Nikon LV100D, LV150, LV150A User Manual

En
Specifications and equipment are subject to change without any notice or obligation on the part of the manufacturer. April 2005.
©2000-05 NIKON CORPORATION
This brochure is printed on recycled paper made from 40% used material.
WARNING
TO ENSURE CORRECT USAGE, READ THE CORRESPONDING MANUALS CAREFULLY BEFORE USING YOUR EQUIPMENT.
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Industrial Microscopes LV150/150A/100D
Industrial Microscopes
32
A modular microscopy system for breadth and depth
• Printer heads
• Micro sensors
• Optical switches
• GMR heads for HDD
• Medium/small PCB
• FPC
• Interposer substrates
• Bare wafers
• Lithography process
• Probe, test processes
• Post-dicing
• Macromolecules, monomeric materials
• Organic/inorganic materials
• Polymers • Thin film
• Magnetic materials
• Crystals • Metallugraphy
• Precision molds • LCD, color filters
• Polarizing filters
• Organic EL
• CCD • CMOS
• LCOS • DMD
• LF/TAB • WL-CSP
• QFP • SIP
• BGA, CSP, FC
VersatilityVersatility
Versatility
Extend your vision
Optical performance
Improved performance
Extend
your
vision
Extend
your
vision
Optical
performance
Optical
performance
Basic
Performance
Improved
performance
• OA equipment parts
• Cell phones, PDAs, DSC, PC parts
• Automobiles, aeronautics
MEMS
PCB
Casts and parts
Precision molds
FPD
Display devices
Semiconductors
Materials Packages
Versatility
5
Extensive range of industrial stages and accessories
Users can select suitable models based on sample and stage stroke. All stages are highly durable with triple-plate design.
Dia base unit for diascopic illumination
In the Eclipse LV series, the LV-DIA Dia Base is available for diascopic illumination OEM use. Users can now take full advantage of the modular design. A UN2 transformer is used for the power supply.
The modular design of the Eclipse LV series allows an unprecedented level of versatility. The Eclipse LV series offers flexibility that enables it to cover a wide variety of products and applications, extending from development and quality control to inspection in the manufacturing process. Users will recognize the superb performance of the Eclipse LV series when inspecting semiconductors, FPD, packages, electronics substrates, materials (material science), medical devices, cast/metallic/ceramic parts, precision molds, MEMS, telecommuni­cations devices, and a wide variety of other samples.
Versatility
Accepts taller samples
The maximum sample height can be increased to 82mm from 47mm by inserting the LV-CR Column Riser 35 between the main body and arm of the microscope. This feature is useful for viewing the surfaces of precision molds, optical materials and other thick samples.
Non-Nikon stages (LV150 or LV150A only)
Use of non-Nikon stages, such as the Suruga Seiki B23-60CR, in combination with the LV-SUB Substage 2 allows the microscope to handle taller samples of up to 116.5 mm, thereby enabling the observation of fiber ends and other tools.
With column riserWithout column riser
Combination of LV-150 with LV-SUB Substage 2 and Suruga Seiki B23-60CR stage
82mm
47mm
Modular design
LV150 standard combination
Appropriate holder and substage are selected based on sample and stage combination.
Compact industrial stage: LV-S32 3x2 Stage
The newly designed LV-S32 3x2 is a compact stage for industrial microscopes. Its triple-plate design ensures
durability, stability and ease of use, even when heavy samples such as metallic materials are observed. The standard glass plate makes this stage suitable for episcopic and diascopic illumination.
An example of LV-DIA Dia Base built into a taped sample inspection system
LV-DIA Bia Base
LV-S6 6x6 Stage Stroke: 150 x 150 mm
LV-S64 6x4 Stage Stroke: 150 x 100 mm
L-S6WH Wafer Holder 6 (for LV-S6 6x6 Stage)
L-S6PL ESD Plate (for LV-S6 6x6 Stage)
LV-S32PL ESD Plate (for LV-S32 3x2 Stage)
LV-S32SGH Slideglass Holder (for LV-S32 3x2 Stage)
LV-SUB Stage (exclusive for LV150/LV150A)
LV-SUB Substage 2 (exclusive for LV150/LV150A)
LV-S32 3x2 Stage Stroke: 75 x 50 mm
Tape-suction
section
Roll-out section Roll-in section
Tape-transport section
Stage section
6
7
Optical PerformanceExtend your vision
A wide variety of observation methods is available with the Eclipse LV series. Observations with first-order compensator, UV polarizing, and epi-fluorescence observations with UV excitation, in addition to brightfield, darkfield, DIC, simple polarizing, epi-fluorescence (excitation using visible light) and double-beam interferometry are all possible. Two new light sources also have been developed: high-intensity, low power­consumption 12V-50W halogen light source and adjustable high-intensity mercury-fiber light source.
Field Aperture Shutter UV-cut
diaphragm diaphragm filter
BF Any diameter Any diameter Open Insert
DF Open Open Open Insert
FL1 Any diameter Any diameter Open
FL2 Any diameter Any diameter Open
Universal epi-illuminator: LV-UEPI
The LV-UEPI universal epi-illuminator enables brightfield, darkfield, simple polarizing and DIC observations. Field and aperture diaphragms are automatically opened when the observation is switched from brightfield to darkfield, and return to their original position when switched back to brightfield.
High-intensity 12V-50W halogen light source:
LV-LH50PC Precentered Lamphouse
Although the LV-LH50PC Precentered Lamphouse is 12V-50W, the brightness is equivalent to or higher than that of 12-100W types. The low power­consumption halogen light source contributes to the compact design of the microscope while also being friendly to the environment. Focus drift due to heat from the illuminator is substantially reduced.
Universal epi-illuminator 2: LV-UEPI2
The LV-UEPI2 universal episcopic illuminator is equipped with advanced optics suited to a wide variety of observation methods—brightfield, darkfield, DIC and epi­fluorescence—and automatically sets optimal illumination in accordance with the field and aperture diaphragm, shutter, and filters, including diffuser and ND. This design enables the operator to concentrate on the observation.
Auto optimal illumination selection
Brightfield
Darkfield
Simplepolarizing
DIC
Brightfield
Darkfield
Simplepolarizing
Observationwithfirst-ordercompensator
UVpolarizingepi-fluorescence
DIC
Epi-fluorescence(UVexcitationpossible)
CFI60 LU Plan Fluor EPI series
CFI60 LU Plan Fluor BD series
CFI60 L Plan EPI CR series of objective lenses with correction ring
With correction at 0.7 mm (50x)
Without correction (50x)
Transmission wavelength coverage extended to UV
CFI LU Plan Fluor series
The new CFI LU Plan Fluor series covers transmission wavelength ranges up to UV. These objective lenses are suitable for various research, analysis and examination needs, while maintaining Nikon’s commitment to high NA and long working distance. Only one kind of objective lens is needed for brightfield, darkfield, simple polarizing, observation with first­order compensator, DIC and UV epi-fluorescence observations. These objective lenses, which offer high resolution and easy-to­use performance, can be combined not only with microscopes but also with other equipment for even greater versatility.
Objective lenses with correction ring
CFI L Plan EPI CR series
The CFI60 series now includes the CFI L Plan EPI CR series to cope with the thinner coverglass used in liquid crystal displays, and highly integrated, and dense devices. Coverglass correction can be continuously made from 0 mm up to 1.2 mm (0-0.7 mm and 0.6-1.3 mm for 100x) with the correction ring. The 100x objective lens offers 0.85 high NA, while enabling high-contrast imaging of cells and patterns without being affected by the coverglass.
Environmentally friendly
The eco glass used in the CFI LU Plan Fluor and L Plan EPI CR series does not contain harmful substances such as lead and arsenic.
Model Magnification NA
Working Distance (mm) CFI L Plan EPI 2.5X 0.075 8.8 CFI LU Plan Fluor EPI 5X 0.15 23.5
New
10X 0.30 17.3 20X 0.45 4.5 50X 0.80 1.0
100X 0.90 1.0
CFI LU Plan EPI ELWD 20X 0.40 13.0
50X 0.55 10.1
100X 0.80 3.5
CFI L Plan EPI SLWD 20X 0.35 24.0
50X 0.45 17.0
100X 0.70 6.5
CFI LU Plan Apo EPI 100X 0.95 0.4
150X 0.95 0.3
CFI L Plan Apo EPI WI 150X 1.25 0.25
Model Magnification NA
Working Distance (mm)
CFI LU Plan Fluor BD 5X 0.15 18.0
New
10X 0.30 15.0 20X 0.45 4.5 50X 0.80 1.0
100X 0.90 1.0
CFI LU Plan BD ELWD 20X 0.40 13.0
50X 0.55 9.8
100X 0.80 3.5
CFI LU Plan Apo BD 100X 0.90 0.51
150X 0.90 0.4
Model Magnification NA (mm) Working Distance (mm) Glass Thickness Correction Range CFI L Plan EPI CR
New
20x 0.45 10.9-10.0 0-1.2mm
CFI L Plan EPI CR
New
50x 0.7 3.9-3.0 0-1.2mm
CFI L Plan EPI CRA
New
100x 0.85 1.2-0.85 0-0.7mm
CFI L Plan EPI CRB
New
100x 0.85 1.3-0.95 0.6-1.3mm
CFI60 Series Objectives
8 9
Usability has been vastly improved as has durability and rigidity.
Improved performance
Highly rigid, vibration-free body
The use of structural analysis during the design process has improved rigidity and antivibration parameters to yield clear images even at high magnification.
Tilting trinocular eyepiece tube
LV-TT2 Tilting Trinocular Eyepiece Tube
The newly developed LV-TT2 tilting trinocular eyepiece tube (erect image) offers comfort to all users, regardless of their stature or viewing position. The optical path changeover of 100:0/20:80 allows the simultaneous use of a monitor.
Highly durable motorized nosepiece
LV-NU5A Nosepiece
The LV-NU5A motorized universal quintuple nosepiece is 10 times more durable than its predecessor and can be used with the LV150A. In combination with the LV-NCNT motorized nosepiece controller, it can also be used in other devices.
Manual nosepiece
A variety of manual nosepieces are available to suit all needs.
Thorough ESD protection
All parts of the microscope that might be touched, including the body, tube and stage, have been insulated. This improves anticontamination and prevents samples from being harmed by static electricity, thereby improving yields.
Electrostatic decay time: 1000-10V, within 0.2 sec.
C-N6 Nosepiece (Brightfield)
L-NBD5 Nosepiece (Bright/darkfield)
L-NU5 Nosepiece (Universal)
LV-P Plate
Brightfield
The antiflare design applied to the objective lenses and light source ensures bright, high-contrast images.
Darkfield
Nikon’s unique “Fly-eye Lens” used in the darkfield illuminator yields a threefold increase in brightness over previous models. This allows high­sensitivity detection of defects and height gaps in samples.
Nomarski DIC
Standard or high contrast DIC sliders can be selected to suit the sample. This method is useful for the surface observations of various devices and precision molds.
Epi-fluorescence
UV, V, BV, B or G excitation fluorescence filter blocks can be selected. This method is perfect for the observation of OEL, ion migration and other substrate uses.
L-DIC DIC Prism (standard) L-DIHC DIC Prism (high contrast) Brightfield Epi-fluorescence B-2A
Fluorescence filter blocks
Simple polarizing
In addition to simple polarizing, a lambda plate can be inserted into the optical path to achieve observations with a first­order compensator. This is useful for liquid crystal inspections (when used in combination with the LV­UEPI 2).
Double-beam interferometry equipment (measures minute height gaps)
Michelson (TI) and Mirau (DI) types of episcopic double­beam interferometry can be carried out. A filar micrometer eyepiece can be used to examine or measure samples while avoiding direct contact.
Diascopic illumination
Diascopic illumination is used to observe optical parts, FPD and other samples that transmit light.
Episcopic Two-beam Interferometry Equipment TI/DI
Condenser
Observation Methods
YM-PO Polarizer
LV-UV Polarizer
LV-FLAN FL Analyzer
L-AN Analyzer
LV-PO Polarizer
LV-FLAN FL Analyzer
L-DIC DIC Prism
L-DICH[??] High-contrast DIC Prism
YM-PO Polarizer
L-AN Analyzer
10 11
Semiconductor (IC wafer) Semiconductor (IC wafer) MEMS (optical switch)
Brightfield Darkfield Brightfield
Micro bump Compact disc (CD) Image sensor (CCD)
Brightfield Simple polarizing Brightfield
PCB (ion migration) PCB (ion migration) Precision mold
Brightfield Epi-fluorescence DIC
L150A controls
(Episcopic illumination type)
Applications
CFI-series eyepiece
An illuminator that can be used for brightfield, darkfield, simple polarizing and DIC observations.
LV-UEPI
A universal motorized nosepiece that is 10 times more durable than its predecessors.
LV-NU5A Nosepiece
These objective lenses feature a high NA, long working distances and an extended transmission wavelength range.
CFI LU Plan Fluor series
The LV150 and LV150A microscopes are used for episcopic illumination.
A trinocular tube with an optical path changeover of 100:0/0:100.
LV150/LV150A
An episcopic illumination stage capable of inspecting 150mm wafers. (With 6” wafer holder)
LV-S6 6x6 Stage
LV-TI3 Trinocular Tube
A low power-consumption 12V-50W halogen light source equivalent to or higher than the 12V-100W type.
LV-LH50PC Precentered Lamphouse
Motorized nosepiece controls
12 13
Applications
(Episcopic/diascopic illumination type)
LCD (color filter) LCD (conductive particle) Test reticle
Diascopic brightfield DIC Diascopic brightfield
リシャ輝石??
Carbon paper Nodular graphite cast iron
DIC Brightfield DIC
Tourmaline Tourmaline Tourmaline
Brightfield DIC Double-beam interferometry
CFI-series eyepiece
The LV-UEPI2 illuminator enables brightfield, darkfield, DIC, simple polarizing, and UV excitation epi-fluorescence observations.
LV-UEPI2
Selectable from C-N6 (brightfield), L-NBD5 (bright/darkfield) and L­NU5 (universal) nosepieces.
Nosepiece
These objective lenses feature high NA, long working distances and an extended transmission wavelength range.
CFI LU Plan Fluor Series
A trinocular tube with an optical path changeover of 100:0/0:100.
This small, industrial-use stage has a triple-plate design and can be used for episcopic and diascopic illumination.
LV-S32 3x2 Stage
LV-TI3 Trinocular Tube
A low power-consumption 12V-50W halogen light source equivalent to or higher than the 12V-100W type.
LV-LH50PC 12V-50W Lamphouse
The LV100D microscope is capable of episcopic and diascopic illumination.
LV100D
14 15
ACCESSORIES
100
IN
0
100
OUT
Eyepiece tubes
Illuminators Double Port Polarizing/DIC accessories
Nosepieces
Objective adapters
Objective lenses
Substages (LV150/LV150A)
Stages
Holders
Micrometers
Diascopic illumination condensers
Model F.O.V. Remarks
CFI 10x 22
CFI 10xM 22 Photomask included CFI 10×CM:for C-TE binocular ergo tube
22 Crosshairs and micrometer included
CFI 12.5x 16
CFI 15x 14.5
CFI UW 10x 25
CFI UW 10xM 25 Photomask included
Mirometer eyepiece 10xN 20 Stroke 10 mm
Main scale: 0.1 mm/increments Sub scale: 0.01 mm/increments
Objective micrometer
Eyepiece micrometer
Grid micrometer
LV-TI3 Trinocular Eyepiece Tube ESD
Y-IDP Double Port (Beamsplit 45:55/0:100) Y-IDP Double Port 0/100 (Beamsplit 100:0/0:100)
LV-TT2 Tilting Trinocular Eyepiece Tube
LV-SUB Stage LV-SUB Stage 2
C-N6 Nosepiece (Brightfield)
L-NBD5 Nosepiece (Bright/darkfield)
L-NU5 Nosepiece (Universal)
C-OA 15mm AdapterLU objective
Adapter M32-25
LV-NU5A Motorized Nosepiece (Universal)
LV-S6 6x6 Stage LV-S64 6x4 Stage LV-S32 3x2 Stage
L-S6WH Wafer Holder
For LV-S6 6x6 Stage For LV-S32 3x2 Stage
L-S6PL ESD Plate LV-S32SGH
Slideglass Holder
LV-S32PL ESD Plate
Simple Polarizing
UV polarizing epi-fluorescence
YM-PO Polarizer
LV-UV Polarizer
LV-FLAN FL Analyzer
L-DIC DIC Prism
L-DICH
High-contrast DIC Prism
L-AN Analyzer
YM-PO Polarizer
L-AN Analyzer
LV-PO Polarizer
LV-FLAN FL Analyzer
LV-P Plate
Observation with first-order compensator
DIC
LWD Achromat
C-C Abbe
DF (Dry)
Slide (Swing-out??)
Achromat 2-100x
C-C Achro
CFI LU PLAN FLUOR EPI series
CFI LU PLAN FLUOR BD series
CFI L PLAN EPI CR series
LV-UEPI
LV-UEPI2
Eyepieces
IN
OUT
0
100
0
100
16 17
Digital cameras for microscopes
The Digital Sight series is a powerful imaging system for monitoring/capturing images taken under brightfield,
darkfield, DIC, epi-fluorescence, and other observation methods.
Ultrahigh-definition Digital Camera
Digital Camera
The DXM1200F produces true-to-life, extremely high-quality images with up to approximately 12 million output pixels. It meets
the demanding requirements of professional users and is excellent for image analysis in advanced R&D fields.
• Approx. 12 million output pixels comparable to film high-end cameras, thanks to Nikon’s exclusive micro­step high-density imaging technology
• Live image display at a frame rate of 12 fps max.
• The wide exposure latitude produces true-to-life images regardless of brightness level.
Standalone type
This type comes with an LCD monitor, making it convenient for on-screen monitoring without a PC and in applications that require long/multiple exposures.
Real imaging camera—DS-2Mv-L1
• Live image display at 30fps max.
• Image size: 1600 x 1200 pixels
• 6.3” TFT monitor
• Analog RGB output
• CompactFlash card slot
• USB mass-storage-class compatible
• Direct print function (Pict bridge compatible) optional
*1
• Ethernet (100BASE/TX) port
*2
*1: A CP900DC dedicated printer
and C-mount adapter are necessary. Provided with real 10 mode (10X printing).
*2: FTP Client/Server, HTTP Server Telnet Server functions provided.
PC-connection type
This type requires connection to a PC and allows observation on a PC monitor, image capture, measurement and analysis when special application software, ACT-2U, is used.
Real imaging camera—DS-2Mv-U1
• Live image display at 12fps (800 x 560)
• Image size: 1600 x 1200 pixels
• PC connection via USB2.0
• Dedicated application software—ACT-2U
Camera heads
Select the best type to match your sample and use.
For brightfield, darkfield, DIC observations
For fluorescence observations (that require long exposure)
A host of measuring tools
*Dedicated ACT-2U camera control software is necessary when using the DS-U1.
DS-2MBW
Image size: 1600 x 1200 pixels
15 fps (30 max.)
Superb movie
DS-5M
Image size: 2560 x 1920 pixels
True-to-life recording of minute
images
DS-2MBWc
Image size: 1600 x 1200 pixels
Sensitivity approx. 5 times greater
than predecessors
Includes a Peltier device
Brilliant images with minimum noise
DS-5Mc
Image size: 2560 x 1920 pixels
Includes a Peltier device
Brilliant images with minimum noise
Cross scale (DS-L1 only)
Option: camera control software
ACT-2
The optional ACT-2U software offers the following arrays of convenient measurement tools.
Camera control software
ACT-1
Minimizes fatigue during large-volume, extended time shooting.
All essential sections, including live image preview, captured image window, thumbnail, and image capture parameter setting panel, are simultaneously displayed on a single screen, enabling users to easily understand image capture procedures. The size of the parameter setting panel has been reduced to leave more space for image display.
Dedicated camera control software ACT-2U
Wafer/IC chip
Two-point distance
Area (DS-U1 only) XY scale
Screen pattern (crossline, circle)
Scale Point to line distance Intersection angle
Circumference/diameter
Metal/ceramics PCB
Camera control software for DS-L1/DS-U1
Scene mode—optimal imaging with a single mouse click
Optimal imaging parameters have been preset for each sample type, therefore anyone, regardless of experience, can easily perform photography of the highest level.
Two-point distance
Scale
Point to line distance
Intersection angle
Circumference/diameter
Area
XY scale
Screen pattern (crossline, circle)
1918
Dimensional diagrams
LV-UEPI Universal Epi-illuminator LV-UEPI2 Universal Epi-illuminator 2
LV- DIA Dia Dase
1
0
0
I
N
0
0
1
0
0
O
U
T
95.5
267.090
508.5
387.2 326
193
78.1
341
456.8
134.5
36
250
25.5
J
APA
N
341
495
391
326
193
92
15176
250
140.5
95.5
LV-TI3 Trinocular
Tube ESD
LV-TT2 Tilting
Trinocular Tube
LV-CR Column Riser 35
LV-S6 6x6 Stage LV-S64 6x4 Stage
LV-SUB Stage
LV-NU5A
Nosepiece
LV-NCNT Nosepiece
Controller
LV-SUB Stage 2 LV-S32PL
ESD Plate
LV-S32SGH Slideglass
Holder
LV-S32 3x2 Stage
LV150A/LV150
LV100D
192.7 65.5
φ
60
φ
50
137.3
E.P.
20°
96.8
T
U
I
O
N
0
1
0
0
0
1
0
0
φ
51
60 67 202.5
205
186
17431
317
357
317
109
155 35
118
59
E.P.
118
103
82
92.5
54.55
73.7
264.6 66 31
138.3
20°
φ
100
153
φ10
φ
52
104
98.5
75
51
114
35
205.5
140.5
188
φ34
25.5
227
181
134
134
8445.5
JAPAN
140.5
φ34
109
25.5
34 φ
129 299
JAPAN
174
111129
40 31
45.5
φ
34
34
φ
217 25.5
299
25.5
109
205.5
188
140.5
45.5
φ
34
130
130
336
295
110
79.3
100
φ48
13
54
81.3
φ40
27660
61
25
57
29
336
295
95
110
54
81.3 79.3
13
27660
61
Cablelength220mm (cordbushexittoconnectorexit)
25
105
φ40
410.5
370
45°
40
25.5
100
φ48
300.5113.3
65
5
16
410.5
370
45°
40
300.5113.3
65
5
16
φ21
φ51
25.5
95
Cablelength220mm (cordbushexittoconnectorexit)
φ21
φ51
94
100
54
106
4-M4
470
)
35
39 (
57 12
74
120
ケーブル長
15°
:固定部より160mm
(89)
88
105
149
93.7
55.7
69
48
φ43 .5
15
φ127
50
50
74
30
66
8-M4
96
13
30.5
26.5 4
110
(182)
10°
28
111
48
122
88
5
171.5
167.5 71
171.5
122
88
26.5
76.5
4.7
100
φ60
250
55
341 367
φ62
127
250
φ48
116
115 73.5
20 21
LV150/150A
Main specifications
Main body Baseless type (spacer insertable between arm and stand); Max. sample height 47mm (when configured with 3x2 stage/6x4 stage),
82mm with column riser, 116.5mm with Suruga Seiki B23-60CR; 12V-50W brightness control transformer built in
Focusing section Coaxial coarse/fine focus knob, left: coarse/fine, right: fine; Stroke 40mm, coarse 14.0mm/rotation (torque adjustable, with
refocusing mechanism), fine focusing 0.1mm/rotation (1mm/increments)
Nosepiece C-N6 Nosepiece (brightfield, sextuple), L-NBD5 Nosepiece (bright/darkfield quintuple, with flare prevention), L-NU5 Nosepiece
(universal quintuple, with flare prevention), LV-NU5A Nosepiece (for LV150A, high-durability motorized universal quintuple, with flare prevention)
Episcopic illuminator 12V-50W high-intensity halogen lamp (ESD-applied); Field (centerable) and aperture diaphragms synchronized with B/D LV-U EPI changeover; ø25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer mountable
Episcopic illuminator 12V-50W high-intensity halogen lamp (ESD-applied); 120W high-intensity mercury-fiber illuminator (with brightness LV-U EPI2 control, no centering necessary) mountable; Centerable field and aperture diaphragms synchronized with B/D changeover;
f25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer/l plate insertable, excitation balancer insertable
Eyepiece tube LV-TI3 Trinocular (erect image, F.O.V. 22/25), LV-TT2 Tilting Trinocular (erect image, F.O.V. 22/25), Y-TF Trinocular (inverted
image, F.O.V 22/25), Y-TB Binocular (inverted image, F.O.V 22), C-TE Tilting Binocular (inverted image, F.O.V 22)
Stage LV-S32 3x2 Stage (stroke: 75x50 mm including glass plate), ESD-applied (excluding glass plate)
LV-S64 6x4 Stage (stroke: 150x100 mm including glass plate), ESD-applied (excluding glass plate) LV-S6 6x6 Stage (stroke: 150x150 mm; only for episcopic illumination)
Eyepiece CFI eyepiece series
Objective lens CFI60 series
Electrostatic decay time 1000-10V, within 0.2 sec.
Power consumption 1.2A/75W
Weight Approx. 8.6kg
LV100D
Main body Baseless type (spacer insertable between arm and stand); Max. sample height 29mm, 64mm with column riser; 12V-50W
brightness control transformer built in
Focusing section Coaxial coarse/fine focus knob, left: coarse/fine, right: fine; Stroke 30mm, coarse 14.0mm/rotation (torque adjustable, with
refocusing mechanism), fine focusing 0.1mm/rotation (1mm/increments)
Nosepiece C-N6 Nosepiece (brightfield, sextuple), L-NBD5 Nosepiece (bright/darkfield quintuple, with flare prevention), L-NU5 Nosepiece
(universal quintuple, with flare prevention)
Episcopic illuminator 12V-50W high-intensity halogen lamp (ESD-applied); Field (centerable) and aperture diaphragms synchronized with B/D LV-U EPI changeover; f25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer insertable
Episcopic illuminator 12V-50W high-intensity halogen lamp (ESD-applied); 120W high-intensity mercury-fiber illuminator (with brightness control, LV-U EPI2 no centering necessary) mountable; Centerable field and aperture diaphragms synchronized with B/D changeover; f25mm filter
(NCB11, ND16, ND4) insertable; Polarizer/analyzer/l plate insertable, excitation balancer insertable
Diascopic illuminator 12V-50W high-intensity halogen lamp; Field (centerable) and aperture diaphragms synchronized with B/D changeover; Filters
(ND8, NCB11) insertable
Eyepiece tube LV-TI3 Trinocular (erect image, F.O.V. 22/25), LV-TT2 Tilting Trinocular (erect image, F.O.V. 22/25), Y-TF Trinocular (inverted
image, F.O.V 22/25), Y-TB Binocular (inverted image, F.O.V 22), C-TE Tilting Binocular (inverted image, F.O.V 22)
Stage LV-S32 3x2 Stage (stroke: 75x50 mm including glass plate)
LV-S64 6x4 Stage (stroke: 150x100 mm including glass plate)
Eyepiece CFI eyepiece series
Objective lens CFI60 series
Electrostatic decay time 1000-10V, within 0.2 sec.
Power consumption 1.2A/75W
Weight Approx. 9.4kg
Polarizers/analyzers/plate
JAPAN
JAPAN
JAPAN
L.U
L.U
L.U
JAPAN
L.U
JAPAN
L.U
JAPAN
L.U
JAPAN
L.U
JAPAN
L.U
JAPAN
L.U
JAPAN
JAPAN
JAPAN
JAPAN
JAPAN
L.U
Objective lenses
YM-PO Polarizer LV-PO Polarizer
85.4 79
30
6.5
30
7.5
LV-FLAN FL Analyzer LV-P Plate
5°±'
4
30
6.5
λ板の
30
3
CFI LU PLAN FLUOR
CFI LU Plan Fluor EPI 5X CFI LU Plan Fluor EPI 10X
φ29
φ23.8
5
L.U
5X /
45°
36.5
φ20
JAPAN
WD
15A
23.5
M25x0.75
W.D.=23.5
CFI LU PLAN FLUOR BD
φ36 φ34
M32x0.75
φ30.8
5
JAPAN
0.2
L.U
35
5X /
3.95
φ27.6 φ35.5
15A
18
WD
W.D.=18
42
6.7
CFI L PLAN EPI CR
CFI L PLAN EPI 20XCR
φ35 φ33.5 φ29.5
φ27.5
(0.5)
5
11°
10.8
11.7
49.1
L
20X / 0.45
(45°)
φ20
φ31.5
JAPAN
0.6(CG)
21.1 5
W.D.=10.5
60
60
60.2
φ29
φ23.8
5
42.5
45
30°
0.2
4
JAPAN
L.U
10X /
30A
17.5
WD
φ17.5
φ36 φ34
φ30.8
JAPAN
L.U
10X /
30A
15
WD
φ25
CFI L PLAN EPI 50XCR
(0.5)
5
°)
7
(
14.5
13
56.1
L
15.56.5
45°
3
30°
3.1
W.D.=3.5
φ33.5
φ32 φ29 φ27
φ23.8
50X / 0.70
φ13 φ18.8 φ23.3
φ26 φ31.5
LV-UVPO Polarizer
85.4 85.4 79
307.5
47113.5
90
M25x0.75 M25x0.75
60
W.D.=17.5
M32x0.75 M32x0.75
60
W.D.=15
M25x0.75
60.2
JAPAN
0.6(CG)
10
CFI LU Plan Fluor EPI 20X
φ29
φ23.8
5
JAPAN
L.U
20X /
55.5
55.5 5
50°
51
45A
60
4.5
WD
4.5
φ9
φ36 φ34
φ30.8
0.2
JAPAN
L.U
20X /
45 A
60
4.5
WD
4
φ26.2 φ33.5
W.D.=4.5
CFI L PLAN EPI 100XCRA
φ35.5
φ34 φ29.5 φ28.5
(0.7)
5
)
°
14.313226.225
(16
58.7
L
°
45
6.5
° 5 2
φ11.5
W.D.=1.1
φ19.8 φ24.8
φ27 φ32.5
100X / 0.35
79
CFI LU Plan Fluor EPI 50X
59
54
59 5
JAPAN
L.U
47.5
50X /
45°
°
4.5
40
2.3
(Overheadscrew)
φ40 φ35
φ30.8
0.5
L.U
50X /
35°
3
(φ28.4)
φ37
M25x0.75-6g
60.1
0.3(CG)
φ30
φ23.8
φ8.5
φ17.5 φ21.8
φ24
40.4
JAPAN
WD
80 A
JAPAN
WD
1.0
80A
1.0
L-AN Analyzer
30
6.5
CFI LU Plan Fluor EPI 100X
M25x0.75
47.5
59
60
W.D.=1
M32x0.75
60
W.D.=1
CFI L PLAN EPI 100XCRB
(0.7)
(16
14.313226.4
58.2 5W.D.=1.2
4
2
1.8
°)
°
5
6.5
° 6
CFI LU Plan Fluor BD 100XCFI LU Plan Fluor BD 50XCFI LU Plan Fluor BD 20XCFI LU Plan Fluor BD 10XCFI LU Plan Fluor BD 5X
59 5
L
45°
4.5
0° 3
3.5
(Overheadscrew)
0.5
54
35°
3
φ35.5
φ34 φ29.5 φ28.5 φ23.8
100X / 0.35
JAPAN
φ14.5
φ19.8 φ24.8
φ27
φ32.5
100X /
φ23.8
L.U
100X /
φ21.8
40.4
φ40 φ35
φ30.8
L.U
(φ28.4)
φ37
M25x0.75
0.9(CG)
90
φ30
φ8.8
φ18
φ24
JAPAN
60.3
M25x0.75
JAPAN
WD
90A
60
1.0
W.D.=1
M32x0.75
90 A
1.0
WD
60
W.D.=1
22 23
System diagram
LV150/LV150A LV100D
D-FB
ND4ND16
NCB11
λ
OUT
IN
F
F
E
A
B
A
F
E
B
I I’
I’
I’
F
E
OP
P'
T
Q
Q'
R
Q
S
O
T
Q'
R
S
*Not necessary on the LV150A as the operation unit has been built into the main body.
Fiber
External Power Supply
S
I
P
P'
POWER
MIN. MAX.
Photomicrographic System FX-III Series
ENG-mount CCTV Camera C-mount CCTV Camera
Camera Mount
V-T Photo Adapter
Projection Lenses PLI 2x PLI 2.5x PLI 4x PLI 5x
ENG-mount CCTV Adapters
0.45x
0.6x
ENG-mount CCTV Adapter
Relay Lens 1x
ENG-mount Zooming Adapter
Zooming Lens
C-mount Zooming Adapter
C-mount CCTV Adapter
Relay Lens 1x
C-mount CCTV Adapters
0.35x
0.45x
0.6x
0.7x
C-mount CCTV Adapter VM2.54x
C-mount CCTV Adapter VM4x
C-mount Direct CCTV Adapter
C-mount Adapter A
0.7x
DXM1200F
DS-5M DS-2M
LV-TV TV Tube
C-mount Adapter
0.55x
0.5x 2nd Objective
Y-TB Binocular Tube
Other Eclipse series eyepiece tubes can be used.
LV-TI3 Trinocular Tube ESD
LV-TT2 Tilting Trinocular Tube
Eyepiece Tubes
Epi-fluorescence Accessories
C-FL Fluorescence Filter Block
L-AN Analyzer
YM-PO Polarizer
LV-FLAN FL Analyzer
LV-λP λPlate
LV-PO Polarizer
LV-UVPO Polarizer
D-FB Excitation Light Balancer
NCB Slider
ND Slider
Adapter
CFI UW 10x
CFI UW 10x M
F.N.ø25
F.N.ø22
CFI 15x
C-CT
Centering
Telescope
CFI
12.5x
CFI
10xCM
CFI
10xM
CFI 10x
L-W
10x
ESD
Filar Micrometer 10xN
Eyepieces
LV-SUB Substage
Surugaseiki B23-60CR
LV-SUB Substage 2
LV-CR Column Riser 35
C-ER Eyelevel Riser
Y-IDP Double Port (100:0 / 55:45)
Y-IDP Double Port (100:0 / 0:100)
LV-UEPI Universal Epi-Illuminator
LV-UEPI2 Universal Epi-Illuminator 2
Intermediate Modules
L-S6WH Wafer Holder
L-S6PL ESD Plate
LV-S32SGH Slidegalss Holder
LV-S32PL ESD Plate
LV-S6 6x6 Stage
LV-S64 6x4 Stage
LV-S32 3x2 Stage
Stages
LV-LH50PC Precentered Lamphouse
D-LH 12V-100W Precentered Lamphouse (Requires TE2 External External Power Supply)
C-HGF Fiber Adapter
LV-HL50W 12V-50W-LL Halogen Lamp
12V-100W Lamp
100W TE2 Power Supply
Lamphouses
L-DIC DIC Prism
L-DIHC High Contrast DIC Prism
LV-NU5A Motorized Nosepiece
L-NU5 U5 Nosepiece
L-NBD5 DB5 Nosepiece
C-N C-N6 Nosepiece
P-N P-N5 Nosepiece
Adapter
LV-NCNT Nosepiece Controller*
LV-NCNT Nosepiece Controller Cable 10m
LU Plan Fluor BD Objective
LU Plan Fluor EPI Objective
LU Nosepiece Adapter M32-25
C-OA 15MM Adapter
DI Objective
CFI L/LU EPI P Objective
TI Objective Adapter
Nosepieces
C
D-FB
ND4ND16
NCB11
λ
OUT
IN
F
F
E
A
F
E
B
I
F
E
OP
P'
T
Q
Q'
R
Q
S
I’
O
T
Q'
R
S
LV-S32 3x2 Stage
鏡筒
S
I
P
P'
A
B
I
C
カメラマウント
TE2-PS100W Power Supply (YM-EPI3 3-pin extension cord is required)
POWER
MIN. MAX.
POWER
MIN. MAX.
I I’
I’
Photomicrographic System FX-III Series
ENG-mount CCTV Camera C-mount CCTV Camera
Camera Mount
V-T Photo Adapter
Projection Lenses PLI 2x PLI 2.5x PLI 4x PLI 5x
ENG-mount CCTV Adapters
0.45x
0.6x
ENG-mount CCTV Adapter
Relay Lens 1x
ENG-mount Zooming Adapter
Zooming Lens
C-mount Zooming Adapter
C-mount CCTV Adapter
Relay Lens 1x
C-mount CCTV Adapters
0.35x
0.45x
0.6x
0.7x
C-mount CCTV Adapter VM2.54x
C-mount CCTV Adapter VM4x
C-mount Direct CCTV Adapter
C-mount Adapter A
0.7x
DXM1200F
DS-5M DS-2M
LV-TV TV Tube
C-mount Adapter
0.55x
0.5x 2nd Objective
Y-TB Binocular Tube
Other Eclipse series eyepiece tubes can be used.
LV-TI3 Trinocular Tube ESD
LV-TT2 Tilting Trinocular Tube
Eyepiece Tubes
Epi-fluorescence Accessories
C-FL Fluorescence Filter Block
L-AN Analyzer
YM-PO Polarizer
LV-FLAN FL Analyzer
LV-λP λPlate
LV-PO Polarizer
LV-UVPO Polarizer
D-FB Excitation Light Balancer
NCB Slider
ND Slider
Adapter
CFI UW 10x
CFI UW 10x M
F.N.ø25
F.N.ø22
CFI 15x
C-CT
Centering
Telescope
CFI
12.5x
CFI
10xCM
CFI
10xM
CFI 10x
L-W 10x
ESD
Filar Micrometer 10xN
Eyepieces
C-SP Simple Polarizing Polarizer
LV-CR Column Riser 35
C-ER Eyelevel Riser
Y-IDP Double Port (100:0 / 55:45)
Y-IDP Double Port (100:0 / 0:100)
LV-UEPI Universal Epi-Illuminator
LV-UEPI2 Universal Epi-Illuminator 2
Intermediate Modules
LV-S32SGH Slidegalss Holder
LV-S32PL ESD Plate
LV-S64 6x4 Stage
Stages
LV-LH50PC Precentered Lamphouse
D-LH 12V-100W Precentered Lamphouse (Requires TE2 External Power Supply)
C-HGF Fiber Adapter
LV-HL50W 12V-50W-LL Halogen Lamp
12V-100W Lamp
100W TE2 Power Supply
Lamphouses
L-DIC DIC Prism
L-DIHC High Contrast DIC Prism
L-NU5 U5 Nosepiece
L-NBD5 DB5 Nosepiece
C-N C-N6 Nosepiece
P-N P-N5 Nosepiece
External Power Supply
LU Plan Fluor BD Objective
LU Plan Fluor EPI Objective
LU Nosepiece Adapter M32-25
C-OA 15MM Adapter
DI Objective
CFI L/LU EPI P Objective
TI Objective Adapter
Adapter
Nosepieces
DF (dry)
D-C Abbe
C-C Achromat
LWD Achromat
Slide (Swing-out??) Achromat 2-100x
Condensers
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