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
and operating it.
Read carefully through the User Manual before you switch on the
instrument.
2
TPS1100 - User Manual 2.2.1en
Page 3
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:
3
Product identification
Page 4
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.
Index ........................................................... 156
TPS1100 - User Manual 2.2.1en
9
Contents
Page 10
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
10
TPS1100 - User Manual 2.2.1en
Page 11
ValidityDocumentation
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.
6
TPS1100 - User Manual 2.2.1en
11
Introduction
Page 12
Description of the system
6
0
Instrument descriptions
1
2
3456
12 1315
1110
1418191720
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
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
6
10
1100Z461100Z47
TPS1100 - User Manual 2.2.1en
13
Description of the system
Page 14
Extended Range (Option)
6
0
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 thechapter "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 andadjusting"). 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
14
TPS1100 - User Manual 2.2.1en
Page 15
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.
6
10
1100Z55
TPS1100 - User Manual 2.2.1en
15
Description of the system
Page 16
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
16
TPS1100 - User Manual 2.2.1en
Page 17
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.
6
10
TPS1100 - User Manual 2.2.1en
17
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
18
TPS1100 - User Manual 2.2.1en
Page 19
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.
6
10
TPS1100 - User Manual 2.2.1en
19
Description of the system
Page 20
Leica Survey Office PC software package
6
0
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
20
TPS1100 - User Manual 2.2.1en
Page 21
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
TPS1100 - User Manual 2.2.1en
21
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
22
TPS1100 - User Manual 2.2.1en
Page 23
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
12
TPS1100 - User Manual 2.2.1en
23
Preparing to measure, setting up
Page 24
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
24
TPS1100 - User Manual 2.2.1en
Page 25
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.
TPS1100 - User Manual 2.2.1en
25
Preparing to measure, setting up
Page 26
Insert PC-card
6
0
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
CONTL.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.
CONTL.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, tCompensator index error
• iVertical-index error
• cLine-of-sight error
• aTilting-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,tic/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.
Compensator Index Error l,t
Date/Time:03/04/2000 15:43
Old values:l=0.0000g t= 0.0000g
Measurements
L= -0.0126gT= 0.0298g
L= 0.0368gT= 0.0164g
New values:l=0.0010gt= 0.0023g
Vertical Index Error i
Date/Time:03/04/2000 15:45
Old value:i= 0.0000g
Measurements
Hz= 377.0597 gV= 104.2828 g
Hz= 177.0562 gV= 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:
OKABORT
Turn the instrument through 180°
(200 gon) so that ∆Hz = 0° 00' 00"
(0.0000 gon).
TPS1100 - User Manual 2.2.1en
OKABORT
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 RETRYNO
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'.
OKABORT
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 RETRYNO
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.
OKABORT
QUIT
QUIT
After successful completion of the
second measurement, the older and
the newly-determined line-of-sight
errors are displayed.
YES RETRYNO
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?
YESNO
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
OKABORT
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 RETRYNO
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 displayon 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
12
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
CONTMOREABORT
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 RETRYNO
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 tribrachAdjustment
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
TPS1100 - User Manual 2.2.1en
Page 49
System functions
\Selection ( )
Meas Job
DEFAULT.GSIPC-Card
RS232RS232
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.
CONTNEWEDITDEL
|<<-- -->>|QUIT
αα
αNUM
αα
6
10
12
21
26
TPS1100 - User Manual 2.2.1en
49
System functions
Page 50
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-
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
SEARCHINPUTVIEW
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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Page 52
\ Data View and Edit
1/20
Point ID:1
East:0.000m
North:0.000 m
Elev.:0.000 m
MC
Data management, continued
Display of point data found
CONT NEW S <----> <<REP REP>>
INS-C |<<- ->>|DELQUIT
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.
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".
System functions
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Page 54
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
54
TPS1100 - User Manual 2.2.1en
Page 55
Displaying GSI data, continued
InputResultsRemarks
11.
11, 110, 1101, 11 ABC 5,
111111
After 11 there can be any character
and in any amount.
.1111 , ABC 11, 11111
Before 11 there can be any character
in any amount.
1.010, 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 0at 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.
55
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Page 56
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.
CONTREC
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
56
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.
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
OKASCII
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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57
System functions
Page 58
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.
OKDEFLT
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).
System functions
58
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Page 59
CONV\ CONVERSION
Completed!
Points converted: 135
Lines not converted:12
MC
Converting data, continuedFormatting 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.
NEWQUIT
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
OKABORT
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".
59
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.
System functions
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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.
60
CONTDEFLT
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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Page 61
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.
TPS1100 - User Manual 2.2.1en
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.
CONTDEFLT
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
61
Each line can display any and all of
the available display data.
Sets the current DSP mask to
"Standard", i.e. to the DSP
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).
System functions
62
TPS1100 - User Manual 2.2.1en
Page 63
GSI-parameters, continued
WI-No.ParametersDescription
--Offs. Elev.Elevation offset of target point
--Offs. LngthLength offset of target point
--Offs.CrossCross offset of target point
--Offs.ModeView and select offset mode, reset after REC or keep
(*) 52n / sNumber of averaged distances measured and the standard deviation in millimetre
(*) 82NorthNorth coordinate of target point
HzHorizontal 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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63
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Page 64
GSI-parameters, continued
WI-Nr.ParametersDescription
(*) 81EastEast coordinate of traget point
--pp m atm.Atmospheric ppm value
--ppm geom.Geometric ppm value
(*) 59ppm totalTotal ppm-correction
(*) 51ppm/mmTotal ppm-correction and prism constant
--PtC.Descr.Description for the current Code
(*) 71Point CodeCurrent Point Code
(*) 11Point IdCurrent Point Id (either the running or the individual poi nt id)
(*) 87Refl. Ht.Reflector height
--Refl. listView and select a reflector
--Refl.NameDisplay the current reflector name
--Displ.MaskView and select the recording mask
(*) 31Slope DistMeasured slope distance (already corrected using ppm and prism constant)
--S tation IdStati on p oi nt numb er
(*) 86Stn.Elev.
(*) 85Stn.NorthStation northing coordinate (Xo)
(*) 84
(*) 22VVertical angle
--V-DisplayView and select the V angle display
--Last PtIdDisplay of the last recorded Point Id
--Prev.CodeDisplay of the last recorded Code
--Prev.PtCodDisplay of the last recorded Point Code
--TimeCurrent system-time
--Target TypCurrent target type, reflector or none
Stn.EastStation easting coordinate (Yo)
Station Elevation (Zo)
System functions
64
TPS1100 - User Manual 2.2.1en
Page 65
GSI-parameters, continued
DMaskCoord. Seq.
Display in
measurement
mode
Change
Easting/NorthingE/N as in DMaskEasting/Northingnone
Easting /No rthi ngchange E/N S eq .Northing/Eastingyes
Northing/EastingE/N as in DMaskNorthing/Eastingnone
Northi ng/Easti ngchange E/N S eq .E asting/Northingyes
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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65
System functions
Page 66
\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 :256431.871m
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)".
DISTCONT INPUT
ALLREC 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 "Datamanagement".
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.
66
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.
TPS1100 - User Manual 2.2.1en
Page 67
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.
SETHz=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 ->TRKTEST 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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Page 68
Distance measurement, continuedSelecting 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
CONTREFL
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.
68
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
TPS1100 - User Manual 2.2.1en
Page 69
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 tochapter "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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Page 70
\ 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 "Reflectorselection".
CONTDEF 1 DEF 2 DEF 3
QUIT
Choosing the appropriate prism. The
appropriate additive constant is set
automatically at the same time.
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.
CONTFREQSTOP
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.
System functions
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Page 72
\ 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.
CONTGEO=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".
TPS1100 - User Manual 2.2.1en
Page 73
\ 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.
CONTDEFLT
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 "PPMAtmospheric" 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 DISTRECSetHz >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.
System functions
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Page 74
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
TPS1100 - User Manual 2.2.1en
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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75
System functions
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
TPS1100 - User Manual 2.2.1en
Page 77
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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77
System functions
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.
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.
RECL 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.
System functions
6
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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.
RECNEWLAST 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.
TPS1100 - User Manual 2.2.1en
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 NEWLAST 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 SETVIEW LAST
Horiz Dist:-----
∆∆
∆HorizDist:-----
∆∆
Elevation:-----
∆∆
∆Height:-----
∆∆
HELPQUIT
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
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.
CONTDEFLT
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.
System functions
6
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Page 84
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.
PARAMYESNO
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.
TPS1100 - User Manual 2.2.1en
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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85
System functions
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
TPS1100 - User Manual 2.2.1en
Page 87
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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87
System functions
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.
CONTABS
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
TPS1100 - User Manual 2.2.1en
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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89
System functions
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.
CONTDEFLT
QUIT
TPS1100 - User Manual 2.2.1en
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 Searchextent 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 CENTRSHOW
QUIT
Hz leftleft boundary of working
area
Hz rightright boundary of
working area
V upperupper boundary of
working area
V lowerlower 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.
System functions
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Page 92
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".
TPS1100 - User Manual 2.2.1en
Page 93
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+".
93
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 "SafetyDirections").
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
6
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Page 94
\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
6
If an accessory such as the eyepiece
prism or an additional lens for
0
2
measuring to retro foils is used, then
the movement for motorized
instruments is restricted by preset
values.
CONTDEFDEFLT
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.
94
CONTDEFSET
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.
TPS1100 - User Manual 2.2.1en
Page 95
Accessories , continued
\ Load configuration
Current:1100_DEF
New config.:-----
Lang.System:Lang.Confi:
1. ENGLISHENGLISH
2. GERMANGERMAN
MC
Loading a configuration file (LOAD)
Eyepiece V begin Starting value for
V-angle of
eyepiece.
Eyepiece V endFinishing value
for V-angle of
eyepiece.
Lens V beginStarting value for
V-angle of
objective.
Lens V endFinishing value
for V-angle of
objective.
Hz limit beginStarting value for
Hz-direction.
Hz limit endFinishing 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.
95
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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Page 96
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
6
If no file can be found, the message
659 appears along with the note that
0
2
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
96
TPS1100 - User Manual 2.2.1en
Page 97
System parameters
...\ Load Application
New appl.:Area
Version:1.01
Lang.System:Lang.Appl:
1. EnglishEnglish
2. DeutschDeutsch
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
LOADDEL-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.
97
Load system language
LOADDEL-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
6
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Page 98
General parameters, continued
6
0
2
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
98
TPS1100 - User Manual 2.2.1en
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:
MetreMetres (m)
Int.FtInternational feet,
storage in US feet [fi]
Int.Ft/InchInt. feet, inches and 1/8
inches
(0' 00 0/8fi),
storage in US feet [fi]
US FtUS feet [ft]
US Ft/Inch US feet, inches and 1/8
inches
(0' 00 0/8fi) [ft]
Dist. Dec.
Decimal places for distance:
Metre0,1,2,3
Int.Ft0,1,2,3
Int.Ft/Inch0
US Ft0,1,2,3
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
6
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TPS1100 - User Manual 2.2.1en
99
System parameters
Page 100
Configuration parameters, continued
6
0
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Temp. Unit
Units of temperature
° CDegrees Celsius
° FDegrees Fahrenheit
Press. Unit
Units of atmospheric pressure
mbarmillibars
mm Hgmillimetres of mercury
inch Hginches of mercury
hPahectopascals
psipounds 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 AzimuthClockwise angle
measurement (+)
starting at South
Face I
Definition of faces:
V-drive leftVertical drive on the
left side
V-drive rightVertical drive on the
right side
System parameters
100
TPS1100 - User Manual 2.2.1en
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