Transcript
Industrial Microscopes ECLIPSE LV150/LV150A/LV100D/LV100DA LV Focusing Modules LV-IM/LV-IMA/LV-FM/LV-FMA
Industrial Microscopes
LV Focusing Modules
MEMS
Semiconductors
Materials
Extend Your Vision
Versatility
• Bare wafers • Lithography process • Probe, test processes • Post-dicing
• Printer heads • Micro sensors • Optical switches • GMR heads for HDD
IC Packages
• LF/TAB • WL-CSP • QFP • SIP • BGA, CSP, FC
• Macromolecules, monomeric materials • Organic/inorganic materials • Polymers • Thin film • Magnetic materials • Crystals • Metallography
Casts and Parts LV-ECON
LV-IMA • OA equipment parts • Cell phones, PDAs, DSC, PC parts • Automobiles, aeronautics (To be released in Feb. 2006)
(To be released in Feb. 2006)
A versatile microscope system with a modular design PCB
Precision Molds
FPD
Improved Performance
Optical Performance • Medium/small PCB • FPC • Interposer substrates 2
Display Devices
• Precision molds
• LCD, color filters • Polarizing filters • Organic EL
• CCD • LCOS
• CMOS • DMD 3
Versatility 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.
Modular Design Major parts of the microscope main body—arm, stand, base, etc.—have been modularized for greater flexibility according to use. The LV-ARM Basic Arm, LV-FM FM Module, LV-FMA FM Module A, LV-EPI Epi Base, and LV-DIA Dia Base can be freely combined or incorporated into the system.
LV-ARM Basic Arm
LV-FMA FM Module A (motorized)
LV-FM FM Module (manual)
LV-EPI Epi Base
LV-DIA Dia Base
Modular Design
If the LV-DIA Dia Base is used, a diascopic illuminator can be incorporated into the system*. * An optional power source, the TE2-PS100W, and related options are needed to perform diascopic illumination.
Roll-out section
Roll-in section Tape-suction section
Tape-transport section Stage section
An example configuration of the LV150
An example of the LV-DIA Dia Base incorporated into a tape-transport sample inspection system.
Versatility 4
Accepts Thicker 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.
Users can select suitable models based on sample and stage stroke. All stages are highly durable with their triple-plate design.
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 LV-S32 3x2 Stage illumination.
82mm
47mm
Extensive Range of Industrial Stages and Accessories
Stroke: 75 x 50 mm
Without column riser
With column riser
Non-Nikon Stages (LV150 or LV150A only)
LV-S32PL ESD Plate (for LV-S32 3x2 Stage)
LV-S32SGH Slideglass Holder (for LV-S32 3x2 Stage)
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 thicker samples of up to 116.5 mm, thereby enabling the observation of fiber ends and other tools. LV-S64 6x4 Stage Stroke: 150 x 100 mm
LV-S6 6x6 Stage Stroke: 150 x 150 mm
Combination of LV-150 with LV-SUB Substage 2 and Suruga Seiki B23-60CR stage
L-S6WH Wafer Holder (for LV-S6 6x6 Stage)
LV-SUB Stage (exclusive for LV150/LV150A)
L-S6PL ESD Plate (for LV-S6 6x6 Stage)
LV-SUB Substage 2 (exclusive for LV150/LV150A)
Appropriate holder and substage are selected based on sample and stage combination. 5
Extend Your Vision A wide variety of observation methods are available with the Eclipse LV series. Observation with first-order red compensator, UV polarizing, and epi-fluorescence observation with UV excitation, in addition to brightfield, darkfield, DIC, simple polarizing, epi-fluorescence (excitation using visible light) and double-beam interferometry are all possible. A new motorized illuminator has been added to the existing manual type. A 12V-50W halogen light source—equivalent to or even brighter than the 12V100W type—and a high-intensity mercury fiber light source are available. The inclusion of a compact and lightweight white LED illuminator exclusively for brightfield use gives you the option of selecting the most appropriate combination for your purpose.
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.
Universal Epi-Illuminator 2: LV-UEPI2 The LV-UEPI2 universal episcopic illuminator is equipped with advanced optics suitable for a wide variety of observation methods—brightfield, darkfield, DIC and epifluorescence. It allows the operator to concentrate on the observation by automatically maintaining optimal illumination conditions for the aperture diaphragm, shutter, filters, including diffuser and ND filter.
• Brightfield • Darkfield • Simple polarizing • DIC • Double-beam interferometry
Motorized Universal Epi-Illuminator 2: LV-UEPI2A In this illuminator, the illumination changeover turret and the aperture diaphragm, as well as the illumination voltage control, have been motorized, for accurate reproduction of illumination—therefore, images can be taken under consistent illumination. Aperture is automatically optimized according to the objective and illumination technique in use. It can, however, also be changed manually depending on the sample and purpose. When configured with the LV100DA microscope, this illuminator can be controlled on the microscope or from the connected PC. Control from the PC is possible when the illuminator is incorporated into the system using the LVECON E controller.
• Brightfield • Darkfield • Simple polarizing • Observation with first-order red compensator • DIC • Epi-fluorescence (UV excitation possible) • UV polarizing epi-fluorescence • Double-beam interferometry
• Brightfield • Darkfield • Simple polarizing • Observation with first-order red compensator • DIC • Epi-fluorescence (UV excitation possible) • UV polarizing epi-fluorescence • Double-beam interferometry
Optimal Illumination Function Field diaphragm
Aperture diaphragm
Shutter
UV-cut 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
—
LV-PAB PA Cube With a polarizer and analyzer attached in the shape of a crossed Nicol prism, this cube is used for DIC observations. It is used by installing it into the turret of the LV-UEPI2 or LV-UEPI2A epi-illuminator; to begin observations simply insert a DIC slider into the optical path.
Extend your v 6
High-Intensity 12V-50W Halogen Light Source: LV-LH50PC Precentered Lamphouse Although the LV-LH50PC Precentered Lamphouse is 12V50W, the brightness is equivalent to or higher than that of 12V-100W. The low power-consumption halogen light source contributes to the compact design of the microscope while also being friendly to the environment. Defocus induced by heat is substantially reduced.
High-intensity Mercury Fiber Light Source (for LV-UEPI2/LV-UEPI2A) Use of the fiber light source eliminates the centering process when replacing the lamp and reduces the influence of heat to the microscope. Brightness can be mechanically adjusted in 5 steps from 0-100%. Two types are available: manual type and PC-control type that enables external control via RS-232C interface. When configured with the LV150A or LV100DA microscope, use the PC-control type that enables control via the LV-ECON controller.
Manual control type
Why is 50W brighter than 100W? Image brightness is not determined by wattage. Nikon’s new light source delivers greater brightness by optimizing the lamp filament size and improving pupil illumination fulfillment by optically expanding the size of the light source. This has resulted in a 50W light source that is brighter than a 100W lamp. With 50x or higher objectives, brightness is about 20% greater under episcopic illumination, 40-50% greater with diascopic illumination, than previous Nikon illuminators.
LV-EPILED White LED Illuminator With emphasis on light weight and compact design, this white LED illuminator was specially developed for brightfield use. It is operated via the attached power source controller. By using the LV-ECON E controller, external control is also possible.
ision
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Optical Performance Improved Transmission Rate for UV Wavelength CFI LU Plan Fluor series The transmission rate in the UV wavelength range has been improved for the new CFI LU Plan Fluor series. 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 first-order red compensator, DIC and UV epifluorescence observations. These objective lenses, which offer high resolution and easy-to-use performance, can be combined not only with microscopes but also with other equipment for even greater versatility.
CFI60 LU Plan Fluor EPI series
Objective Lenses with Correction Ring
ptical Performance
CFI L Plan EPI CR series
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CFI60 LU Plan Fluor BD 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. CFI60 L Plan EPI CR series of objective lenses with correction ring
Environment 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.
Without correction (50x)
CFI60 Series Objectives Brightfield Model CFI L Plan EPI CFI LU Plan Fluor EPI
CFI LU Plan EPI ELWD
CFI L Plan EPI SLWD
CFI LU Plan Apo EPI CFI L Plan Apo EPI WI
Bright/darkfield Magnification 2.5X 5X 10X 20X 50X 100X 20X 50X 100X 20X 50X 100X 100X 150X 150X
NA 0.075 0.15 0.30 0.45 0.80 0.90 0.40 0.55 0.80 0.35 0.45 0.70 0.95 0.95 1.25
Working Distance (mm) 8.8 23.5 17.5 4.5 1.0 1.0 13.0 10.1 3.5 24.0 17.0 6.5 0.4 0.3 0.25
Model CFI LU Plan Fluor BD
CFI LU Plan BD ELWD
CFI LU Plan Apo BD
With correction mechanism Model CFI L Plan EPI CR CFI L Plan EPI CR CFI L Plan EPI CRA CFI L Plan EPI CRB
With correction at 0.7 mm (50x)
Magnification 20x 50x 100x 100x
NA (mm) 0.45 0.7 0.85 0.85
Magnification 5X 10X 20X 50X 100X 20X 50X 100X 100X 150X
NA 0.15 0.30 0.45 0.80 0.90 0.40 0.55 0.80 0.90 0.90
Condensers Product Name
Working Distance (mm) 10.9-10.0 3.9-3.0 1.2-0.85 1.3-0.95
Glass Thickness Correction Range 0-1.2mm 0-1.2mm 0-0.7mm 0.6-1.3mm
Working Distance (mm) 18.0 15.0 4.5 1.0 1.0 13.0 9.8 3.5 0.51 0.4
LWD Achromat condenser C-C Slide Achromat condenser 2-100X C-C Abbe condenser C-C Achromat condenser Darkfield (dry) condenser
N.A. 0.65 0.9 0.9 0.85 0.8-0.95
W.D. (mm) 10.2 1.2-2.2 1.9 4.2 4
Improved Performance Overall performance has been improved with better durability and rigidity.
Thorough ESD Protection
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 positions. The optical path changeover of 100:0/20:80 allows simultaneous use of monitor. *C-mount adapter 0.55x can be directly mounted to LV-TT2 and LV-TI3 for the DS-2M series.
Highly Durable Motorized Universal Nosepieces
All parts of the microscope that might be touched, including the body, tube and stage, have been insulated. This improves anti-contamination and prevents samples from being harmed by electrostatic, thereby improving yields. Electrostatic decay time: 1000-10V, within 0.2 sec.
LV-NU5A Nosepiece
LV-NU5AC Nosepiece
LV-NU5A and LV-NU5AC Nosepieces Two types of motorized universal quintuple nosepieces are available. The LV-NU5A boasts greater durability thanks to a new click mechanism and control system. The LV-NU5AC comes with a centering mechanism that suppresses image drift during objective changeover. These nosepieces can not only be configured with the LV150A or LV100A microscope, but also incorporated into other devices in combination with the LV-NCNT nosepiece controller and LV-ECON controller.
Manual Nosepiece A variety of manual control nosepieces are available to suit all needs.
C-N6 Nosepiece (Brightfield)
L-NBD5 Nosepiece (Bright/darkfield)
L-NU5 Nosepiece (Universal)
Highly Rigid, Vibration-Free Body The use of structural analysis during the design process has improved rigidity and anti-vibration parameters to yield clear images even at high magnification.
mproved Performance
Tilting Trinocular Eyepiece Tube
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A motorized system that optimizes image capturing conditions—
An example configuration of the LV100DA
LV100DA Interface Motorized universal illuminator
USB1.1
High-intensity mercury fiber illuminator
Among performance requirements demanded of a microscope, those associated with digital imaging— digital image capture, analysis, and database formation—are growing faster than ever before. The LV100DA motorized system squarely addresses these demands and now comes equipped with a mechanism that automatically optimizes observation technique and illumination—and these settings can be quantitatively controlled from external devices.
TE2-PS 100W power supply (simultaneous epi/dia illumination)
Auto Optimization of Illumination In configuration with the LV-UEPI2A motorized universal illuminator, the system automatically sets optimum illumination conditions for the objective and observation technique in use, for quick recall of observation conditions.
Synchronized control window (setup software)
Motorized universal illuminator
Objective lens window (setup software)
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LV100DA, Focusi
Focusing Modules and Controller Amply Support Motorized Control Four types of new focusing modules are available. • For incorporation into system: LV-IMA IM Module A (motorized) LV-IM IM Module (manual) • For incorporation into microscope: LV-FMA FM Module A (motorized) LV-FM FM Module (manual) The new offerings complement Nikon’s rich variety of modular units—such as the LV-UEPI2A Motorized Universal Illuminator, LVNU5A Motorized Universal Nosepiece, LV-NU5AC Motorized Universal Nosepiece with centering mechanism, and LV-ECON E Controller—to give you greater flexibility in configuring a system best suited to your purpose.
LV-IMA IM Module A (motorized)/LV-IM IM Module (manual)
LV-IMA IM Module A
An example configuration of the LV-IMA LV-IM IM Module
These modules are suitable for incorporation into systems. The position for the mounting screw holes is selectable from the back or bottom. • The LV-IMA IM Module A (motorized) has a vertical stroke of 20mm, while the LV-IM IM Module (manual) has one of 30mm. • To ensure a good grip of hefty modules such as the LV-UEPI2A motorized universal illuminator, the rigidity of the modules has been greatly enhanced. • The LV-IMA IM Module A (motorized) can be externally controlled via the LV-ECON E controller.
LV-FMA FM Module A (motorized)/LV-FM FM Module (manual)
Nosepiece moves up and down.
LV-FMA FM Module A
An example configuration of the LV-FMA
LV-FM FM Module
These modules are suitable for incorporation into microscopes. Mounting screw holes are located on the bottom of the units only. • The LV-FMA FM Module A (motorized) has a 20mm vertical stroke. When configured with the LV-EPI Epi Base or the LV-DIA Dia Base, it turns your microscope into a system with a motorized nosepiece up/down mechanism; the system can be externally controlled via the LV-ECON E Controller. • The combination of the LV-FM FM Module (manual; 30mm vertical stroke) and the LV-EPI Epi Base creates a system with a nosepiece up/down mechanism that has an ultra-long vertical stroke of 68mm—it facilitates operations such as semiconductor probe inspections.
ng Module
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LV-ECON E Controller This controller provides interface to externally control the light source, motorized illuminator, nosepiece, focusing module and other motorized units from the connected PC and other devices. Communication between this and the PC is established via USB1.1 It is also possible to manually operate the connected units from the front panel. A Software Development Kit (SDK) is available to support the user in creating software for proper incorporation and operation of the units. * Nikon’s warranty covers Nikon equipment only.
Interface • Motorized universal illuminator, LV-UEPI2A • Halogen lamphouse, LV-LH50PC (TE2-PS100W power supply is required) • PC-control type high-intensity mercury fiber light source • White LED illuminator, LV-EPILED • Motorized universal nosepiece, LV-NU5A, LV-NU5AC (with centering mechanism) • Motorized focusing module, LV-IMA IM Module A • Motorized focusing module, LV-FMA FM Module A • USB1.1
LV-UEPI2A Motorized Universal Illuminator LV-EPILED White LED Illuminator
LV-IMA IM Module A
LV-NU5AC Nosepiece LV-ECON Controller
LV-NU5A Nosepiece LV-FMA FM Module A
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(Episcopic Illumination Type) LV-TI3 Trinocular Tube A trinocular tube with an optical path changeover of 100:0/0:100.
LV-LH50PC Precentered Lamphouse A low power-consumption 12V-50W halogen light source equivalent to or higher than the 12V-100W type.
CFI-Series Eyepiece
LV-UEPI An illuminator that can be used for brightfield, darkfield, simple polarizing and DIC observations.
LV150/LV150A The LV150 and LV150A microscopes are used for episcopic illumination.
LV-NU5A Nosepiece A universal motorized nosepiece that is 10 times more durable than its predecessors.
CFI LU Plan Fluor Series These objective lenses feature high NA, long working distances and improved transmission rate in the UV range.
LV-S6 6x6 Stage An episcopic illumination stage capable of inspecting 150mm wafers. (With 6” wafer holder)
L150A controls An example configuration of the LV150A
Motorized nosepiece controls
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(Episcopic/Diascopic Illumination Type)
LV-TT2 Tilting Trinocular Tube The LV-TT2 is a tilting trinocular tube that has an optical path changeover of 100:0/20:80.
LV-LH50PC 12V-50W Lamphouse A low power-consumption 12V-50W halogen light source equivalent to or higher than the 12V-100W type.
CFI-Series Eyepiece
LV-UEPI2 LV100D
The LV-UEPI2 illuminator enables brightfield, darkfield, DIC, simple polarizing, and UV excitation epi-fluorescence observations.
The LV100D microscope is capable of episcopic and diascopic illumination.
Nosepiece CFI LU Plan Fluor Series
Selectable from C-N6 (brightfield), L-NBD5 (bright/darkfield) and LNU5 (universal) nosepieces.
These objective lenses feature high NA, long working distances and improved transmission rate in the UV range.
LV-S32 3x2 Stage This small, industrial-use stage has a triple-plate design and can be used for episcopic and diascopic illumination.
An example configuration of the LV100D
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(Episcopic/Diascopic Illumination Type) LV-TT2 Tilting Trinocular Tube The LV-TT2 is a tilting trinocular tube that has an optical path changeover of 100:0/20:80.
LV-LH50PC 12V-50W Lamphouse A low power-consumption 12V-50W halogen light source equivalent to or higher than the 12V-100W type.
CFI-Series Eyepiece LV100DA Compatible with both episcopic and diascopic illumination and supports the LV-UEPI2A motorized universal epi-illuminator and motorized nosepiece.
LV-UEPI2A This illuminator controls the illumination changeover turret and aperture diaphragm via a motor. The diaphragm is automatically optimized according to the objective in use.
Nosepiece The LV-NU5AC motorized nosepiece comes with a centering mechanism that minimizes image drift during objective changeover.
CFI LU Plan Fluor Series These objective lenses feature high NA, long working distances and improved transmission rate in the UV range.
LV-S64 64 Stage Compatible with both episcopic and diascopic illumination, this stage accommodates samples up to 150 x 100mm.
LV100DA controls
An example configuration of the LV100DA
Enable motorized control of motorized nosepiece, illumination changeover turrets, aperture diaphragm, light source (epi/dia), etc.
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Observation Methods Simple Polarizing
Brightfield
In addition to simple polarizing, a lambda plate can be inserted into the optical path to achieve firstorder red compensator observation. This is useful for liquid crystal inspections (when used in combination with the LVUEPI 2).
The antiflare design applied to the objective lenses and light source ensures bright, and 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
YM-PO Polarizer
L-AN Analyzer
LV-PO Polarizer
LV-FLAN FL Analyzer
LV-P Plate
Epi-Fluorescence UV, V, BV, B or G excitation fluorescence filter blocks can be selected. This method is perfect for the observation of OLED, ion migration and other substrate uses.
L-DIC DIC Prism (standard)
YM-PO L-AN L2-DIC L-DIHC Polarizer Analyzer DIC Prism High-contrast DIC Prism
L-DIHC DIC Prism (high contrast)
Standard or high contrast DIC sliders can be selected to suit the sample. This method is useful for the surface observations of various devices LV-PAB PA and precision Cube molds.
Double-Beam Interferometry Equipment (measures nano scale height gaps)
Brightfield
LV-FLAN FL Analyzer
Diascopic Illumination Diascopic illumination is used to observe optical parts, FPD and other samples that transmit light.
Condensers
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LV-UVPO Polarizer
Fluorescence filter blocks
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.
Episcopic double-beam Interferometry Equipment TI/DI
Epi-fluorescence B-2A
Applications Semiconductor (wafer)
Semiconductor (wafer)
MEMS (optical switch)
Micro Bump
Brightfield
Darkfield
Brightfield
Brightfield
Compact Disc (CD)
Image Sensors (CCD)
PCB (ion migration)
PCB (ion migration)
Simple polarizing
Brightfield
Brightfield
Epi-fluorescence
PCB
PCB
Precision Mold
LCD (color filter)
Brightfield
Epi-fluorescence
DIC
Diascopic brightfield
LCD (conductive particle)
Test reticle
Spodumene
Carbon Paper
DIC
Diascopic brightfield
DIC
Brightfield
Nodular Graphite Cast Iron
Tourmaline
Tourmaline
Tourmaline
DIC
Brightfield
DIC
Double-beam interferometry 17
Eyepiece Tubes
Illuminators
White LED Illuminator
Polarizing/DIC accessories Simple Polarizing
Observation with First-Order Red Compensator
UV Polarizing with EpiFluorescence
DIC
LV-UV PO UV Polarizer
YM-PO L-AN L2-DIC Polarizer Analyzer DIC Prism
LV-UEPI LV-TI3 Trinocular Eyepiece Tube
LV-EPILED
LV-TT2 Tilting Trinocular Eyepiece Tube
Eyepieces Model
F.O.V.
CFI 10x
22
Double Port
Remarks
CFI 10xM
22
Photomask included
CFI 10xCM: for C-TE binocular ergo tube
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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
YM-PO Polarizer
L-AN Analyzer
LV-PO LV-FLAN FL LV-P Polarizer Analyzer Plate
L-DIHC DIC Prism HC
LV-UEPI2
Substages (LV150/LV150A)
LV-UEPI2A
Y-IDP Double Port (Ratio 100:0/55:45) Y-IDP Double Port 0/100 (Ratio 100:0/0:100) LV-PAB PA Cube LV-S6 6x6 Stage
Nosepieces
LV-S64 6x4 Stage
LV-S32 3x2 Stage
Substages (for LV150/LV150A) C-N6 Nosepiece (Brightfield)
L-NBD5 Nosepiece (Bright/darkfield)
L-NU5 Nosepiece (Universal)
LV-NU5A Motorized Nosepiece (Universal)
LV-NU5AC Motorized Nosepiece (Universal; with centering mechanism)
IN
OUT
0 100
LV-SUB Stage
LV-SUB Stage 2
100 0
Holders For LV-S6 6x6 Stage
Objective Lenses
L-S6WH Wafer Holder CFI LU PLAN FLUOR EPI series
For LV-S32 3x2 Stage
L-S6PL ESD Plate
LV-S32PL ESD Plate
LV-S32SGH Slideglass Holder
CFI L PLAN EPI CR series
Arm
Focusing Modules
CFI LU PLAN FLUOR BD series
Objective Adapters LV-ARM Basic Arm LU Objective Adapter M32-25
LV-FM FM Module (manual)
LV-FMA FM Module (motorized)
C-OA 15mm Adapter
Bases Diascopic Illumination Condensers
LV-EPI Epi Base LWD Achromat
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Slide Achromat 2-100x
C-C Abbe
C-C Achro
Darkfield (Dry)
LV-DIA Dia Base
Modular Design
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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.
PC-Connection Type
Standalone Type
This type requires connection to PC and allows observation on a PC monitor, image capture, measurement and analysis when the special application software ACT-2U is used.
This type comes with an LCD monitor, making it convenient for on-screen monitoring without PC and in applications that require long/multiple exposures.
Real-time 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
Real-time imaging Camera—DS-2Mv-U1 • Live image display at 12fps (800 x 600) max. • Image size: 1600 x 1200 pixels • PC connection via USB2.0 • Dedicated application software—ACT-2U
*1: A CP900DC dedicated printer and C-mount adapter are necessary. Provided with real 10 mode (10X printing).
Dedicated camera control software ACT-2U
*2: FTP Client/Server, HTTP Server Telnet Server functions provided.
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. Metal/Ceramics
Wafer/IC Chip
PCB
A host of measuring tools Two-point distance
Scale
Point to line distance
Intersection angle
Area (DS-U1 only)
XY Scale
Screen pattern (crossline, circle)
XY measurement (DS-L1 only)
Circumference/diameter
*Dedicated ACT-2U camera control software is necessary when using the DS-U1.
Camera Heads The following four camera heads are available in addition to the DS-2Mv to suit your sample and application.
For brightfield, darkfield, DIC observations
For fluorescence observations (that require long exposure)
DS-2MBW
DS-5M
DS-2MBWc
• Image size: 1600 x 1200 pixels • 15 fps (30 max.) • Superb movie • Sensitivity 5 times greater than before
• Image size: 2560 x 1920 pixels • True-to-life recording of minute images
• Image size: 1600 x 1200 pixels • Image size: 2560 x 1920 pixels • Sensitivity approx. 5 times greater • Includes a Peltier device than predecessors • Brilliant images with minimum noise • Includes a Peltier device • Brilliant images with minimum noise
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DS-5Mc
D
Ultrahigh-definition 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 the advanced R&D fields.
• Approx. 12 million output pixels comparable to highend film 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.
Camera Control Software
ACT-1 Minimizes fatigue during large-volume and 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.
Option: Camera Control Software
ACT-2U The optional ACT-2U software offers the following arrays of convenient measurement tools.
Two-point distance
Circumference/diameter
Scale
Area
Point to line distance
XY Scale
Intersection angle
Screen pattern (crossline, circle)
Digital Camera
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Dimensional Diagrams Unit: mm
LV150A/LV150 96
IN
OUT
0
100 0
36
134.5
326 78
193
387.2
508.5
100
341
250
457 90
267
LV100D
92
193
JA P A N
140.5
326
25.5
391
495
96
341
250 484
76
151
LV100DA
92
193
140.5
326
391
495
96
341
250 484
115
22
73.5
LV-IMA IM Module A (motorized)
LV-IM IM Module (manual) 95 95 55
49(48∼78) 25
30
87
138.8 87
138.8
20
65.5
2
65.5 49(48∼68) 25
40
50
Nosepiece port
170
A □
170 2-M4 深8
70
Nosepiece port
90
80
Eyepiece tube port
Eyepiece tube port
2
0 10
Vertical stroke: up 29, down 1
60
55 Vertical stroke: up 19, down 1
A □
47
47 80±0.1
104
42
42
95±0.1 114
60 80±0.1
42
120±0.1
4-M6 depth 10
95±0.1 114 120.7
9
4-M6 depth 10
80±0.1
9
42 60 80±0.1
120±0.1
2-M4 depth 8
3.4
2-φ 9d
62±0.1 10
(2R4 )
φ 8H 7
4-M6 Screw depth: less than A surface 9mm from
3.4
+ 0 0.01 5
18
10
62±0.1
(2-
R4 )
de
pt
h
φ
4-M6
3. 4
8H
7
+ 0 0.0 15
de pt h
LV-FM FM Module (manual)
80±0.1
31 28 18 26
-0.001
φ8 -0.041
62±0.1 18
pth
de 3.4
LV-UEPI Universal Epi-Illuminator
A □
95
260
(2-R4) 10
2φ
2-φ
9d ep
113 163.5
225(224∼254)
113 163.5 4-M6 Screw depth: less than A surface 9mm from
55
5 .01 +0
.4 10
114
70
th 3
dep
(2-R4)
A □
8H φ
5 .01 +0 0
H7
φ8 62±0.1 18
Nosepiece port Vertical stroke: up 18.5 down 1
80±0.1
φ8+0.001 0.041 95
260
8 +0.015 depth 3.4 0
18 26 114
Fixed plate thickness
Vertical stroke: up 19 down 1
55
126.5±0.1 308
48
4-M6
31 28
25 Nosepiece port
225(224∼244)
Eyepiece tube port
104
120.7
Screw depth: less than A surface 9mm from
308
25
48
Eyepiece tube port
114
80±
126.5±0.1
Fixed plate thickness
80±0.1
114
80±
4-M4 depth 8
LV-FMA FM Module A (motorized)
3. 4
4-M4 depth 8
Screw depth: less than A surface 9mm from
8+0.015 depth 3.4 0 80±0.1
18
epth
80±0.1 8 +0.015 depth 3.4 0
epth
80±0.1
9d
depth 3.4 8+0.015 0
2-φ
th
3.4
9
de
pth
3. 4
LV-UEPI2 Universal Epi-Illuminator 2 510
336
370
25.5
110
0 φ4
105
400
Cable length 220mm (cord bush exit to connector exit)
25
61
65
276
5
60
40 32 113.3
Cable length 220mm (cord bush exit to connector exit)
16
13
45°
105
130
95
81.3
95
79.5
295
φ21 φ51
23
LV-EPIELD White LED Illuminator
LV-UEPI2A Motorized Universal Epi-Illuminator 2
266.7 207
510 370
25
6.3
58
25.5
68
45°
54
23
32
φ8.85 86
94
95
79.5
110
400Cable length 220mm
100
16
22.5
50
5 65
105
65.5
φ86
(cord bush exit to connector exit)
φ21
5
φ51
LV-TI3 Trinocular Tube ESD
φ51.2
LV-CR Column Riser 35
LV-TT2 Tilting Trinocular Tube
118
100 153
155
114
φ10 192.7
65.5
.3
264.6
59
φ60 φ50
137
66
31 φ52
138
.3
E.P.
φ51 60
75 98.5 104
20°
35
0
73.7
100
54.5 82 92.5 103 118
100
OUT
0
5
20° 96.8
E.P. IN
φ51
67
202.5
LV-S6 6x6 Stage
LV-S32 3x2 Stage
LV-S64 6x4 Stage
205
129
299
140.5 227 181
JAPAN
317
40
31
217
357 317
25.5
25.5
140.5 45.5
φ34
140.5
45.5
45.5
129
31
25.5
25.5
299
φ34
109
φ34
109
LV-SUB Stage
109
LV-SUB Stage 2
94
LV-S32PL ESD Plate
LV-S32SGH Slide Glass Holder
50 122
66 96
88
30
26.5
106 120
88
74 50
74 54
8-M4
4-M4
100 70
122
4.7
5
26.5
13
30.5
35
(39)
4
4
76.5
24
φ34
134
84
134
φ34
205.5
188
205.5
φ34
188
174
111
186
174
JAPAN
LV-NU5A Nosepiece
(89)
φ 70
48
48 88
69 15
62
34
22 1
45°
88
54
)
)
69 15
62
34
22 1
93.7
55.7
54
93.7
55.7
15° Cable length: 160mm from connection point
149
(182
(89)
15°Cable length 160mm
149
(182
φ 70
LV-NU5AC Nosepiece
45° φ43.5
φ43.5
7
7
φ12
φ12
LV-ARM Basic Arm
LV-NCNT Nosepiece Controller
Main arm 3 reference plane
25
Nosepiece port 0.5
308 260
Eyepiece tube port
48
3-φ7 Counter boring φ13 depth 9 (6 positions)
118
132 90
0.5
60 80 114
90
60°
φ72 50 +0.2 +0.1 25 45
110 10° 48
28
1-φ6H7 +0.012 0 Tooling hole
30
25
6 +0.012 0
R170
0.5
3
28
111
LV-EPI Epi Base
250 114
LV-DIA Dia Base 100
5
R12
245
245
φ62
φ60
φ62
95
5
95
R12
φ60
250 114
58
250
116 73.5
115 79
77 101
78 71
80 71
77 101
167
171.5 167.5
26
26
250
115 79
55
116 73.5
55 341
341
367
LV-ECON E Controller
14
109 95
165
210
C-HGFIE
LV-AF
UEPI2A
DIA TE2-PS100W
LV-FMA
EPI TE2-PS100W
LV-DICA
USB
100-240V∼ １．２Ａ ５０／６０Ｈｚ
NOSEPIECE
55.8
25
Polarizers/Analyzers/Plate YM-PO Polarizer
LV-PO Polarizer
85.4 79
LV-UVPO Polarizer
6.5
30
30
90
7.5
7.5
6.5
L-AN Analyzer
85.4 79
30
30
85.4 79
LV-P Plate
LV-FLAN FL Analyzer
47
10
λp
30
45° ±' late dire 30 ction
113.5
3
6.5
90
Objective Lenses CFI LU PLAN FLUOR CFI LU Plan Fluor EPI 5X
CFI LU Plan Fluor EPI 10X
CFI LU Plan Fluor EPI 20X
CFI LU Plan Fluor EPI 50X
CFI LU Plan Fluor EPI 100X
φ30 φ29
φ29 φ23.8
100X /
W.D.=1
90 A WD 1.0
3.5
30°
4.5
60
L.U
45°
φ8.5
φ9
47.5
59
80 A WD 1.0
40°
4.5 2.3
φ17.5
60
47.5
50X /
45°
W.D.=1
45 A WD 4.5
50°
JAPAN
L.U
60
20X /
59
L.U
55.5
60
W.D.=17.5
42.5
30 A WD 17.5
φ20
JAPAN
JAPAN
30° 10X /
60
15A WD 23.5
M25x0.75
M25x0.75
JAPAN
L.U
W.D.=23.5
5X /
45°
φ23.8
M25x0.75
5
JAPAN
L.U
36.5
φ23.8
M25x0.75
5
5
M25x0.75
φ30
φ23.8
W.D.=4.5
φ23.8
φ29
φ8.8
φ17.5 φ21.8
φ18 φ21.8
φ24
φ24
CFI LU PLAN FLUOR BD
M32x0.75
5 0.5
0.5
0.2
80 A WD 1.0
°
100X /
54
54
59
50X /
45 °
WD 4.5
90 A WD 1.0
° 35
3
3
35
φ26.2 φ33.5
φ25
L.U
L.U
45 A
60
51
55.5
20X /
JAPAN
JAPAN
L.U
W.D.=4.5
φ27.6 φ35.5
60
45
45 °
30 A WD 15
W.D.=15
JAPAN
10X /
3.95
6.7
WD 18
JAPAN
L.U
60
15A
W.D.=18
5X /
40.4 (Over head screw) φ40 φ35 M32x0.75 φ30.8
5
5 0.2
0.2 35
42
JAPAN
L.U
CFI LU Plan Fluor BD 100X
40.4 (Over head screw) φ40 φ35 φ30.8 M32x0.75
(φ28.4) φ37
(φ28.4) φ37
CFI L PLAN EPI CR CFI L PLAN EPI 100XCRA
CFI L PLAN EPI 100XCRB φ35.5 φ34 φ29.5 φ28.5 φ23.8
M25x0.75-6g (0.7)
M25x0.75
φ35.5 φ34 φ29.5 φ28.5
M25x0.75
(1 6° )
φ27 φ32.5
60.3
L
100X / 0.35 JAPAN
φ14.5 φ19.8 φ24.8 φ27 φ32.5
0.9(CG)
22
26°6.5 45 °
13
14.3 φ11.5 φ19.8 φ24.8
1.8 6.4
JAPAN
0.3(CG)
100X / 0.35
58.2
60.1
(1 6° )
25°6.5 45 °
13 14.3
58.7
22 6.2
L
W.D.=1.2
φ13 φ18.8 φ23.3 φ26 φ31.5
W.D.=1.1
JAPAN
25
60.2
50X / 0.70
30°
L
0.6(CG)
°
56.1
°) (7
45
3.1
φ20 φ31.5
W.D.=3.5
JAPAN
3 6.5 15.5
20X /0.45
(45
°）
L
60.2
°
0.6(CG)
11
13 14.5
5
5
(0.5)
φ33.5 φ32 φ29 φ27 φ23.8
5
(0.5)
φ35 φ33.5 φ29.5 φ27.5
5 5 11.7 10.8
49.1
21.1 W.D.=10.5
26
CFI L PLAN EPI 50XCR
(0.7)
CFI L PLAN EPI 20XCR
60
M32x0.75
CFI LU Plan Fluor BD 50X
W.D.=1
φ36 φ34 φ30.8
5
M32x0.75
CFI LU Plan Fluor BD 20X
59
φ36 φ34 φ30.8
60
CFI LU Plan Fluor BD 10X
φ36 φ34 φ30.8
W.D.=1
CFI LU Plan Fluor BD 5X
Main Specifications LV150/150A Main body Focusing mechanism
Baseless type (column riser 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 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 (1µm/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 LV-U EPI
12V-50W high-intensity halogen lamp; Field (centerable) and aperture diaphragms synchronized with B/D changeover; ø25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer insertable
Episcopic illuminator LV-U EPI2
12V-50W high-intensity halogen lamp; 120W high-intensity mercury-fiber illuminator (with brightness control, no centering necessary) mountable; Centerable field and aperture diaphragms synchronized with B/D changeover; ø25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer/ 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-TT Trinocular (inverted image, F.O.V. 22/25)
Stage
LV-S32 3x2 Stage (stroke: 75x50 mm including glass plate) LV-S64 6x4 Stage (stroke: 150x100 mm including 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 (main body)
LV150: approx. 8.6kg; LV150A: approx. 8.7kg
LV100D Main body Focusing mechanism
Baseless type (column riser insertable between arm and stand); Max. sample height 29mm (with LV-S32 3x2 Stage or LV-S64 6x4 Stage), 64mm with column riser; 12V-50W brightness control transformer built in 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 (1µm/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 LV-U EPI
12V-50W high-intensity halogen lamp; Field (centerable) and aperture diaphragms synchronized with B/D changeover; ø25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer insertable
Episcopic illuminator LV-U EPI2
12V-50W high-intensity halogen lamp; High-intensity mercury-fiber illuminator (with brightness control, no centering necessary); Centerable field and aperture diaphragms synchronized with B/D changeover; ø25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer/ 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
Condenser
LWD Achromat, Sliding Achromat 2-100x, C-C Abbe, C-C Achromat, Darkfield (dry)
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-TT Trinocular (inverted image, F.O.V. 22/25)
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 (main body)
Approx. 9.4kg
27
Main Specifications 100DA Main body
Baseless type (column riser insertable between arm and stand); Max. sample height 29mm (with LV-S32 3x2 Stage or LV-S64 6x4 Stage), 64mm with column riser; 12V-50W brightness control transformer built in
Focusing mechanism
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 (1µm/increments)
Interface
Motorized nosepiece: LV-NU5A Nosepiece, LV-NU5AC Nosepiece (with centering mechanism) Episcopic illuminator: LV-UEPI2A, High-intensity mercury fiber illuminator (PC-control only)
Nosepiece
LV-NU5A Nosepiece (high-durability motorized universal quintuple, with flare prevention mechanism) LV-NU5AC Nosepiece (high-durability motorized universal quintuple, with flare prevention and centering mechanisms)
Episcopic illuminator LV-UEPI2A
12V-50W high-intensity halogen lamp; High-intensity mercury-fiber illuminator (with brightness control, PC control); Motorized operation/control of illumination changeover turret; Motorized aperture diaphragm (centerable, automatically optimized for the selected objective)/field diaphragm (centerable) synchronized with B/D changeover; ø25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer/ plate insertable, excitation balancer insertable
Diascopic illuminator
12V-50W high-intensity halogen lamp; Centerable field and aperture diaphragms; Built-in filters (ND8, NCB11)
Condenser
LWD Achromat, Sliding Achromat 2-100x, C-C Abbe, C-C Achromat, Darkfield (dry)
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-TT Trinocular (inverted image, F.O.V. 22/25)
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/90W
Weight (main body)
Approx. 9.9kg
LV-IMA (motorized)/LV-IM (manual)/ LV-FMA (motorized)/LV-FM (manual) Main body
LV-IMA IM Module/LV-FMA FM Module A (motorized) Motorized nosepiece up/down section: stroke 20mm, resolving power 0.025µm, max. speed 2.5mm/sec. (resolving power 0.05µm) LV-IM IM Module/IV-FM FM Module (manual) Coarse/fine focus knob: stroke 30mm, coarse 5.2mm/rotation, fine 0.1mm/rotation (in 1µm 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 (high-durability motorized universal quintuple, with flare prevention), LV-NU5AC Nosepiece (high-durability motorized universal quintuple, with flare prevention and centering mechanism)
Episcopic illuminator LV-UEPI
12V-50W high-intensity halogen lamp; Field (centerable) and aperture diaphragms synchronized with B/D changeover; ø25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer insertable
Episcopic illuminator LV-UEPI2
12V-50W high-intensity halogen lamp; High-intensity mercury-fiber illuminator (with brightness control, manual control/PC control); Centerable field and aperture diaphragms synchronized with B/D changeover; ø25mm filter (NCB11, ND16, ND4) insertable; 2 epi-filter cubes insertable; Polarizer/analyzer/ plate insertable, excitation balancer insertable
Episcopic illuminator LV-U EPI2A
12V-50W high-intensity halogen lamp; High-intensity mercury-fiber illuminator (with brightness control, PC control); Motorized operation/control of illumination changeover turret; Motorized aperture diaphragm (centerable, automatically optimized for the selected objective)/field diaphragm (centerable) synchronized with B/D changeover; ø25mm filter (NCB11, ND16, ND4) insertable; 2 epi-filter cubes insertable; Polarizer/analyzer/ 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-TT Trinocular (inverted image, F.O.V 22/25), TV tube lens unit 0.5x, 1x
Eyepiece
CFI eyepiece series
Objective lens
CFI60 series
Electrostatic decay time
1000-10V, within 0.2 sec.
Weight (main body)
LV-IMA: approx. 3.7kg, LV-IM: approx. 3.5kg, LV-FMA: approx. 6.0kg, LV-FM: approx. 5.8kg,
LV-ECON Controller Interface
28
Motorized nosepiece: LV-NU5A, LV-NU5AC (with centering mechanism) Episcopic illuminator: LV-UEPI2A, LV-EPILED, high-intensity mercury fiber light source (PC-control type only) Motorized focusing module: LV-IMA, LV-FMA Halogen lamphouse (powered by TE2-PS 100W power source): LV-LH50PC PC (USB1.1) *Software Development Kit (SDK) is available.
System Diagram LV150/LV150A Camera Mount Photomicrographic System FX-III Series
Projection Lenses PLI 2x PLI 2.5x PLI 4x PLI 5x
Eyepieces
DXM1200F DS-5M DS-2M ENG-mount CCTV Camera
L-W 10x ESD
C-mount CCTV Camera C-mount Zooming Adapter
ENG-mount ENG-mount CCTV Adapter Zooming Adapter ENG-mount CCTV Adapters 0.45x 0.6x Relay Lens 1x
C-mount CCTV Adapters 0.35x 0.45x C-mount Direct 0.6x CCTV Adapter 0.7x
C-mount CCTV Adapter Relay Lens 1x
Zooming Lens
C-mount CCTV Adapter VM2.5x
V-T Photo Adapter
CFI 10x
Filar Micrometer 10xN
CFI CFI CFI 10xM 10xCM 12.5x
C-CT CFI Centering 15x Telescope
CFI UW CFI UW 10x M 10x
Adapter C-mount Adapter A 0.7x
F
C-mount CCTV Adapter VM4x
E
F.N.ø22
Filter Blocks and Sliders C-FL Fluorescence Filter Block
O
L-AN Analyzer
P
JAPAN
YM-PO Polarizer
D-FB Excitation Light Balancer
R
Q
D-FB
NCB Slider
JAPAN
LV-PAB Cube
C-mount Adapter 0.55x
LV-TV TV Tube
F.N.ø25
NCB11
Q'
P'
S
LV-PO Polarizer
LV-FLAN FL Analyzer
ND Slider ND16
ND4
T LV-P Plate
LV-UVPO Polarizer
Intermediate Modules Eyepiece Tubes LV-TT2 Tilting Trinocular Tube
E F
C-ER Eyelevel Riser
E F
0.5x 2nd Objective LV-TI3 Trinocular Tube ESD
Episcopic Illuminators Y-IDP Double Port (100:0 / 55:45) LV-UEPI Universal Epi-Illuminator
P
Other Eclipse series eyepiece tubes can be used.
Y-IDP Double Port (100:0 / 0:100)
I LV-UEPI2 Universal Epi-Illuminator 2
Q
S R
P'
I I’
O LV-CR Column Riser 35
B
Surugaseiki B23-60CR
Q'
T
A
LV-SUB Substage
S
LV-EPILED White LED Illuminator
LV-SUB Substage 2
LED Controller
Lamphouses LV-HL50W 12V-50W-LL Halogen Lamp LV-LH50PC Precentered Lamphouse
Stages L-S6WH Wafer Holder
L-S6PL ESD Plate
LV-S32SGH Slidegalss Holder
LV-S32PL ESD Plate
I I’
12V-100W Lamp D-LH 12V-100W Precentered Lamphouse (Requires TE2 External Power Supply) POWER
LV-S6 6x6 Stage
LV-S64 6x4 Stage
LV-S32 3x2 Stage
MIN.
B
I’ LV-HGFA Fiber Adapter
L2-DIC DIC Prism
MAX.
TE2-PS100W Power Supply (YM-EPI3 3-pin extension cord is required)
Nosepieces
Fiber
A
W W L-DIHC High Contrast DIC Prism
W LV-NU5AC U5AC Nosepiece (with LV150A)
Adapter
W LV-NU5A Motorized Nosepiece
L-NU5 U5 Nosepiece
L-NBD5 DB5 Nosepiece
C-N C-N6 Nosepiece
High-intensity Mercury Fiber Light Source X-CITE120 (with LV-150) X-CITE120PC (with LV-150A)
P-N P-N5 Nosepiece
LU Nosepiece Adapter M32-25 LU Plan Fluor BD Objective LV-NCNT Nosepiece Controller*
LV-NCNT Nosepiece Controller Cable 10m *Not necessary on the LV150A as the operation unit has been built into the main body.
LU Plan Fluor EPI Objective
C-OA 15MM Adapter
TI Objective Adapter
DI Objective
29
System Diagram LV100D
Camera Mount Photomicrographic System FX-III Series
Projection Lenses PLI 2x PLI 2.5x PLI 4x PLI 5x
Eyepieces
DXM1200F DS-5M DS-2M ENG-mount CCTV Camera
L-W 10x ESD
C-mount CCTV Camera
ENG-mount ENG-mount CCTV Adapter Zooming Adapter ENG-mount CCTV Adapters 0.45x 0.6x Relay Lens 1x
C-mount Zooming Adapter
C-mount CCTV Adapters 0.35x 0.45x C-mount Direct 0.6x CCTV Adapter 0.7x
C-mount CCTV Adapter Zooming Lens
Relay Lens 1x
C-mount CCTV Adapter VM2.5x
V-T Photo Adapter
CFI 10x
Filar Micrometer 10xN C-CT CFI Centering 15x Telescope
CFI CFI CFI 10xM 10xCM 12.5x
CFI UW CFI UW 10x M 10x
Adapter C-mount Adapter A 0.7x
F
C-mount CCTV Adapter VM4x
E
F.N.ø22
F.N.ø25
Filter Blocks and Sliders C-FL Fluorescence Filter Block
O
JAPAN
L-AN Analyzer
YM-PO Polarizer
P
D-FB Excitation Light Balancer
R
Q
D-FB
NCB Slider
JAPAN
LV-PAB Cube
C-mount Adapter 0.55x
LV-TV TV Tube
NCB11
Q'
P'
S
LV-PO Polarizer
LV-FLAN FL Analyzer
ND Slider ND16
ND4
T LV-P Plate
LV-UVPO Polarizer
Intermediate Modules Eyepiece Tubes LV-TT2 Tilting Trinocular Tube
E F
C-ER Eyelevel Riser
Episcopic Illuminators
E F
0.5x 2nd Objective LV-TI3 Trinocular Tube ESD
Y-IDP Double Port (100:0 / 55:45) LV-UEPI Universal Epi-Illuminator
P
Other Eclipse series eyepiece tubes can be used.
Y-IDP Double Port (100:0 / 0:100)
I Q
LV-UEPI2 Universal Epi-Illuminator 2
S R
P'
I I’
O LV-CR Column Riser 35 C-SP Simple Polarizing Polarizer
T
A B C
Q'
S
LV-EPILED White LED Illuminator
I
LED Controller
Condensers DF (dry)
Stages
LV-S32SGH Slidegalss Holder
D-C Abbe
LV-S32PL ESD Plate
C-C Achromat
LWD Achromat
Slide Achromat 2-100x
C
Lamphouses LV-S64 6x4 Stage
LV-HL50W 12V-50W-LL Halogen Lamp
LV-S32 3x2 Stage
LV-LH50PC Precentered Lamphouse
B I I’ L2-DIC DIC Prism
Nosepieces
A
12V-100W Lamp D-LH 12V-100W Precentered Lamphouse (Requires TE2 External Power Supply) POWER
MIN.
L-DIHC High Contrast DIC Prism
Adapter L-NU5 U5 Nosepiece
L-NBD5 DB5 Nosepiece
C-N C-N6 Nosepiece
I’ LV-HGFA Fiber Adapter
P-N P-N5 Nosepiece
MAX.
TE2-PS100W Power Supply (YM-EPI3 3-pin extension cord is required)
Fiber
External Light Source LU Nosepiece Adapter M32-25 LU Plan Fluor BD Objective
LU Plan Fluor EPI Objective
C-OA 15MM Adapter DI Objective
30
TI Objective Adapter
High-intensity Mercury Fiber Light Source X-CITE120
LV100DA/LV-FMA/LV-FM/LV-IMA/LV-IM Camera Mount
Projection Lenses PLI 2x PLI 2.5x PLI 4x PLI 5x
Eyepieces
DXM1200F DS-5M DS-2M
Photomicrographic System FX-III Series
ENG-mount CCTV Camera
L-W 10x ESD
C-mount CCTV Camera C-mount Zooming Adapter
ENG-mount ENG-mount CCTV Adapter Zooming Adapter ENG-mount CCTV Adapters 0.45x 0.6x Relay Lens 1x
C-mount CCTV Adapters 0.35x 0.45x C-mount Direct 0.6x CCTV Adapter 0.7x
C-mount CCTV Adapter Relay Lens 1x
Zooming Lens
C-mount CCTV Adapter VM2.5x
CFI CFI CFI 10xM 10xCM 12.5x
CFI UW CFI UW 10x M 10x
Adapter C-mount Adapter A 0.7x
F
E
F.N.ø22
F.N.ø25
Filter Blocks and Sliders
C-mount CCTV Adapter VM4x
V-T Photo Adapter
CFI 10x
Filar Micrometer 10xN C-CT CFI Centering 15x Telescope
C-FL Fluorescence Filter Block
O
L-AN Analyzer
P
JAPAN
YM-PO Polarizer
D-FB Excitation Light Balancer
R
Q
D-FB
NCB Slider
JAPAN
LV-TV TV Tube
NCB11
Q'
P'
LV-PAB Cube
C-mount Adapter 0.55x
S
LV-PO Polarizer
LV-FLAN FL Analyzer
ND Slider ND16
ND4
T LV-P Plate
LV-UVPO Polarizer
Intermediate Modules Eyepiece Tubes LV-TT2 Tilting Trinocular Tube
E F
C-ER Eyelevel Riser
E F
0.5x 2nd Objective LV-TI3 Trinocular Tube ESD
Episcopic Illuminators Y-IDP Double Port (100:0 / 55:45) LV-UEPI Universal Epi-Illuminator
P
Other Eclipse series eyepiece tubes can be used.
Y-IDP Double Port (100:0 / 0:100)
I LV-UEPI2 Universal Epi-Illuminator 2
K
Q
S R
P'
I I’
O
Condensers K D-C Abbe
DF (dry)
C-C Achromat
LWD Achromat
Slide Achromat 2-100x
Q'
T
LV-ARM Basic Arm
LV-UEPI2A Motorized Universal Epi-illuminator 2 P'
A
O
BF
FL1
DF
FL1
S R
I I’
FL2
FL2
C
Q'
T
S
LV-EPILED White LED Illuminator
C-SP Simple Polarizing Polarizer
K
K
LV-CR Column Riser 35
LV-FM FM Module
LV-FMA FM Module A
K
LED Controller
D
A
A
LV-IM IM Module
B
A B C
B C
LV-SUB Substage
D
Surugaseiki B23-60CR
I
D LV-SUB Substage 2
LV-IMA IM Module A
K
K
A
A
I LV-EPI Epi Base
LV-DIA Dia Base LV-HL50W 12V-50W-LL Halogen Lamp
Lamphouses LV-LH50PC Precentered Lamphouse L-S6WH Wafer Holder
Stages
L-S6PL ESD Plate
LV-S32SGH Slidegalss Holder
LV-S32PL ESD Plate
I I’ LV-S6 6x6 Stage
LV-S64 6x4 Stage
LV-S32 3x2 Stage
12V-100W Lamp D-LH 12V-100W Precentered Lamphouse (Requires TE2 External Power Supply) POWER
MIN.
I’
B
LV-HGFA Fiber Adapter
L2-DIC DIC Prism
Nosepieces
MAX.
TE2-PS100W Power Supply (YM-EPI3 3-pin extension cord is required)
Fiber
A
W L-DIHC High Contrast DIC Prism
W
W LV-NU5AC U5AC Nosepiece
Adapter
W LV-NU5A Motorized Nosepiece
L-NU5 U5 Nosepiece
L-NBD5 DB5 Nosepiece
C-N C-N6 Nosepiece
P-N P-N5 Nosepiece
High-intensity Mercury Fiber Light Source X-CITE120PC (with LV100DA)
LU Nosepiece Adapter M32-25 LU Plan Fluor BD Objective LV-NCNT Nosepiece Controller*
LU Plan Fluor EPI Objective
LV-NCNT Nosepiece Controller Cable 10m
C-OA 15MM Adapter DI Objective
TI Objective Adapter
E Controller (See page 28 for interface)
*Not necessary on the LV150A as the operation unit has been built into the main body.
31
Specifications and equipment are subject to change without any notice or obligation on the part of the manufacturer. December 2005. ©2005 NIKON CORPORATION WARNING
TO ENSURE CORRECT USAGE, READ THE CORRESPONDING MANUALS CAREFULLY BEFORE USING YOUR EQUIPMENT.
NIKON CORPORATION Fuji Bldg., 2-3, Marunouchi 3-chome, Chiyoda-ku, Tokyo 100-8331, Japan www.nikon.com/
NIKON INSTECH CO., LTD.
NIKON INSTRUMENTS EUROPE B.V.
NIKON INSTRUMENTS INC.
Parale Mitsui Bldg., 8, Higashida-cho, Kawasaki-ku, Kawasaki, Kanagawa 210-0005, Japan phone: +81-44-223-2175 fax: +81-44-223-2182 http://www.nikon-instruments.jp/eng/
P.O. Box 222, 1170 AE Badhoevedorp, The Netherlands phone: +31-20-44-96-222 fax: +31-20-44-96-298 http://www.nikon-instruments.com/
1300 Walt Whitman Road, Melville, N.Y. 11747-3064, U.S.A. phone: +1-631-547-8500; +1-800-52-NIKON (within the U.S.A.only) fax: +1-631-547-0306 http://www.nikonusa.com/
NIKON FRANCE S.A.S. FRANCE phone: +33-1-45-16-45-16 fax: +33-1-45-16-00-33 NIKON GMBH GERMANY phone: +49-211-9414-0 fax: +49-211-9414-322 NIKON INSTRUMENTS S.p.A. ITALY phone: + 39-55-3009601 fax: + 39-55-300993 NIKON AG SWITZERLAND phone: +41-43-277-2860 fax: +41-43-277-2861 NIKON UK LTD. UNITED KINGDOM phone: +44-20-8541-4440 fax: +44-20-8541-4584
NIKON CANADA INC. CANADA phone: +1-905-625-9910 fax: +1-905-625-0103
NIKON INSTRUMENTS (SHANGHAI) CO., LTD. CHINA phone: +86-21-5836-0050 fax: +86-21-5836-0030 (Beijing office) CHINA phone: +86-10-5869-2255 fax: +86-10-5869-2277 NIKON SINGAPORE PTE LTD SINGAPORE phone: +65-6559-3618 fax: +65-6559-3668 NIKON MALAYSIA SDN. BHD. MALAYSIA phone: +60-3-78763887 fax: +60-3-78763387 NIKON INSTRUMENTS KOREA CO., LTD. KOREA phone: +82-2-2186-8420 fax: +82-2-555-4415
Printed in Japan (0512-XX)T
En
Code No. 2CE-KVKH-2 This brochure is printed on recycled paper made from 40% used material.
