4
4
4
1. Target the ground point or activate
the laser plummet.
2. Set up the GST20, centring it as
well as possible.
The laser plummet is built into the vertical axis of the TPS1100 instruments. Projecting a red dot on to the ground makes it appreciably easier to centre the instrument.
TPS1100 - User Manual 2.2.1en
1100Z13
3. Using the footscrews of the tribrach, centre the plummet to the ground point.
4. Move the legs of the tripod to centre the bull’s-eye bubble.
The laser plummet cannot be used in conjunction with a tribrach which already has an optical plummet.
27
1100Z14
5. Level-up precisely, using the electronic bubble (see the chapter
"Levelling-up with the electronic bubble").
6. Centre precisely by shifting the tribrach on the tripod plate.
Repeat steps 5 and 6 until the required accuracy is reached.
Preparing to measure, setting up
1100Z15
Page 28
Levelling-up with the electronic bubble
Elect. Level
Tilt L : -0°03'40" Tilt T : -0°18'30"
L.Plumet : 50% X
MC
Elect. Level
Tilt L : -0°00'10" Tilt T : -0°00'20"
L.Plumet : 50% X
MC
6
0
2
longitudinal and transverse tilt of the instrument’s vertical axis. The current settings of the laser plummet are indicated numerically as a percentage.
Graphical and numerical display of the
CONT L.Pl+
Switches the laser plummet on or off.
Varies the intensity of the laser dot.
QUIT
Using the footscrews, the instrument can be levelled-up without having to turn it through 90° (100 gon) or 180° (200 gon). In the display which is closest to the bull's-eye bubble, the movement of the small circle runs parallel to the movement of the bubble in the alidade. The other display shows the movement in the opposite direction.
When the bubble is centred, the TPS1100 has been perfectly levelled up.
CONT L.Pl+
QUIT
Preparing to measure, setting up
28
TPS1100 - User Manual 2.2.1en
Page 29
Checking and adjusting
Electronically
All instruments basically have inherent mechanical defects which can affect the measurement of angles. The electronic angle­measuring system of the TPS1100 routinely corrects the mechanical instrument errors listed below; the vertical angles relate to the plumb line and the horizontal measurements are corrected for line-of-sight error, for tilting-axis error and for vertical­axis tilt:
• l, t Compensator index error
• i Vertical-index error
• c Line-of-sight error
• a Tilting-axis error
• ATR ATR zero-point error (only for TCA and TCRA versions)
The instrument errors listed on the left can change over time and with temperature.
They should, therefore, be redetermined in the order shown below:
• before the first use
• before each precision survey
• after long periods of transport
• after long periods of work
• if the temperature alters by more than 20°C
Before determining the instrument errors, level-up the instrument using the electronic bubble. The instrument should be secure and firm, and should be protected from direct sunlight in order to avoid thermal warming on one side only.
Take note that the procedure
for determining the relevant instrument error has to be followed precisely and carefully.
The determination of the
instrument errors can be started in any telescope face.
Immediately after the first
measurement has been completed, motorized instruments change automatically to the second face, after which the user merely needs to carry out the fine pointing.
6
10
12
21
TPS1100 - User Manual 2.2.1en
29
Checking and adjusting
Page 30
Electronic checking and adjusting, continued
Main\ Instr. calibration
current l Compens.long.: 0°00'37" t Compens.trans: -0°00'34" i V-index error: 0°00'28" c Hz-coll.error: 0°00'20" a Tilting-axis : 0°00'26"
MC
6
Activating the "Instrument calibration" function.
0
2
l,t i c/a i/c/a ATR + EXIT
LOGF+ QUIT
Determines the compensator index error. Simultaneous adjustment of the electronic bubble.
Determines the index error for the vertical circle (V-index error).
Defines line-of-sight errors and, if required, tilting-axis errors.
Checking and adjusting
Joint determination of the V­index errors, line-of-sight errors and, if required, tilting­axis errors.
Determines the collimation error of the ATR (TCA and TCRA versions only).
Enables the calibration Log-file (see next
page).
30
The instrument errors reported are displayed in the sense of an error. When measurements are being corrected, they are used in the sense of corrections and have the opposite sign to the error.
TPS1100 - User Manual 2.2.1en
Page 31
Electronic checking and adjusting, continued
Calibration Log-File
If the Log-File is enabled [LOGF+], the measurements and results of the calibration are stored in an ASCII-file. This file is created in the directory LOG on the memory card. Subsequently, you can read the memory card on your PC and obtain a hard copy of the Log-file.
New data is always appended to the calibration
Log-file.
TPS1100 - Instrument Calibration Instrument : TCRA1102plusSerial 619216
Compensator Index Error l,t Date/Time : 03/04/2000 15:43
Old values : l= 0.0000g t= 0.0000g Measurements
L= -0.0126g T= 0.0298g L= 0.0368g T= 0.0164g
New values : l= 0.0010g t= 0.0023g
Vertical Index Error i Date/Time : 03/04/2000 15:45
Old value : i= 0.0000g Measurements
Hz= 377.0597 g V= 104.2828 g Hz= 177.0562 g V= 295.7176 g
New value : i= 0.0001g
Example of a Calibration Log-file (here compensator and vertical index errors)
6
10
12
21
TPS1100 - User Manual 2.2.1en
31
Checking and adjusting
Page 32
Compensator (electronic bubble)
Main\ Compens.Index Error
1st tilt measurement in any face
L Compens.: 0°00'25" T Compens.: 0°00'04"
MC
6
Vertical axis
0
2
The determination of the index error for the longitudinal and transverse axes of the compensator ( l, t ) corresponds to the determination of the centre of the bubble used in the level.
The instrument should be set up away from warmth coming from one side some
time before the calibration so that it can adjust to the ambient temperature.The index error for the longitudinal and transverse axes is determined at the factory and adjusted to zero before delivery.
Checking and adjusting
Activate the calibration procedure. (Refer to display
on page 30)
If the tilt cannot be measured, e.g. due to an unstable instrument, the error message ERROR: 557 is displayed and the following keys are
The longitudinal and transverse axes
l
q
(l, t) are displayed afterwards in the following dialog.
defined:
Repeat measurement.
Abort measurement.
1100Z01
Non-motorized instruments perform the second measurement after the alidade of the instrument has been
MEAS
QUIT
turned 180° (200 gon), with an accuracy of ±4° 30' (±5 gon). After the initial measurement has been started by pressing the key
, motorized instruments will
Initiate the measurement of the longitudinal and
transverse tilt ( l, t ).
automatically complete the determination of l and t without any other assistance. The following dialog is displayed after completing the first tilt measurement with non-motorized instruments.
32
TPS1100 - User Manual 2.2.1en
Page 33
Compensator , continued
Telescope Positioning
Hz- and V-positioning: set direction(s) to zero.
∆ ∆
∆ ∆
Hz : 0°00'00" ∆ ∆
∆ ∆
V : ------
MC
Telescope Positioning
Hz- and V-positioning: set direction(s) to zero.
∆ ∆
∆ ∆
Hz : 180°00'00" ∆ ∆
∆ ∆
V : ------
MC
Main\ Compens.Index Error
new l Comp: 0°03'02" t Comp: -0°02'06"
Accept new value(s)?
MC
After the first measurement of tilt, the menu for non-motorized instruments is the following:
OK ABORT
Turn the instrument through 180° (200 gon) so that Hz = 0° 00' 00" (0.0000 gon).
TPS1100 - User Manual 2.2.1en
OK ABORT
QUIT
If the differences between the hori­zontal and vertical angles lie within ±4° 30' (±5 gon), the display can be
quitted with .
The user is made aware by an acoustic signal that the -key is redefined as "OK".
Activates the second tilt measurement.
Terminates the determination of the compensator indexes.
The following dialog shows the two newly-determined values for the longitudinal and transverse compensator-index errors.
II
33
YES RETRY NO
QUIT
Stores the new values.
Repeats the complete calibration procedure.
Leaves the previous values unchanged.
If the values for the index
errors (l, t) exceed 5' 24" (0.1 gon), the complete calibration procedure repeat, but first check that the instrument is correctly levelled and is free of vibration. If these values are exceeded repeatedly, please notify service.
Checking and adjusting
6
10
12
21
Page 34
V-index error
Main\ V-Index Error
Aim accurately at a target positioned at a dist. >100m
Hz : 343°18'54" V : 93°47'41"
MC
6
0
2
The V-index error is the zero-point error of the vertical encoding circle in relation to the vertical axis of the instrument. The V-index error is set to "0.00" before delivery. All vertical angles are corrected with the V-index error.
The instrument should have adapted to the
against warming from one side.
Checking and adjusting
ambient temperature and should be protected
i
1.
ca. 100m
+/-9°
MEAS
QUIT
1100Z17
To determine the V-index error, aim the telescope at a target about 100m distant. The target must be
1100Z18
Afterwards, the display shows a message asking for the telescope to be turned to the other face.
Starts the measurement for the vertical circle.
positioned within ±9° (±10 gon) of the horizontal plane.
2.
Activate the calibration procedure (Refer to display
180°
on page 30). The two-axis compensator is turned off automatically when determining the
180°
V-index error.
This fact is shown by the symbol.
34
TPS1100 - User Manual 2.2.1en
1100Z19
Page 35
V-index error , continued
Main\ V-Index Error
old new i Vind: 0°00'03" -0°00'22"
Accept new value(s)?
MC
Telescope Positioning
Hz- and V-positioning: Set direction(s) to zero.
∆ ∆
∆ ∆
Hz : 0°00'00" ∆ ∆
∆ ∆
V : 0°00'00"
MC
Main\ V-Index Error
Aim accurately at the same target in other face
Hz : 163°18'54" V : 266°12'19"
MC
If the differences between the hori­zontal and vertical angles do not exceed ±27' ( ±0.5 gon ), the display shows that the instrument is ready to measure. The user is made aware by an acoustic signal that the key is redefined as 'OK'.
OK ABORT
Confirms the readiness to measure and changes the display.
TPS1100 - User Manual 2.2.1en
QUIT
MEAS
QUIT
Sight the target accurately again.
Starts the second measurement.
After the measurements are complete, the older and newly-determined V­index errors are displayed.
35
YES RETRY NO
QUIT
Stores the new values.
Repeats the complete V­index error determination
procedure.
Leaves the old values unchanged.
If the value of the V-index
error (i) exceeds 54' (1 gon) you should repeat the measurement procedure. If this value is exceeded repeatedly, please contact service.
Checking and adjusting
6
10
12
21
Page 36
Line of sight
Main\ Hz-collim. Error
Aim accurately at a target positioned at a dist. >100m
Hz : 373°19'24" V : 90°51'15"
MC
6
The line-of-sight error c is the divergence of the line of sight from a
0
2
line perpendicular to the tilting axis. The line-of-sight error is adjusted and reduced to "0.00" before delivery from the factory. Horizontal angles are only corrected by this line of sight error when the correction is turned "ON" (setting in accordance with section
"Deactivating the instrument-error correction").
Checking and adjusting
c
Line of
Tiltingaxis
sight
To determine the line-of­sight error, aim the telescope at a target about
100m distant. The target must lie within ±9° (±10 gon) of the horizontal plane. The procedure is analogous to that of determining the V-index error.
Activates the calibration procedure. (Refer to display
on page 30).
The two-axis compensator is turned off automatically when determining the line-of-sight error.
This fact is shown by the symbol.
1100z20
36
MEAS
QUIT
Perform the measurement.
Afterwards, a message in the display prompts you to change telescope face.
If the differences between the hori­zontal and vertical angles do not exceed ±27' ( ±0.5 gon ), the display shows that the instrument is ready to measure. The user is made aware by
an acoustic signal that the key is redefined as "OK".
TPS1100 - User Manual 2.2.1en
Page 37
Line of sight, continued
Main\ Hz-Collim. Error
old new c Hz-c: -0°00'03" 0°00'08"
Accept new value(s)?
MC
Main\ Hz-Collim. Error
MC
Telescope Positioning
Hz- and V-positioning: set direction(s) to zero.
∆∆
∆∆
Hz : 0°00'00" ∆∆
∆∆
V : 0°00'00"
MC
Main\ Hz-collim. Error
Aim accurately at the same target in other face
Hz : 193°19'24" V : 269°08'45"
MC
Confirms readiness for measurement and goes to
the measuring menu.
MEAS
Sight the target accurately.
TPS1100 - User Manual 2.2.1en
Perform the second measurement.
OK ABORT
QUIT
QUIT
After successful completion of the second measurement, the older and the newly-determined line-of-sight errors are displayed.
YES RETRY NO
QUIT
Stores the new values.
Repeats the complete line-of­sight error determination procedure.
Leaves the old values unchanged.
If the value of the line-of-
sight error (c) exceeds 5' 24" (0.1 gon), the collimation error is to be redetermined. If the limit is repeatedly exceeded, please notify service.
37
When the new line-of-sight error has been confirmed, the tilting-axis error can be determined.
Continue to determine the tilting-axis errror?
YES NO
Confirms that the tilting-axis error should also be
determined.
Ends the function and returns to the calibration dialog.
Checking and adjusting
6
10
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21
Page 38
Tilting axis
Main\ Tilting-Axis Error
Aim accur. at high/low target positioned at a dist. > 100m
Hz : 373°19'24" V : 90°51'15"
MC
6
The tilting-axis error a is the deviation of the tilting axis from a line
0
2
perpendicular to the vertical axis. The tilting-axis error is adjusted to "0.00" before delivery. The horizontal angles are only corrected by the tilting axis error when the Hz-correction is turned "ON" (setting in accordance with
section "Deactivating the instrument­error correction").
Vertical axis
Tilting axis
Checking and adjusting
To determine the tilting­axis error, aim the telescope at a target about
100m distant. The target must be positioned at least ±27° (±30 gon) above or beneath the horizontal plane. The two-axis
MEAS
QUIT
compensator is turned off automatically during determination of the tilting-axis error.
This fact is shown by the symbol.
display prompts the user to change
Start measurement. Afterwards, a message in the
telescope face.
If the differences between the hori­zontal and vertical angles do not exceed ±27' (±0.5 gon), the display shows that it is ready to measure. The user is made aware by an
acoustic signal that the key is redefined as "OK".
a
1100Z21
38
TPS1100 - User Manual 2.2.1en
Page 39
Tilting axis, continued
Main\ Tilting-Axis Error
old new
a Tilt: -0°00'03" 0°00'17"
Accept new value(s)?
MC
Telescope Positioning
Hz- and V-positioning: set direction(s) to zero.
∆∆
∆∆
Hz : 0°00'00" ∆∆
∆∆
V : 0°00'00"
MC
Main\ Tilting-Axis Error
Aim accurately at the same target in other face
Hz : 193°19'24" V : 269°08'45"
MC
6
10
Confirms readiness to measure and the display
changes as follows.
TPS1100 - User Manual 2.2.1en
OK ABORT
QUIT
MEAS
QUIT
Sight the target accurately.
Performs the second measurement of the horizon-
tal angle.
After the second measurement has been completed, the old and newly­determined tilting-axis errors (a) are displayed.
39
YES RETRY NO
QUIT
Stores the new values.
Repeats the complete tilting­axis error determination procedure.
Leaves the old values unchanged.
If the value of the tilting axis
error (a) exceeds 5' 24" (0.1 gon), the measurements are to be repeated. If this happens often, please notify service.
Checking and adjusting
12
21
Page 40
Combined error determination
Main\ Compensator
Compensator ON/OFF Hz corrections ON/OFF
compensat.: ON Hz-corr. : ON
MC
Deactivating the instrument-error correction
6
By using the key in the display on page 30, it is possible to
0
determine the errors for vertical index, line of sight and tilting axis (i/c/
2
k) with a single operation.
The V-index and line-of-sight errors can be determined using a common target which does not lie more than ± 9° (± 10 gon) away from the horizon­tal plane. The determination of the tilting-axis error requires a target which lies at least ± 27° (± 30 gon) above or beneath the horizontal plane.
For exact procedural details, please refer to the previous chapters.
Also the mechanical instrument-error correction can be deactivated if the need is to display and record only raw data. To deactivate, set the compensator correction and the horizontal-circle correction to OFF, i.e. the vertical angles relate to the vertical axis and the horizontal corrections are not taken into account.
QUIT
Checking and adjusting
40
TPS1100 - User Manual 2.2.1en
Page 41
ATR collimation
CAL\ ATR Collim. Errors
actual ATR Hz-coll.err: 0°00'05" ATR V-coll.err: 0°00'10"
MC
CAL\ ATR Collim. Errors
Aim accurately at a target positioned at a dist. >100m
Hz : 73°25'36" V : 88°45'14" Determ.c/i: NO
▼▼
▼▼
MC
(Available for TCA and TCRA versions only)
The ATR collimation error is the combined horizontal and vertical an­gular divergence of the line of sight from the axis of the CCD camera. The collimation procedure includes, optionally, the determination of the line-of-sight error and the vertical­index error. The correction for the ATR collimation errors is always applied regardless of the "ON/OFF" status of the Hz­correction setting. (See section
"Deactivating the instrument-error correction").
Hz-component
V-com­ponent
Crosshair
TPS1100 - User Manual 2.2.1en
Centre of prism
To define the ATR collimation error, a prism must be accurately targeted at a distance of about 100 m. The target must lie within ±9° (±10 gon) of the horizontal plane. The procedure is analogous to that of determining the V-index error.
Activates the calibration
procedure (Refer to display on page 30). The ATR target recognition is automatically switched
on. This fact is shown by the symbol. The display shows the
current horizontal and vertical ATR collimation errors.
CONT
1100Z30
41
QUIT
Starts the calibration.
The two-axis compensator is turned off automatically when determining the ATR collimation error.
This fact is shown by the
symbol.
MEAS
QUIT
Sight the prism accurately with the crosshair.
Starts the measuring procedure.
Checking and adjusting
6
10
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21
Page 42
ATR collimation, continued
CAL\ ATR Collim. Errors
Aim accurately at the same target in other face.
Hz : 253°25'36" V : 271°14'46"
MC
6
Toggles between simple and combined error
0
2
determination.
YES = Simultaneous
determination of ATR­collimation error, line-of­sight error and vertical-index error
NO = Only determination of
ATR-collimation
It is advisable to determine
the ATR-collimation error, the line-of-sight error and the vertical­index error at the same time.
Checking and adjusting
Changes face automatically directly after completing the initial measurement.
MEAS
QUIT
Sight the prism accurately with the crosshair.
Performs the second-face measurement of the
collimation errors.
42
If the differences between the hori­zontal and vertical angles exceed ±27' ( ±0.5 gon ), the display gives an error message. The user is made aware of this by an acoustic signal
and the key is redefined as "OK". The measurement procedure can be repeated.
When the second measurement has been taken, the accuracy of ATR and, if previously selected, the accuracy of the index and the line-of­sight errors are displayed.
TPS1100 - User Manual 2.2.1en
Page 43
ATR collimation, continued
CAL\ ATR Accuracy
No. of Meas: 2
σσ
σσ
σATR Hz : 0°00'05" σσ
σσ
σATR V : -0°00'08" σ σ
σ σ
σ i V-Ind. : ----- σ σ
σ σ
σ c Hz-col : -----
Take more measurements?
MC
CAL\ATR Collim. Errors
old new ATR Hz : 0°00'08" 0°00'05" ATR V : 0°00'10" 0°00'09" i V-ind : 0°00'00" 0°00'10" c Hz-c : 0°00'10" 0°00'02" Accept new value(s)?
MC
CONT MORE ABORT
No further repeat measure-
ments are required. The old and the newly-defined ATR-collima­tion errors become optional, and are displayed together with the line-of­sight errors (c) and the V-index errors (i).
The calibration can be
repeated as often as necessary until the required level of accuracy is obtained. The result is the mean of all the measurements taken. It is recommended that at least two measuring sequences be carried out.
will be left intact.
TPS1100 - User Manual 2.2.1en
The calibration process is
interrupted. The old values
YES RETRY NO
Stores the new values.
Repeats the ATR1 error determination procedure.
Leaves the old values unchanged.
43
If the value of the ATR hori-
zontal and vertical collimation errors exceeds 2' 42" (0.05 gon), repeat the measurement procedure. Similarly, if the value of the V-index error (i) exceeds 54' (1 gon) or if the value of the line-of-sight error (c) exceeds 5' 24" (0.1 gon) , the measurements are to be repeated. If these values are often exceeded, please contact service.
Checking and adjusting
6
10
12
21
Page 44
Mechanically
6
0
Tripod
12
Bull's eye bubble on instrument
Bull's eye bubble on the tribrach
2
1100Z23
Level the instrument and then remove it from the tribrach. If the bubble is not centred, adjust it using the adjusting pin in conjunction with the two cross-headed adjustment screws (GDF121 bzw. GDF122). Turning the adjustment screws:
• to the left: the bubble approaches
the screw
• to the right: the bubble goes in the
1100Z24
The connections between timber and metal must always be firm and tight.
• Moderately tighten the Allen screws (2).
• Tighten articulated joints (1) just enough to keep the tripod legs open when you lift the tripod off the ground.
1100z22
Level-up the instrument in advance with the electronic bubble. The bubble must be centred. If it extends beyond the circle, use the adjusting pin supplied to centre it with the adjustment screws.
After adjustment no screw shall be loose.
other direction. After adjustment no screw shall be loose.
Checking and adjusting
44
TPS1100 - User Manual 2.2.1en
Page 45
Optical plummet
Checking by plumb-bob:
Set-up and level the instrument on the tripod. Check the centring sleeve for eccentricity by hanging it in place in various positions, then mark the ground point. Remove the plumb­bob. Check that the crosshairs of the optical plummet intersect at the ground point. The accuracy achievable is about 1mm.
Checking by turning the tribrach Adjustment
1
2
3
120° 120°
1100Z26
1. Level-up the instrument using the
1100Z25
electronic bubble. Mark the ground point. Using a soft, well-sharpened pencil, mark the outline of the tribrach on the tripod plate.
2. Turn the tribrach 120 ° and level­up the instrument, fit it into the outline, and again mark the ground
Use a screwdriver to turn the two set screws alternately by the same small amount in order to centre the crosshairs on the ground point marked.
point.
3. Repeat again in the third position.
If the three points do not coincide, adjust the crosshairs to the centre of the triangle formed by the three ground points.
because any deviation of its line of sight from the vertical axis will result in a centring error.
6
10
12
21
1100Z27
Inspect the optical plummet of the tribrach regularly,
TPS1100 - User Manual 2.2.1en
45
Checking and adjusting
Page 46
Laser plummet
6
0
2
The laser plummet is located in the vertical axis of the instrument.
Under normal conditions of use the laser plummet does not need adjusting. If an adjustment is necessary due to external influences
1100Z28
1
2
360°
Laser dot: Diam. 2.5 mm /
1.5 m the instrument has to be returned to any Leica Geosystems service department.
Inspecting by turning the plummet 360°:
1. Place the instrument on the tripod
and level it up.
2. Switch on the laser plummet and
3 mm / 1.5 m
mark the centre of the red dot.
3. Slowly turn the instrument through
360°, carefully observing the movement of the red laser dot.
Inspection of the laser plummet should be carried out on a bright, smooth and horizonal surface (e.g. a sheet of paper).
If the centre of the laser dot describes a perceptible circular movement or moves more than 3 mm away from the point which was first marked, an adjustment may be required. Inform your nearest Leica Geosystems service workshop.
Depending on brightness and surface, the diameter of the laser dot can vary. At a distance of 1.5 m it will be about 2.5mm. The maximum diameter of the circular movement described by the centre of the laser point should not exceed 3 mm at a distance of 1.5m.
Checking and adjusting
46
TPS1100 - User Manual 2.2.1en
Page 47
Reflector-free EDM
The red laser beam used for measuring without reflector is arranged coaxially with the line of sight of the telescope, and emerges from the objective port. If the instrument is well adjusted, the red measuring beam will coincide with the visual line of sight. External influences such as shock or large temperature fluctuations can displace the red measuring beam relative to the line of sight.
The direction of the beam
should be inspected before precise measurement of distances is attempted, because an excessive deviation of the laser beam from the line of sight can result in imprecise distance measurements.
Inspection
A target plate is provided. Set it up between five and 20 metres away with the grey reflective side facing the instrument. Move the telescope to face II. Switch on the red laser beam by activating the laser-point function. Use the telescope crosshair to align the instrument with the centre of the target plate, and then inspect the position of the red laser dot on the target plate. Generally speaking the red dot cannot be seen through the telescope, so look at the target plate from just above the telescope or from just to the side of it. If the dot illuminates the cross, the achievable adjustment precision has been reached; if it lies outside the limits of the cross, the direction of the beam needs to be adjusted.
If the dot on the more reflective side of the plate is too bright (dazzling), use the white side instead to carry out the inspection.
6
10
12
21
1100Z29
TPS1100 - User Manual 2.2.1en
47
Checking and adjusting
Page 48
Reflector-free EDM, continued
6
0
Adjusting the direction of the beam
Pull the two plugs out from the adjustment ports on the top side of
1100Z31
telescope pointing to the target plate.
Throughout the adjustment procedure, keep the
the telescope housing.
2
To correct the height of the beam, insert the screwdriver into the rear adjustment port and turn it clockwise
After each adjustment, replace the plugs in the ports
to keep out damp and dirt.
(dot on target plate moves obliquely upwards) or anticlockwise (dot moves obliquely downwards). To correct the beam laterally, insert the screwdriver into the front adjustment port and turn it clockwise (dot moves to the right) or anticlockwise (dot moves to the left).
1100Z32
Checking and adjusting
48
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Page 49
System functions
\Selection ( )
Meas Job DEFAULT.GSI PC-Card RS232 RS232
MC
Data configuration
This section describes the system functions of the TPS1100 instruments. The presentation of the dialogs, and the sequence and names of the individual functions, are in accordance with the basic TPS1100 configuration.
Data job (D JOB) and meas. job (M JOB)
A distinction is made between:
• Input data, which are generally fixed-point coordinates, and
• Output data, which are generally measurements, coordinates, or values derived from "new points."
It is useful to store the input data and the output data in two separate files, although they can be stored together in one file.
Up to 60 files can be managed. The names of the files can be chosen freely, but the extension must always be GSI (e.g. "PROJ2563.GSI").
In the directory \LOG, additional data from most of the loadable applications can be stored in a protocol file.
The data can be output in GSI format to the serial interface instead of on to the PC card.
If the data is stored on the
serial interface, no data from the applications will be output to the protocol file. Fixed-point coordinates can be read only from the PC card.
The following dialog (e.g. measurement file) can be basically used to create, edit and delete files.
CONT NEW EDIT DEL
|<<-- -->>| QUIT
αα
αNUM
αα
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Creating a new job (NEW)
\ Create new job
Device : PC-Card REC format : GSI Job name : 12345678
MC
CodelistData job (D JOB) and meas. job (M JOB), cont.
Selects the file required.
Creates new measurement file (see dialog opposite).
Displays and edits files.
Deletes file.
Jumps to the first file in
the list. This key is not assigned if the file displayed is already at the beginning of the list.
Jumps to the last file in
the list. This key is not assigned if the file displayed is already at the end of the list.
CONT
Creates a new file having the file name which was entered.
QUIT
This function enables to create a standard codelist. Existing standard codelists, point codelists and mixed codelists can be edited, deleted and copied. For the instrument to recognize the codelist and to access it, the codelist must be saved under the name *.CRF in the "CODE" directory.
The assignations of the keys, and the subsequent course of the program, are the same as in the dialog "Meas. job", with the exception of the additio-
nal function on (COPY).
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Creating a new codelist (NEW)
\ New Codelist
Name of the new codelist Name : 12345678
Device : Internal
MC
\ Copy codelist
Codelist : 12345678
From : PC-Card To : Internal
MC
\ File & Pt.Selection
Rec.device : PC-Card Mem. size : 511.5 KB Free : 193,0 KB PtId/Code : 100 File :FILE01.GSI A: File size : 4.0 KB
MC
Copying a codelist (COPY)
Data management
Only so-called "standard codelists" can be created on the instrument.
CONT
Creates a codelist with the file name entered.
TPS1100 - User Manual 2.2.1en
QUIT
This function enables a codelist to be copied from one data carrier to another.
CONT
QUIT
Display of the selected codelist, the "source data carrier" and the "target data carrier".
Copies the codelist.
51
The following three general dialogs are also then reused in the descriptions of the functions "OPEN", "VIEW", "SEARC" and "INPUT".
Selecting and searching for file / point
SEARCH INPUT VIEW
QUIT
Selecting the file name and entering the search criterion and the complete point number or code number.
Starts a search in the current file.
Enters the coordinates.
Displays the data found.
System functions
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\ Data View and Edit
1/20 Point ID : 1 East : 0.000 m North : 0.000 m Elev. : 0.000 m
MC
Data management, continued
Display of point data found
CONT NEW S <-- --> <<REP REP>>
INS-C |<<- ->>| DEL QUIT
In the first line, the bar provides a graphical representation of the position of the point within the complete file. There follows the running number, and then the total number of data sets within the file.
Transfers the displayed values to the appropriate
function or application.
Starts a search for new points. Jumps to the display
"File & Pt. Selection".
beginning of the file.
System functions
Displays the points in a sequence going towards the
Displays the points in a sequence going towards the
end of the file.
Repeats the search for the
point number, going towards the beginning of the file, in order to find points stored more than once with the same point number or with wild cards (placeholders).
Repeats the search for the
point number, going towards the beginning of the file, in order to find points stored more than once with the same point number or with wild cards (placeholders).
Inserts a codeblock
(Code, Info1…8) in the active file before the displayed measurements.
Jumps to the first block
in the file. This key is not assigned if the first data set is already displayed.
52
Jumps to the last block
in the file. This key is not assigned if the last data set is already displayed.
Deletes the displayed
data.
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\ Data View and Edit
17/20 Point Id : 17 Hz :286°12'36" V :275°45'12" Slope Dist : 123.236m ppm tot/mm : +0051+000
MC
Data management, continued
Importing point data (IMPOR)
Number of GSI data found
CONT NEW S <-- --> <<REP REP>>
|<<- ->>| DEL QUIT
The data is displayed point by point in accordance with the recording mask in use at the time of the storage. The data displayed can therefore change from one point to another. The assignations of the keys, and the subsequent course of the program, are the same as in the dialog "Data View and Edit", with the exception of the following function:
TPS1100 - User Manual 2.2.1en
Deletes the displayed
data block from the file. A message is called to confirm that you want to delete the block.
53
This function searches in the current data job for the coordinates of the point required. It accepts the first data set found after the start of the file, but does not display this data set.
If no point data are found, a message is displayed along with the note that no points with this point number were found. With "NEW S", the dialog "File & Pt. Selection" is called. The file for the data search can be changed and/or a new point number can be entered.
Or:
The missing data can be entered with "INPUT".
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Displaying and importing point data (VIEW)
Displaying and editing GSI data (SEARC)
This function searches in the current data job for the coordinates of the required point. The first data set found after the beginning of the file is the one accepted. The data set found is displayed in every case.
If point data are found, refer to the dialog "Data View and Edit". "CONT" accepts the values displayed, and terminates the function.
Or:
Using "NEW S", call the dialog "File & Pt. Selection". The file for the data search can be changed and/or a new point number can be entered.
If no point data is found, a message appears with the note that no points with this point number were found.
Using "NEW S", call the dialog "File & Pt. Selection". The file for the data search can be changed and/or a new point number can be entered.
Or:
Using "INPUT", enter the missing data.
This function searches in the current measurement file for data relating to the required point. The user has the option of displaying the data stored on the PC-card within a chosen file and to delete data blocks. Individual points, and multiple entries of points with the same point number, can be searched for, displayed and deleted. The last point number in the file is displayed automatically. If editing of the data is permitted, point numbers, code information, attributes, instrument height and reflector height can all be changed. True measurement data such as directions and distances cannot be changed.
To activate the dialog "File & Pt. Selection", refer to the appropriate dialog.
System functions
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Displaying GSI data, continued
Input Results Remarks
11.
11, 110, 1101, 11 ABC 5, 111111
After 11 there can be any character and in any amount.
.11 11 , ABC 11, 11111
Before 11 there can be any character in any amount.
1.0 10, 100, 1ABCD0, 11111110
Between 1 and 0 there can be any character and in any amount.
.10.
10, 3410ABC, 111110, 1000000
A 10 must be present at least once
.1.0.
10, 341ABC0, 1123Z0Y, 1001A000
A 1 must be present in frount of a 0 at least once, and any amount of characters can be present between them.
Placeholder (wild cards) in searching for points
If no point or code is found, a message is displayed along with the note that no point or code was found in the current measurement file.
The search for stored data can be made easier if a placeholder is used instead of the complete point number. In the TPS1000, a decimal point "." is used instead of the more usual star "*", because it is more easily entered. There is no entry corresponding to "?".
If a point or code is found, refer to the dialog "Data View and Edit".
TPS1100 - User Manual 2.2.1en
Example of the use of placeholders:
If a number with placeholder is entered instead of the complete point number, the controlled data search is always started and the first matching data set is displayed. The subsequent procedure is the same as that used when entering a complete point number.
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Manual input of coordinates (INPUT)
\ Enter coordinate set
Data Job : papillon.gsi Enter min. : PointId+E+N Indiv.PtId : 1 East : 0.000 m North : 0.000 m Elev. : 0.000 m
MC
Converting data
This function enables point coordinates to be entered and stored in the current data file.
CONT REC
Transfers the displayed values to the calling function.
Sets the point data and
stores them in the data file. The height is stored only if a value has been entered.
System functions
QUIT
This function permits the conversion of coordinates (P, E, N, (H)).
Three different file formats are supported:
• GSI (Leica Geosystems standard format) = *.GSI
• ASCII (normal ASCII text files) = *.ASC
• TDS (Tripod Data Systems) = *.CR5
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After the function has been called, the dialog shown on the next page appears, permitting rapid selection of the original file and its format and also input of the name of the target file (output file) and its format.
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Main\ File Selection
Source Path : A:\DATA\ Source File : PAPILLON.CR5 Format : TDS sequent. Output Path : A:\GSI Output File : PAPILLON.GSI Format : GSI 16
MC
Converting data, continued
CONV\ Configuration
Source file settings Search extens. : ASC Header lines : 0
Output file settings Default extens : GSI
MC
Conversion dialog
GO CONF
QUIT
Source Path
Selects the directory for the source file.
Source File
Selects the name of the source file.
Format
Selects the file format. There is a choice between the following formats: GS18, GSI16, ASCII, TDS sequential, TDS non-sequential.
Output Path
Selects the directory for the output file.
Output File
Enters the name of the output file.
Format
Selects the file format.
Starts the conversion.
Calls up the configuration.
Configuration dialog
OK ASCII
Decimals : As System
QUIT
Source file settings Search extens.
Determines the file extension to be searched for.
Header lines
Determines the number of lines to be jumped at the beginning of a source file, i.e. which should not be converted (range of values 0-999).
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Converting data, continued
CONV\ ASCII File Format
Separator : Space Id Pos : 1 East Pos : 2 North Pos : 3 Height Pos : 4 Pt. Code Pos: 5
MC
Configuration dialog (continued)
Settings for output file Search extens.
Determines the extension for the output file.
Decimals
Determines the number of decimal places in the output if this is not limited by the format (e.g. by GSI). Choice between "As System" and up to six decimal places.
Returns to conversion dialog.
Calls the ASCII ­configuration dialog.
ASCII configuration dialog
The ASCII file format can be defined in the ASCII configuration dialog. The defined format is valid for ASCII source files and ASCII output files.
OK DEFLT
Attrib 1 Pos: 6 Attrib 2 Pos: 7
QUIT
Separator
Determines the separator between the data during output. Spacing, commas and tabulator can be set.
PtId, East, North,... Position
The position in the ASCII format has to be defined for each component ("None" or 1,..,10 can be set).
Reset to the default settings (as shown above).
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CONV\ CONVERSION
Completed!
Points converted : 135 Lines not converted: 12
MC
Converting data, continued Formatting the PC-card (FORMT)
\Format PC-Card
WARNING: 1151
Formatting deletes all data on the PC-Card.
MC
\ Format PC-Card
Formatting finished.
Memory space of PC-card Card type : SRAM Total : 523776 Byte Free : 509952 Byte
MC
Closing dialog
The closing dialog indicates the end of the conversion and shows the user how many lines were converted and how many not.
NEW QUIT
Points converted
Output of the number of successfully­converted points.
Lines not converted
Output of the number of lines not converted.
Starts new conversion and
TPS1100 - User Manual 2.2.1en
calls the conversion dialog.
Quits the function.
QUIT
OK ABORT
Formatting the PC-card irretrievably deletes all data.
Confirms the formatting is to
go ahead. The storage capacity of the PC-card is ascertained and the card is formatted accordingly.
Aborts the function "Format
PC-Card".
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OK
QUIT
After the formatting is complete, the total memory capacity and the memory available on the card are displayed. The difference between the total memory capacity and the available memory is used for managing the directories.
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\ REC-Mask Definition
Define : Rec-Mask 1 Mask name : Polar REC format : GSI16(16 char) 1st word : Point Id (11) 2nd word : Hz (21) 3rd word : V (22)
MC
Inspecting the PC-card (PROOF)
\ Check PC-Card
Card type : ATA-Flash Card name : TPS-1100 Total : 523776 Byte Free : 509952 Byte Status : Not protected Card.Batt : Good
MC
CONT
Display of the type of card (SRAM or ATA-Flash).
Display of the total memory capacity and the available memory.
Display of the write-protection function: NOT PROTECTED or PROTECTED.
Display of the battery status (only for SRAM cards): GOOD or LOW. (If LOW appears, fit a new internal battery for the PC-card immediately).
System functions
QUIT
Setting the recording mask (RMask)
Activates the function "REC-Mask Definition".
Five REC masks can be defined for recording measurement data, and one REC mask for setting the station data.
The first line (point number) cannot be changed. For the remaining 11 lines, the data to be recorded can be selected from a list.
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CONT DEFLT
4th word : Slope Dist.(31) 5th word : East 6th word : North 7th word : Elev. (83) 8th word :ppm tot/mm (51) 9th word : (empty) 10th word : (empty) 11th word : (empty) 12th word : (empty)
QUIT
Sets the current REC mask to "Standard", i.e. to the REC
masks originally defined.
In contrast to the display mask, the parameters in the recording template can be set only once.
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Setting the recording mask (RMask), cont.
\Displ.mask definition
Define : Displ.Mask 1 Mask name : Standard 1 1st word : Point Id 2nd word : Hz 3rd word : V 4th word : Slope Dist.
MC
Setting the display mask (DMask)
If Point Codes and Attributes
need to be stored , it must be defined in the recording mask. If attributes are defined in the display mask, they can directly be entered in the measuring dialog.
The standard REC masks
are different from the standard display mask. The REC mask does not include the reflector height, for example. If the heights of targets are to be inspected in the office, the attribute "Refl. Height" must be added to the recording mask.
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Activates the function from the "DIS­PLAY MASK" dialog.
Three DSP masks can be defined.
The 12 lines can be set up by using the parameters available from the lists.
CONT DEFLT
5th word : Horiz.Dist 6th word : Elev.Diff. 7th word : East 8th word : North 9th word : Elev. 10th word : ppm/mm 11th word : (empty) 12th word : (empty)
QUIT
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Each line can display any and all of the available display data.
Sets the current DSP mask to "Standard", i.e. to the DSP
masks originally defined.
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GSI-parameters
Complete list of display and recording parameters
(*) = only on the record screen
WI-No. Parameters Description
-- \empty Empty line
-- Displ.Mask Current display mask
(*) 58 Add.const. Prism constant
-- Backs. Id Current backsight Id
(*) 72 (*) 73 (*) 74 (*) 75 (*) 76 (*) 77 (*) 78 (*) 79
-- AVG n max. Maximum number of distance measurements in the averaging mode
41 Code Code blocks serve to record additional information used in further processing of the measurement data. The codes are
-- Code Mngmt Codelist managment: view, select, create, edit
-- Code Descr Description for the current code
-- Codelist View and select Codelist
-- Data job View and select Data-Job
-- Date Current date
-- DJob Mngmt Data-Job management: view, select, create, edit
Attrib. 1 Attrib. 2 Attrib. 3 Attrib. 4 Attrib. 5 Attrib. 6 Attrib. 7 Attrib. 8
Attributes (1-8) can be used to store additional information in the field. Each of the editable parameters can contain up to 8 or 16 alphanumeric characters. Contrary to CODE-words, Point codes and Attributes are stored within the measurement data block, as long as the record mask contains attributes.
stored in blocks separate from the measurement data blocks and contain at least one CODE-word and up to87 more information words (Info 1 to 8).
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GSI-parameters, continued
WI-No. Parameters Description
-- Offs. Elev. Elevation offset of target point
-- Offs. Lngth Length offset of target point
-- Offs.Cross Cross offset of target point
-- Offs.Mode View and select offset mode, reset after REC or keep
-- Half line space Half empty line
(*) 32 Horiz.dist. Horizontal distance (reduced slope distance)
(*) 21
(*) 83
(*) 33 Elev.Diff. Height difference between the station point and the target point with allowance made for the instrument and reflector
(*) (11) Indiv.PtId Current individual point number
42 43 44 45 46 47 48 49
-- Increment Increment to encrease the running point id
(*) 88
(*) (11) Runn.PtId Current running point id
-- Meas job View and select Meas-Job
-- EDM Prog. View and select EDM program
-- MJob Mngmt Meas-Job management: view, select, create, edit
(*) 52 n / s Number of averaged distances measured and the standard deviation in millimetre
(*) 82 North North coordinate of target point
Hz Horizontal direction
Elev. Target point height (Z)
hei ghts
Inf o 1 Inf o 2 Inf o 3 Inf o 4 Inf o 5 Inf o 6 Inf o 7 Inf o 8
Inst.Ht
Additional information to the Code. Each of these editable information words can contain up to 8 or 16 alphanumeric characters.
Ins tr ument
hei ght
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GSI-parameters, continued
WI-Nr. Parameters Description
(*) 81 East East coordinate of traget point
-- pp m atm. Atmospheric ppm value
-- ppm geom. Geometric ppm value
(*) 59 ppm total Total ppm-correction
(*) 51 ppm/mm Total ppm-correction and prism constant
-- PtC.Descr. Description for the current Code
(*) 71 Point Code Current Point Code
(*) 11 Point Id Current Point Id (either the running or the individual poi nt id)
(*) 87 Refl. Ht. Reflector height
-- Refl. list View and select a reflector
-- Refl.Name Display the current reflector name
-- Displ.Mask View and select the recording mask
(*) 31 Slope Dist Measured slope distance (already corrected using ppm and prism constant)
-- S tation Id Stati on p oi nt numb er
(*) 86 Stn.Elev.
(*) 85 Stn.North Station northing coordinate (Xo)
(*) 84
(*) 22 V Vertical angle
-- V-Display View and select the V angle display
-- Last PtId Display of the last recorded Point Id
-- Prev.Code Display of the last recorded Code
-- Prev.PtCod Display of the last recorded Point Code
-- Time Current system-time
-- Target Typ Current target type, reflector or none
Stn.East Station easting coordinate (Yo)
Station Elevation (Zo)
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GSI-parameters, continued
DMask Coord. Seq.
Display in
measurement
mode
Change
Easting/Northing E/N as in DMask Easting/Northing none
Easting /No rthi ng change E/N S eq . Northing/Easting yes
Northing/Easting E/N as in DMask Northing/Easting none
Northi ng/Easti ng change E/N S eq . E asting/Northing yes
Display and recording
parameters can be defined independently. Therefore make sure that the recording mask contains all parameters necessary for evaluation.
display mask and if the coordinate display shows "Easting/Northing" then also the Easting value followed by the Northing value appears in the measurement mode. However, in connection with the display mask and the display in the measurement mode four cases must be considered:
If values "East" and then "North" are defined in the
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\Quick station setup
Station Id : 1 Backs. Id : A Inst. Ht. : 1.500 m Refl. Ht. : 1.000 m
∆∆
∆∆
HorizDist : ----- m
Measure to Backs.point
MC
MAIN\Quick station setup
Station Id : 1 Inst. Ht. : 1.600 Stn.East : 726530.424 m Stn.North : 256431.871 m Stn.Elev. : 459.173 m Set Station with REC or CONT
MC
Measurement functions
Single-point orientation (quick station setup)
This function brings together in a sin­gle dialog all of the relevant inputs needed to set up the instrument from scratch. Activate the function "Quick-station setup (QSET)".
DIST CONT INPUT
ALL REC I<>II VIEW QUIT
Enter the numbers of the station point and of the backsight point respectively. The appropriate point is immediately searched for in the data file and, if the search is successful, the coordinates will be assigned to the station point and backsight point without this fact being displayed.
System functions
After the instrument height and the reflector height have been entered, target the backsight point and measure the distance and/or the direction.
Measure the distance. The
difference between the calculated distance and the measured distance to the backsight point is displayed.
Determine the direction, but
do not store the values. The graduated circle is orientated.
Using the keyboard, enter the
coordinates for the station or for the tie point. See chapter "Data management".
Measure the distance
and determine the direction, and store the measurement block. The graduated circle is orientated. The difference between the calculated distance and the measured distance to the backsight point is displayed.
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Determine the direction
and store it, including the previously-measured distance where appropriate. The graduated circle is orientated.
Activate controlled data
search within data file. See chapter "Data management".
REC CONT
QUIT
Station data are set.
Station data are set and are stored in the measurement
file.
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Setting and entering the Hz direction (SetHz)
\ Set Hz to any angle
Set Hz-direction
Hz :123°17'56"
MC
\ Distance Meas.
EDM Prog. : Standard IR Refl.Name : Leica 360° prism
Add.const. : 23.1 mm ppm total : 0.0
MC
Distance measurement
Activate the function "Set Hz to any angle". Target the tie point exactly. The direction must always be set using face I.
Set Hz direction to 0° 00' 00" (0.0000 gon) or enter a known value.
SET Hz=0 HOLD
Sets Hz to 0° 00' 00" (0.0000 gon).
QUIT
Instead of entering a value, this can be set by turning the instrument.
Secures the value (clamp the circle)
Target the tie point exactly.
Releases the circle.
This function is also activated from other dialogs
in order to enter the Hz direction.
The following dialog is displayed during the "first" distance measurement:
->Ref ->TRK TEST STOP EDM-P
QUIT
The display shows the current measuring program and reflector, the current additive constant (prism constant) and the total ppm value.
Switches between infrared (with reflector, !REF) and
red laser (no reflector, RL).
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Distance measurement, continued Selecting the EDM measuring program, target type and reflector
\ EDM parameters
Set EDM Prog for DIST/ALL Target Typ : IR=Reflector EDM Prog. : Standard IR
Refl.Name : Leica circ.prism Add.const.: 0.0 mm
MC
Activates the tracking mode if
the measuring program "Standard distance measurement" was selected, or the rapid-tracking mode if the measuring program "Fast distance measurement" was selected.
Calls the EDM test (signal
and frequency)
Stops the current measuring
program.
Calls the function " EDM
parameters".
System functions
CONT REFL
Infrared:
Standard IR Normal distance measurement. Accuracy 2mm+2ppm. Measuring time 1.0 seconds.
Standard Fast IR Rapid distance measurement. Accuracy 5mm+2ppm. Measuring time 0.5 seconds.
Tracking IR Continuous measurement. Accuracy 5mm+2ppm. Measuring time 0.3 seconds.
Tracking Fast IR Continuous measurement. Accuracy 10mm+2ppm. Measuring time <0.15 seconds.
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QUIT
Average IR Repeat measurements in standard measuring mode with display of the number of distance measurements (2≤n≤999), the current average and the standard deviation for the averaged distance.
Very short distances may
be measured reflectorless in Infrared-mode (e.g. to well reflecting targets like traffic signs). In this case the distances are corrected with the addition constant defined for the active reflector.
Reflector-free and long range: (red laser)
Standard Long RL Normal distance measurement. Accuracy 3mm+2ppm.
Average Long RL Repeat measurements in normal measuring mode
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Selecting the EDM ..., continued
Switch between IR/RL
WARNING: (only for Extended Range Instruments)
Reflector-free: The visible laser beam may only be used within a controlled area (refer to chapter "Safety Directions") and must hit a non reflecting material at the end of its intended path. Long Range to prisms: This mode is only permissible from a distance of 1000 m (3300 ft) from the telescope. No persons may stay within the beam path up to 1000 m (=controlled area; refer to chapter "Safety Directions").
Selecting the target type
This line appears only if a reflectorless instrument is being used. There is a choice between "reflectorless" and "reflector".
Wrong target type setting leads to bad measurements.
Refl.Name
The current reflector is indicated and, on the next line, the additive constant associated with it.
Calls the function "Reflector selection".
Wrong prism setting leads to bad measurements.
[ >REF ] Activates infrared
distance measurement (with reflector). The last used ATR/LOCK settings are simultaneously activated.
[ >RL ] Activates reflectorless
distance measurement.
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\ Reflector Selection
Select reflector type Refl.Name : Leica circ.prism Add.const. : 0.0mm
DEF 1,2,3 for new reflector
MC
Switch between Fast measurement/RapidSwitch between Standard/Tracking
Setting / defining prisms
[ >STD ] Activates standard
distance measurement.
[ >TRK ] Activates distance
tracking.
Tracking
[>RTRK] Activates rapid distance
tracking.
[>FAST] Activates rapid distance
measurement.
Activating the function "Reflector selection".
CONT DEF 1 DEF 2 DEF 3
QUIT
Choosing the appropriate prism. The appropriate additive constant is set automatically at the same time.
Wrong prism setting leads to
bad measurements.
,,
Define reflectors from other manufacturers.
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\ EDM Return Signal
Signal strength
0% 100%
75%
Tone : OFF
▼▼
▼▼
MC
\ ATMOSPHERIC CORR.
Temperature : 12.0 °C Atm. press. :1013.3 mBar Temp.wet-b. : 60.0 % ppm atmospheric : 0.0 ppm geometric : 0.0 ppm total : 0.0
MC
\Define new reflector 1
Define type of reflector Ref.1 Type : Not defined
Ref.1 Name : ----­Ref.1 Cons : ----- mm
MC
Setting / defining prisms, continued
EDM test
Distance corrections, ppm
CONT
The user can freely define the name and additive constant (additive constant) for three reflectors and can enter the type of reflector (prism or retro tape). The additive constant is always given in millimetres [mm]. It is advisable to determine the additive constant for "non Leica Geosystems prisms" on a baseline by means of an appropriate procedure. For the reflector to be available for choice, the reflector type may not be "None".
TPS1100 - User Manual 2.2.1en
QUIT
Displays the signal strength or measurement frequency.
CONT FREQ STOP
QUIT
Toggles between the displays
of measurement frequency and signal strength. The measurement frequency display is similar to the display shown above.
End and return to the
previous dialog.
ON/OFF - key for the acoustic tone. The stronger the signal the more the black intensity bar is extending to the right against 100%. With an already low signal distances can be measured.
71
A distinction is made between atmospheric (ppm) and geometric (ppm) corrections, the sum of which is used as the final distance correction.
Atmospheric correction
The atmospheric distance corrections are derived from the dry­air temperature, air pressure or height over mean sea-level, and rela­tive air humidity or wet-air temperature.
CONT GEOM REFRA P<>E %<>T' ATM=0
QUIT
Settings for the geometrical correction.
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\ GEOMETRIC CORR.
Scale C.M. : 1.0000000 Offset C.M. : 51000 m Height aRef : 350 m Indiv. ppm : 0.0
ppm geometric : -22.9
MC
Distance corrections ppm, continued
Settings for the refraction correction.
Toggle between air pressure and height above mean sea-
level.
Toggle between relative air humidity and wet-air
temperature.
Set the atmospheric ppm to
"0.00". (Individual parameters are set to the standard atmospheric values, corresponding to the atmospheric correction ATM=0)
System functions
Geometrical correction
The geometrical distance correction is derived from the projection distortion and the height above the reference datum. The calculation of the geometrical ppm follows the formula for the Transversal Mercator Projection. The individual factors are: the scale factor of the line of projection (central meridian, Gauss-Krüger = 1.0, UTM = 0.9996, etc.); the offset from the line of projection; the height above the reference datum (normally this is the height above mean sea-level); and an additional individual scale correction.
The distance without any
projection distortion is used to determine the height difference. The individually-set scale adjustment is always applied to the distance.
72
The individual scale correction can be used to enter a total geometrical correction.
CONT GEO=0
ppm ref. level : 0.0 ppm map projection: 0.0
QUIT
Sets the geometrical ppm to
"0.00". The scale on the Central Meridian is set to "1.0000000". The other parameters are set to "0.00".
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\ PPM Corrections
Enter your correction values
Atm.pressure : 1013.3 mbar Temperature : 12.0 °C
ppm total : -0.0
MC
Distance corrections ppm, continued
\ REFRACTION CORR.
Set coeff. of refraction
Correction : ON Refr.coeff. (k) : 0.13
MC
MEAS\ Measurement & Record
Point Id : 1 Attrib. 1 : ----­Refl. Ht. : 1.500 m Hz :286°55'50" V : 91°16'20" Horiz.Dist. : ----- m
MC
Reduced distance corrections ppm
Measurement & recording (REC)
Refraction correction
The refraction correction is taken into account during the calculation of the height difference.
CONT DEFLT
Sets the refraction coefficient to standard values.
TPS1100 - User Manual 2.2.1en
QUIT
For standard applications the distance is corrected only on account of atmospheric influences. The geometrical correction and the projection distortions are set to "0.00". Heights are reduced with the standard refraction coefficient
Activate the function "PPM Atmospheric" from the dialog "Function Selection".
CONT
QUIT
Input of air pressure and temperature or Input of ppm value. The values for pressure and temperature are erased.
73
ALL DIST REC SetHz >DISP
Elev.Diff. : ----- m East : ----- m North : ----- m Elev. : ----- m
INPUT Del B I<>II INDIV QUIT
The data shown above represent the standard display mask.
Measurement block
recording. The recorded measurement-block corresponds to the active recording template. The last measured distance is also recorded.
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Measuring distances and angles separately (DIST + REC)
This procedure offers the option of realigning the telescope on another point after measuring the distance and before measuring the angle. In this way two points can be used for measurements of angle and distance. It is therefore possible to record inaccessible points, e.g. house corners, fences surrounded by hedges.
MEASURING
DISTANCE
STORING DATA
For calculations which depend on distance, the V-angle after completion of the distance measurement is used, along with the current Hz-direction. Consequently, calculated heights and height differences are retained and the coordinates for easting and northing which correspond to the new Hz direction are recalculated using the last-measured distance.
The V-angle displayed corresponds to the position
of the telescope on completion of the
1000QS361000QS37
distance measurement. The V-angle is not altered until the measurement is recorded for a new distance is measured.
When distances, heights, or height differences are displayed as empty fields (i.e. -----), the V-angle is continuously displayed and updated.
If, after the distance has been measured, changes are made to the target-point data which have an influence on the distance measured or on the height and height difference (e.g. ppm, prism constant, reflector height, refraction coefficient), the dependent data will be correspondingly re-computed.
System functions
74
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Page 75
Measuring distances and angles together with storage (ALL)
Storing station data (REC)
Changing face (I<>II)
Hz-angle measurement is carried out after the distance has been measured. Immediately afterwards all data is stored. The measurement block stored in the meas.job corresponds with the active recording mask.
Therefore the instrument
may only be moved after data storage is complete. This is signalled acoustically by the third beep after the ALL key has been pressed.
The data is automatically recorded after the distance has been measured. The distance, and all data which depend on it, are then displayed with the tag "-----", which indicates that the data storage is complete.
The station data (point number, easting, northing, station height, reflector height and instrument height) are recorded in the measurement job. The coordinates are set as station coordinates.
Positioning in the other face. Display of DHz and DV. If the instrument is turned so that these values are at "0.000", the target becomes visible in the telescope again. This aid is an advantage under conditions of poor visibility.
If the instrument is motorized, the
instrument automatically travels to the other face.
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Page 76
Last point number (L.Pt.)
Deleting the GSI block (Del B) Manual distance entry
Enter the last point number to be stored and use it as the current point number.
This function deletes the last GSI block of the current measuring job. With "Del B", a measuring block (starting with WI11) or a code block (starting with WI41) can be deleted.
Enter the horizontal distance, which was measured with a tape for instance. Immediately after confirmation of input, the horizontal distance is shown corrected for the geometrical ppm. After the distance has been entered, the V-angle is set to "hori­zontal" 90° ( 100 gon ) or 270° ( 300 gon ). The coordinates are calculated using the corrected horizontal distance, the Hz-direction, and the V­angle. Heights are always corrected for earth curvature and are corrected for refraction according to the parameter settings.
The reflector height is
temporarily set to the value for the instrument height and so there is always a height difference of "0.000". The slope distance is the same as the horizontal distance.
System functions
76
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Positioning the last point stored (LAST)
V-angle modes
(Applies only to motorized instruments)
The telescope is automatically pointed at the latest point to be stored. This function is available only if a point was stored after switching on the instrument.
[>FREE] This function activates
the vertical angle mode "Running" for the following measurements. In this mode, the vertical angle is continuously updated with the telescope movement.
After a distance
measurement, vertical angle, slope distance, height difference, and the elevation coordinate are displayed as running values. Slope distance, height difference, and the elevation coordinate of the target point are calculated from the initial horizontal distance and currently displayed vertical angle. The REC­function records the displayed values in the measurement file.
[>FIX] This function activates
the vertical angle mode "Hold after DIST" for the following measurements. In this mode, the vertical angle is fixed after a distance measurement, whereas the horizontal angle is running.
Function [VRUN]
This function deletes the last measured distance and so releases the locked vertical angle.
(Available only with special configuration.)
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Page 78
Switching between display masks (>DISP)Offset
The Offset function allows offset points to be determined, for instance when the reflector cannot be set up directly on a point. Transverse, longi­tudinal and/or elevation offsets can be defined from the reflector position to the offset point. All of the displayed and recorded measurement data are calculated in relation to the offset point.
The values for target eccentricity will be retained after storage with the choice of "Permanent" in the Offset Mode. The values will be set to zero with the choice of "No reset after REC".
Offs.Cross -
Offs.Lngth -
Offset PT.
Offs.Cross +
Elev. +:
Offset point is higher than measurement
This function is for switching between the display masks. If no mask is defined, or only one, this function key does not appear.
Offs.Lngth +
1100QS07
System functions
78
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Page 79
Individual point number (INDIV / RUN) Coding
\ Coding (standard)
Code : ----­Info 1 : ----­Info 2 : ----­Info 3 : ----­Info 4 : ----­Info 5 : -----
MC
This function is for switching between the individual [INDIV] and running [RUN] point numbers.
TPS1100 - User Manual 2.2.1en
Standard coding (without codelist)
Code blocks are used to record addi­tional information for subsequent processing of the measurement data. They are recorded in separate blocks and consist of at least the CODE number, along with up to 8 further information blocks (Info 1 to 8). Each of these editable information words contains up to 8 (or 16) alphanumeric characters. Information words which include "----­" are not stored. In general, the code function can be called whenever a measurement or another data set in the measurement file can be stored. The code function, together with the measuring mode, is available in most of the loadable applications.
79
calls up the standard coding
(Code, Info 1 to 8) if no codelist was selected.
REC L Pt.
Info 6 : ----­Info 7 : ----­Info 8 : -----
ENDE
When a new code is entered, or after using the - key,
"REC" is assigned to the - key. Only information-bearing elements
are recorded.
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Page 80
MEAS\ TEST.CRF
〈〉〈〉
〈〉〈〉
〈〉
Code 101 Tree 102 Bush 103 Latern 104 Hydrant
MC
Coding, continued
Standard codes (Code, info 1 to 8) are recorded in separate blocks in GSI format behind the last measurement stored. These codes are not part of the recorded data block (recording template).
Calls the latest codes stored, and also the WIs.
WIs for storage:
Code: WI 41 Info 1 - 8: WI 42 - 49
System functions
Point coding (without codelist)
In the TPS1000 instruments, the so­called "Remarks" (REM words) were used for storing additional information in the measurement-data blocks, but in the TPS1100 they have been replaced by "Point code" and "Attrib. 1-8".
WIs for storing:
Point code: WI 71 Attrib. 1-8: WI 72-79
80
Standard coding with codelist
This function becomes active if a standard codelist has been selected.
The fixed key is used for calling up the codelist.
REC NEW LAST INFO
αα
αNUM
αα
QUIT
Stores the code block.
Creates a new code.
Calls the latest code stored.
Enters information.
Switches between numeric and alphanumeric input for a
rapid search of codes.
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Page 81
Coding, continued
MEAS\ Measurement & Record
MEAS: TEST.CRF < > Code 101 Tree 102 Bush 103 Latern 104 Hydrant
MC
Quick Coding (QCod+ / QCod-)
Point coding with codelist
This function becomes active if a point code list has been selected. In the measurement dialog, the codelist is displayed in the line "point code". The list is opened with direct input or with .
CONT NEW LAST ATRIB
Confirms the selection.
Creates a new point code.
Calls the latest point code.
TPS1100 - User Manual 2.2.1en
Enters attribute values.
αα
αNUM
αα
QUIT
Switches between numeric and alphanumeric input for a
rapid search for codes.
81
This function enables a measurement block and a code block for a predefined code to be stored by pressing a key (Quick-Coding). Up to 100 codes defined in the codelist can be called with the numerical keys in this manner (default 10 codes).
The quick coding can be switched on and off with "QCod+ / QCod-". When quick coding is active, the symbol "C" is displayed in the bottom of the graphical status field of the measurement display. When the quick-coding option is switched off, this symbol disappears.
System functions
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Page 82
Check Orientation
.....\ Check Orientation
Station Id : 1 Backs. Id : BS Refl. Ht. : 1.650 m Azimut : 100.2222 g Hz : 95.6650 g
∆∆
∆∆
Hz : -0.0059 g
MC
The Check Orientation dialog allows to check the orientation to a known backsight point, and to reset the orientation if necessary.
Activating the function "Check Orientation".
CONT DIST POSIT SET VIEW LAST
Horiz Dist : -----
∆∆
HorizDist : -----
∆∆
Elevation : -----
∆∆
Height : -----
∆∆
HELP QUIT
System functions
Enter the Backsight Id. With the appropriate point will immediately be
searched for in the data file and, if the search is successful , the coordinates will be assigned to the backsight point. Additionally the calculated azimuth to the point will be shown.
After the reflector height has been entered, target the backsight point and measure the distance and/or the direction and compare azimuth with HZ.
Leave the dialog and continue work.
Measure distance. Distance
and difference between calculated and measured distance to the backsight point will be shown.
82
Position the telescope to the backsight point. For motorised
instruments only!
The instrument positions automatically back to the start position when leaving the "Check Orientation" function. This is particularly suitable for RCS­applications.
Target the backsight point accurately and reset the
orientation.
Search and display the coordinates of the point found
in the active data job.
If Orientation was set more than once, LAST recalls the
last backsight point and azimuth.
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Page 83
Communication
\ GSI parameters
Baudrate : 2400 Protocol : GSI Parity : Gerade Terminator : CR LF Data Bits : 7 Stop Bit : 1
MC
GSI communication parameters
The setting for the interface parameters is valid for communication with the GSI command structure. The baud rate can be chosen from the standard values between 2400 and 19200.
CONT DEFLT
The standard parameters are shown above.
TPS1100 - User Manual 2.2.1en
QUIT
For more detailed information about command- and data structure, please refer to "WILD Instruments On-Line" (document no. G-366-0en), a copy of which is available (in English only) from your local Leica Geosystems agency.
83
Interface parameters (GeoCOM)
The settings of the interface parameters are valid for communication using the "GeoCOM command structure". The baud rate can be chosen from a list of standard values between 2400 and 19200. All other parameters are fixed and cannot be changed.
For more detailed information about command- and data-structure, please refer to the handbook "GeoCOM Reference Manual" (document no. G­560-0en), a copy of which is available (in English only) from your local Leica Geosystems agency.
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RCS communication parameters
\communication mode
NOTICE: 59 Switches to GeoCOM on-line mode.
Do you want to switch?
MC
On-line mode
6
The setting for the interface parameters is valid for
0
2
communication in remote-control mode. The baud rate can be selected within the range 2400 - 19200. No other values can be altered. For detailed information, please refer to the separate instructions for use.
System functions
With on-line operation (GeoCOM), the instrument is switched to a mode which permits communication with, or control by, a data recorder or PC. This mode operates across the RS232 interface; the GeoCOM command set is used.
PARAM YES NO
Calls the settings for the GeoCOM communications
parameters.
84
Activates the "On-line mode".
The operation of the instrument is now totally controlled across the interface. For information about data structures, and for the detailed structure of the control commands, please refer to the "GeoCOM Reference Manual"(G­560-0en), which is available only in English. The on-line mode can be
quitted by pressing "OFF" ( ).
Reverts; "On-line" mode is
not activated.
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Page 85
Automatic Target Recognition
Functionality
TCA and TCRA instruments are motorized and equipped with Automatic Target Recognition (ATR) coaxially in the telescope. The EGL guide light, mounted on the telescope, is optional. These instruments permit automatic angle and distance measurements to normal prisms and reduce the tedium of precise visual sighting to prisms. The prism is sighted with the optical sight only. Initiating a distance measurement will turn the instrument with the help of the motors to sight the prism-centre automatically. The angles V and Hz are measured to the centre of the prism at the completion of the distance measurement.
As with all other instrument
errors, the collimation error of the automatic target recognition (ATR) must be redetermined periodically (Refer to chapter
"Checking and Adjusting").
Reflections or foreign lights
(eg. from car headlights) can affect the ATR-measurement.
The built-in Automatic Target Recognition ATR1 transmits a laser beam. The reflected light is received by the built-in camera (CCD). The position of the received light spot with respect to the centre of the CCD is computed and the offsets are used to correct the horizontal and vertical angles. The offsets are also used to control the motors which turn the instrument so that the crosshairs are centred on the prism.
In order to minimize the times for measuring, the crosshair is not moved to the exact centre of the prism. The offset can be up to 5mm. Then the Automatic Target Recognition ATR1 measures the offsets between the crosshair and prism centre and corrects the Hz and V angles accordingly.
Therefore the Hz and V angles are measured to the prism-centre, regardless of the crosshair pointing precisely to the centre of the prism.
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Page 86
Functionality, continued
ATR-Mode (ATR+ / ATR-) LOCK-Mode (LOCK+ / LOCK-)
6
If the offset is more than 5mm when the prism is exactly aligned and in
0
2
faultless condition, the Automatic Tar­get Recognition ATR1 must be recalibrated. If excessive offsets occur frequently, contact your Leica Geosystems agency.
Hz-offset
Centre of the prism
V-offset
Crosshair
This mode permits the automatic recognition of stationary targets.
The observer must first use the optical sight to target the prism approximately so that it is located within the telescopic field of view.
When the distance measurement is triggered, the motors move the crosshair close to the centre of the prism to make distance measurement possible.
Lock-mode will enable TCA instruments to follow a moving prism. Distances can be measured whenever the prism stops for a short time (Stop and Go mode).
The icon is shown in the lower left area of the status field when the
LOCK-mode is activated and before a prism is found.
Switching to LOCK mode requires an initial distance measurement so that ATR1 "learns" the prism.
This measurement is the same as the initial measurement in ATR
1000Z19
The telescopic field of view is the active field of the ATR. Within this area the prism is identified immediately.
mode.
If the prism is subsequently moved, the telescope tracks it automatically for as long as the prism is aligned to the instrument.
The following functions are valid only for TCA and TCRA
instruments.
System functions
86
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LOCK-Mode (LOCK+ / LOCK-), continued
L.UNT-Mode (L.INT+ / L.GO)
The displayed angles refer to the crosshair direction during search. Once the prism is static, a distance measurement can be activated using "DIST" or "ALL". In this case the angles are measured on the centre of the prism after the distance measurement.
After a distance measurement, these corrected angles (for the centre of the prism) are displayed or recorded.
The icon is shown in the lower left area of the status field if the
LOCK mode is active and if the telescope tracks the prism
Any interruption to the tracking of the prism is indicated for about two seconds graphically in the lower left
status field by the symbol and also by a continuous acoustic signal
(beep).
The LOCK mode is interrupted (LOCK Interrupt), e.g. to measure inbetween to faraway targets without prism (eg. church spires). After the distance has been measured, the ATR immediately returns to its origi­nal condition.
This function should be used for measuring to a second prism (Chan­ging the prism).
The icon is shown in the lower left area of the status field, once the
L.INT-mode is activated. Measured angles refer to the direction of the crosshair.
At the completion of the distance measurement or after pressing L.GO, the LOCK mode is reactivated and the corresponding icon is shown in the lower left area of the status field.
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Page 88
LAST mode (LAST) Hz / V
RCS\ Hz/v
Set relative Hz- and V-angles
Hz/
∆∆
∆∆
Hz : 0°00'00"
V/
∆∆
∆∆
V : 0°00'00"
MC
6
0
2
(Valid only for motorized instruments)
The telescope is automatically pointed at the latest point to be stored. This function is available only if a point was stored after the instrument was switched on.
Activates the Hz/V mode.
CONT ABS
QUIT
In Hz/V mode, the TPS1100 can be turned by set angle values.
The input options are:
• absolute angle values which relate to the orientation of the TPS1100
• relative angle values which cause the TPS1100 to turn away from its present position by the amount entered.
Quits the Hz/V mode and starts the search mode, if ATR is activated.
Switches between absolute (ABS) and relative (REL).
System functions
88
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Page 89
Automatic Reflector Search
If the reflector is in the telescope's field of view, the crosshair is automatically positioned to the reflector when a measurement is triggered. If the target is not within the telescope's field of view, an automatic reflector search is started. Instruments equipped with the option PowerSearch can be switched to PowerSearch mode for a quick detection of prisms.
The shape of the ATR search window is rectangular and the defined area is scanned line by line starting in the center of the searching window.
Depending on the working mode of the instrument different sized search windows and different search strategies are used. The dimension of the search window in RCS mode can be defined in the "RCS Searching Window" function. In RCS mode, a working area can be additionnally defined. This area is automatically scanned if the local search was not successful.
• ATR and LOCK modes:
The operator stands at the instrument and can manually position the telescope to the reflector at any time. When a measurement is triggered, a small search window (Hz:
2.5gon / V: 2.5gon) is used to find the reflector as quickly as possible. If the target is lost in LOCK mode the path of the reflector is predicted for a few seconds.
• RCS mode:
The operator stands at the reflector and directs the telescope to the target with his preferred positioning mode (e.g. joystick). Because the telescope can only be positioned roughly when standing at the reflector, bigger search windows are used in RCS mode. If a search is triggered manually by pressing ALL or DIST the RCS Searching Window (default size Hz: 30gon / V: 15gon) is scanned starting at the current position of the telescope.
• The dimension of the search window in RCS mode can be defined in the "RCS Searching Window" function.
• A Working Area can be defined in RCS mode. This area is scanned automatically if the local search was not successful.
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Page 90
...\ RCS Searching Window
Define size of searching window
Hz Search: 40 g V Search : 40 g
MC
Automatic Reflector Search, cont.
RCS Searching Window
6
If the target is lost in LOCK mode first the path of the reflector is
0
predicted for a few seconds followed by a search which will by carried out
2
mainly in horizontal direction. The size of the search window depends on the shape of the predicted path. If a Working Area is activated then the entire Working Area is scanned after the respective local searches.
System functions
• PowerSearch
Instruments equipped with PowerSearch have the quick prism search feature. When PowerSearch is activated, the instrument performs a 360° rotation around its standing axis. If the laser swath of the PowerSearch sensor detects a prism, the rotation is stopped and the ATR performs a fine aiming in vertical direction. If a working area has been defined, PowerSearch is only active within the defined limits.
90
With this function the dimensions of the RCS Searching Window can be defined. If an automatic reflector search is started by pressing ALL or DIST in RCS mode, a search window with the predetermined dimensions is scanned at the current position of the telescope.
CONT DEFLT
QUIT
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Page 91
...\ Def. Working Area
actual Hz left : 171 g Hz right: 243 g V upper : 90 g V lower : 114 g
MC
RCS Searching Window, continued
Definition of a Working Area (WORKA)
Hz Search extent of search window
in Hz-direction
V Search extent of search window
in V-direction
To confirm the displayed values and leave the dialog.
Returns all values to default values.
TPS1100 - User Manual 2.2.1en
With this function a Working Area can be defined in which the instrument automatically searches for the reflector when working in RCS mode.
CONT DEF CENTR SHOW
QUIT
Hz left left boundary of working
area
Hz right right boundary of
working area
V upper upper boundary of
working area
V lower lower boundary of
working area
91
To confirm the displayed values and return to the
previous dialog.
To define a new working area
by pointing the telescope to two opposite corners of the working area (left corner - opposite right corner).
To centre the working area to
the current telescope position (retains the same size of the WA).
To position the telescope to the
upper left / lower right corner of the defined Working Area.
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Activate/Deactivate Working Area
Main\ Instr. information
Instr.type : TCRA1102plus Serial no. : 618775-2 Refl.less : Normal Range System vers. : Dec 22 2000 2.10 EDM version : 2.00 ATR vers. : 2.00
MC
(WORK+/WORK-)
General functions
6
If the instrument is in RCS mode and the determined working area is
0
2
activated then the entire working area is scanned for the reflector if the target was not found by the standard search method at the current position of the telescope. If the working area is deactivated only the standard search methods at the current position of the telescope are performed.
The instrument follows the
reflector even if the reflector is outside the Working Area. If the target is lost outside the Working Area a local search will be started. If the reflector was not found the predefined Working Area is scanned. On instruments with the optional PowerSearch, the working area can be used to limit PowerSearch to a certain area and when activated, PowerSearch only scans within the defined limits.
System functions
Instrument designation and software version (INFO)
This function displays the most important systems information.
CONT
PS Version 2.00.00
GeoCOM vers. : 1.06.04
QUIT
Display of instrument type, serial number, RL EDM type, software version and creation date, EDM version, ATR version, PS (PowerSearch) and GeoCOM version.
92
Electronic bubble (LEVEL)
Please refer to the description in the section "Levelling-up with the electronic bubble".
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Illumination
Illumination
Display :
⌧⌧
⌧⌧
Heating :
⌧⌧
⌧⌧
Contrast : 50%
⌧⌧
⌧⌧
Reticule : 80%
⌧⌧
⌧⌧
EGL : 100%
⌧⌧
⌧⌧
RedLaser :
⌧⌧
⌧⌧
MC
Switches on the back lighting and crosshair.
Settings for:
• Back lighting (display) on/off
• Heating of display on/off
• Contrast of display
• Brightness of crosshair illumination
• Brightness of EGL guide light (op­tional)
• Eyepiece diode laser on/off (optio­nal)
• Red laser on/off (optional)
The current settings are displayed numerically as percentages and graphically as a bar diagram. Optional settings are possible only if the instrument is additionally equipped.
TPS1100 - User Manual 2.2.1en
OK DISP+ HEAT+ RETI+ EGL+ RedL+
DEFLT QUIT
Switches the back lighting on and off.
Switches the display heating on and off.
Switches the crosshair illumination on and off.
The assignment of the
function key depends on the equipment installed: Switches the guide light on and off (EGL); key assignment "EGL+" .
Or:
Switches the eyepiece diode laser on and off; key assignment "DIOD+".
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Switches the visible red laser on and off (only for TCR/
TCRM instruments).
WARNING: (only for Extended Range Instruments)
If the visible red laser is switched on do not aim at prisms or reflecting objects through or beside the optical sight. Aiming against prisms is only allowed by looking through the telescope. Using the laser pointer is only permissible within a controlled area (refer to chapter "Safety Directions").
Sets standard values (contrast 50%,
crosshair 80%).
At extremely low
temperatures or in very bright ambient light conditions the contrast should be set to a higher value than 50%.
System functions
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\ Define Limits
Eyepiece V begin: 87°18' Eyepiece V end : 114°18' Lens V begin : 24°18' Lens V end : 130°30' Hz limit begin : 180°00' Hz limit end : 180°00'
MC
Accessories
Main\ Accessories
Accessories are attached: Eyepiece : NO Lens : NO
Limit for horiz.rotation Hz Limits active: NO
MC
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If an accessory such as the eyepiece prism or an additional lens for
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measuring to retro foils is used, then the movement for motorized instruments is restricted by preset values.
CONT DEF DEFLT
Sets the limits of the movement
Returns all settings to NO.
System functions
QUIT
A starting value and a finishing value are displayed. These determine the limits of movement of the telescope for motorized instruments. The range of movement between the starting value and the finishing value is defined by one clockwise rotation. The limits are entered for the vertical angle for the objective side (lens) and for the eyepiece side, and for the horizontal directions. The altered values are retained when the instrument is switched off.
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CONT DEF SET
QUIT
Values can be entered directly with the keyboard, or they can be determined through the position of the telescope.
Moves the telescope to the
position of the appropriate limiting value. The value displayed changes during the movement.
Accepts the value displayed
as being the limit of movement.
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Page 95
Accessories , continued
\ Load configuration
Current : 1100_DEF New config. : -----
Lang.System: Lang.Confi:
1. ENGLISH ENGLISH
2. GERMAN GERMAN
MC
Loading a configuration file (LOAD)
Eyepiece V begin Starting value for
V-angle of eyepiece.
Eyepiece V end Finishing value
for V-angle of eyepiece.
Lens V begin Starting value for
V-angle of objective.
Lens V end Finishing value
for V-angle of objective.
Hz limit begin Starting value for
Hz-direction.
Hz limit end Finishing value
for Hz-direction.
TPS1100 - User Manual 2.2.1en
If the Hz direction of the instrument is outside the permitted range but the target is within it, the instrument can still rotate itself towards the target.
1100Z45
Hz direction of
instrument
Permitted range
Rotation towards target possible
If the Hz direction of the instrument is within the permitted range but the target is outside it, rotation is not possible and an error report appears.
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The functions for transferring information between the internal memory and the PC-card are described below. For transfer via RS232 the Leica SurveyOffice PC software is generally used, in which event the instrument is remote­controlled and requires no user interface.
LOAD
QUIT
Selects the configuration files from the PC-card in the directory "\tps\conf\". Displays the languages available in the system or which belong to the configuration file.
Loads the new configuration.
System functions
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Main\Save param.to PC-Card
Enter filename to save para: Param. file : TEST
MC
Main\Load system parameter
Current : T2 New param. : Elec_T16
MC
Loading a configuration file, continued
Loading a system-parameter file
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If no file can be found, the message 659 appears along with the note that
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no configuration file was found.
A precautionary interrogation (message 658) appears before the actual loading and asks for confirmation of the intention to load a new configuration.
"NO" will then abort the function. "YES" will load the configuration.
LOAD SAVE
Select the new system-parameter files from the PC-card.
Loads the new system­parameters.
Stores the current system-
parameters.
The following display appears:
QUIT
SAVE
QUIT
Input the name of the system­parameter file to be saved.
Stores the file on the PC-
card.
System functions
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Page 97
System parameters
...\ Load Application
New appl. : Area Version : 1.01
Lang.System: Lang.Appl:
1. English English
2. Deutsch Deutsch
MC
...\ Load System Language
1. Language: ENGLISH
2. Language: DEUTSCH
3. Language: -----
MC
General parameters
This section describes the system­parameters of the TPS1100 instruments.
TPS1100 - User Manual 2.2.1en
Load application
LOAD DEL-A
QUIT
Selects the application from the PC­card in the directory "\tps\appl\". The column at the right of the diplay shows in which languages the application will be loaded.
Loads the selected
application. New application versions can be loaded directly; it is not necessary to delete the existing application before.
Deletes the selected
application.
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Load system language
LOAD DEL-A
QUIT
Selects the system languages from the PC-card in the directory "\tps\lang\". An existing system language can not be overwritten: it must be deleted first.
Loads a selected system language.
Deletes a selected system language.
System parameters
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General parameters, continued
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Date
Sets the date. Choice of layout: 09-11-98 or
11.09.98.
Date form.
Selects the date format. Choice of layout: Day/Month/Year Month/Day/Year Year/Month/Day
Time
Sets the time.
Time form.
Sets the time format. Choice between 24h clock and 12h clock with am/pm
Alpha mode
The alphanumeric input can be either through the function keys or through the numeric keys. If numeric keys are used, there is a choice between "Numeric keys" and "Numeric exten­ded". In "Numeric extended" mode, more characters are available.
Key beep
Sets the volume of the beep emitted when the keys are pressed. The beep is always active for messages. There is a choice between beep off (None), soft beep (Low) and loud beep (Loud).
System parameters
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Page 99
Configuration parameters
Autoexec.
Selects the application, which will then be started automatically immediately after switching on. The list includes the following permanently-available options: "Main menu", "Measurement & Recording" and "Enter Station Data". Also, all of the applications programs loaded are listed. The function or application selected is automatically started whenever the instrument is switched on.
Language
Selects the system language (a maximum of three languages can be stored). English is always available and cannot be deleted.
Dist. Unit
Units of distance measurement:
Metre Metres (m) Int.Ft International feet,
storage in US feet [fi]
Int.Ft/Inch Int. feet, inches and 1/8
inches (0' 00 0/8fi),
storage in US feet [fi] US Ft US feet [ft] US Ft/Inch US feet, inches and 1/8
inches
(0' 00 0/8fi) [ft]
Dist. Dec.
Decimal places for distance:
Metre 0,1,2,3 Int.Ft 0,1,2,3 Int.Ft/Inch 0 US Ft 0,1,2,3 US Ft/Inch 0
Angle Unit
Units of angle measurement:
400gon 360° ' " 360° dec 6400 mil
Angle Dec.
Decimal places for angle:
TCx1101/1102:
• 400 gon, 360°'", 360°dec. => 2, 3, 4
• 6400 mil => 1, 2, 3
TCx1103/1105:
• 400 gon, 360° dec. => 2, 3, 4 (in steps of five units)
• 360°'" => 2, 3, 4
• 6400 mil => 1, 2, 3
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System parameters
Page 100
Configuration parameters, continued
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Temp. Unit
Units of temperature
° C Degrees Celsius ° F Degrees Fahrenheit
Press. Unit
Units of atmospheric pressure
mbar millibars mm Hg millimetres of mercury inch Hg inches of mercury hPa hectopascals psi pounds per square inch
Coord. Seq.
Sequence of coordinates in display
North / East (X, Y) East / North (Y, X)
For further information, please refer to the section "GSI parameters".
Hz system
Sense of Hz-circle system
North Azimuth(+) Clockwise angle
measurement (+) starting at North
North anticlw (-) Anticlockwise angle
measurement (-) starting at North
South Azimuth Clockwise angle
measurement (+) starting at South
Face I
Definition of faces:
V-drive left Vertical drive on the
left side
V-drive right Vertical drive on the
right side
System parameters
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TPS1100 - User Manual 2.2.1en
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