Industrial Microscopes LV Focusing Moduleszootos.com/home_data/standard/LV150.pdf · 2013. 4. 11. · the shape of a crossed Nicol prism, this cube is used for DIC observations. It

Industrial MicroscopesECLIPSE LV150/LV150A/LV100D/LV100DA

LV Focusing ModulesLV-IM/LV-IMA/LV-FM/LV-FMA

Industrial Microscopes

LV Focusing Modules

32

A versatile microscope system with a modular design

• 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 • Metallography

• Precision molds • LCD, color filters• Polarizing filters• Organic EL

• CCD • CMOS• LCOS • DMD

• LF/TAB • WL-CSP• QFP • SIP• BGA, CSP, FC

VersatilityVersatilityExtendYour

Vision

ExtendYour

Vision

OpticalPerformance

OpticalPerformance

ImprovedPerformance

ImprovedPerformance

• OA equipment parts• Cell phones, PDAs, DSC, PC parts

• Automobiles, aeronautics

MEMS

PCB

Casts and Parts

PrecisionMolds

FPD Display Devices

Semiconductors Materials IC Packages

LV-IMA

LV-ECON

Versatility 5

Extensive Range of Industrial Stages andAccessoriesUsers can select suitable models based on sample and stagestroke. All stages are highly durable with their triple-plate design.

Modular Design Major parts of the microscope main body—arm, stand, base,etc.—have been modularized for greater flexibility accordingto use. The LV-ARM Basic Arm, LV-FM FM Module, LV-FMAFM Module A, LV-EPI Epi Base, and LV-DIA Dia Base can befreely combined or incorporated into the system.

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, telecommuni-

cations devices, and a wide variety of other

samples.

Versatility

Accepts Thicker SamplesThe maximum sample height can be increased to 82mm from47mm by inserting the LV-CR Column Riser 35 between themain body and arm of the microscope. This feature is usefulfor viewing the surfaces of precision molds, optical materialsand other thick samples.

Non-Nikon Stages (LV150 or LV150Aonly) Use of non-Nikon stages, such as the Suruga Seiki B23-60CR,in combination with the LV-SUB Substage 2 allows themicroscope to handle thicker samples of up to 116.5 mm,thereby enabling the observation of fiber ends and othertools.

With column riserWithout column riser

Combination of LV-150 with LV-SUB Substage 2and Suruga Seiki B23-60CR stage

82mm47mm

Modular Design

An example configuration of the LV150

Appropriate holder and substage are selected based onsample and stage combination.

Compact Industrial Stage: LV-S32 3x2 StageThe newly designed LV-S32 3x2 is a compact stage forindustrial microscopes. Its triple-plate design ensures

durability, stability and ease ofuse, even when heavy samplessuch as metallic materials areobserved. The standard glassplate makes this stage suitablefor episcopic and diascopicillumination.

An example of the LV-DIA Dia Base incorporated into a tape-transport sampleinspection system.

LV-S6 6x6 Stage Stroke: 150 x 150 mm

LV-S64 6x4 StageStroke: 150 x 100 mm

L-S6WH Wafer Holder(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-suctionsection

Roll-out section Roll-in section

Tape-transportsection

Stage section

If the LV-DIA Dia Base is used, a diascopic illuminator can beincorporated into the system*. * An optional power source, the TE2-PS100W, and related options are needed to

perform diascopic illumination.

LV-FM FM Module (manual)LV-FMA FM Module A (motorized)

LV-EPI Epi Base LV-DIA Dia Base

LV-ARM Basic Arm

4

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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 12V-

100W 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.

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 —

Optimal Illumination Function

Universal Epi-Illuminator: LV-UEPIThe LV-UEPI universal epi-illuminator enables brightfield,darkfield, simple polarizing and DIC observations. Field andaperture diaphragms are automatically opened when theobservation is switched from brightfield to darkfield, andreturn to their original position when switched back tobrightfield.

Why is 50W brighter than 100W?Image brightness is not determined by wattage. Nikon’s new light source delivers greater brightness by optimizing thelamp filament size and improving pupil illumination fulfillment by optically expanding the size of the light source. Thishas resulted in a 50W light source that is brighter than a 100W lamp. With 50x or higher objectives, brightness is about20% greater under episcopic illumination, 40-50% greater with diascopic illumination, than previous Nikonilluminators.

Motorized Universal Epi-Illuminator 2:LV-UEPI2AIn this illuminator, the illumination changeover turret and theaperture diaphragm, as well as the illumination voltagecontrol, have been motorized, for accurate reproduction ofillumination—therefore, images can be taken underconsistent illumination. Aperture is automatically optimizedaccording to the objective and illumination technique in use.It can, however, also be changed manually depending on thesample and purpose. When configured with the LV100DA microscope, thisilluminator can be controlled on the microscope or from theconnected PC. Control from the PC is possible when theilluminator is incorporated into the system using the LV-ECON E controller.

Universal Epi-Illuminator 2: LV-UEPI2The LV-UEPI2 universal episcopic illuminator is equipped with advanced optics suitable for a wide variety ofobservation methods—brightfield, darkfield, DIC and epi-fluorescence. It allows the operator to concentrate on theobservation by automatically maintaining optimalillumination conditions for the aperture diaphragm, shutter,filters, including diffuser and ND filter.

LV-PAB PA CubeWith a polarizer and analyzer attached inthe shape of a crossed Nicol prism, thiscube is used for DIC observations. It isused by installing it into the turret of theLV-UEPI2 or LV-UEPI2A epi-illuminator;to begin observations simply insert aDIC slider into the optical path.

• Brightfield• Darkfield• Simple polarizing• DIC• 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

• Brightfield• Darkfield• Simple polarizing• Observation with first-order red compensator• DIC• Epi-fluorescence (UV excitation possible)• UV polarizing epi-fluorescence• Double-beam interferometry

Extend your vision

High-Intensity 12V-50W Halogen LightSource:LV-LH50PC Precentered LamphouseAlthough the LV-LH50PC Precentered Lamphouse is 12V-50W, the brightness is equivalent to or higher than that of12V-100W. The low power-consumption halogen lightsource contributes to the compact design of themicroscope while also being friendly to the environment.Defocus induced by heat is substantially reduced.

LV-EPILED White LED IlluminatorWith emphasis on light weight and compact design,this white LED illuminator was specially developed forbrightfield use. It is operated via the attached powersource controller. By using the LV-ECON E controller,external control is also possible.

HG Precentered Fiber Illuminator—Intensilight (for LV-UEPI2/LV-UEPI2A)The use of the Intensilight precentered fiber illuminatoreliminates the need for centering and focus adjustment,even after the lamp is replaced. Because the light sourcecan be placed away from the microscope, heat andelectrical noise on the microscope body is reduced. Sixlevels of light intensity from 3% to 100% are available, andthe shutter is incorporated. The lamp lasts an average of2000 hours, reducing replacement time and costs. Both manual (C-HGFI) and motorized (C-HGFIE) modelsare available. The motorized model should be used incombination with the LV150A/LV100DA. The motorizedmodel can be controlled from an optional dedicatedremote controller or a PC that incorporates Nikon’s NIS-Elements imaging software.

C-HGFI (manual)

98Opt

ical

Per

form

ance

Optical Performance

CFI60 LU Plan Fluor EPI series

CFI60 LU Plan Fluor BD series

CFI60 L Plan EPI CR series of objective lenseswith correction ring

With correction at 0.7 mm (50x)

LV-NU5ANosepiece

LV-NU5ACNosepiece

Without correction (50x)

Improved Transmission Rate for UVWavelength CFI LU Plan Fluor seriesThe transmission rate in the UV wavelength range has beenimproved for the new CFI LU Plan Fluor series. These objectivelenses are suitable for various research, analysis andexamination needs, while maintaining Nikon’s commitment tohigh NA and long working distance. Only one kind of objectivelens is needed for brightfield, darkfield, simple polarizing,observation with first-order red compensator, DIC and UV epi-fluorescence observations. These objective lenses, which offerhigh resolution and easy-to-use performance, can be combinednot only with microscopes but also with other equipment foreven greater versatility.

Objective Lenses with Correction RingCFI L Plan EPI CR seriesThe CFI60 series now includes the CFI L Plan EPI CR series tocope with the thinner coverglass used in liquid crystal displays,and highly integrated, and dense devices. Coverglass correctioncan be continuously made from 0 mm up to 1.2 mm (0-0.7 mmand 0.6-1.3 mm for 100x) with the correction ring. The 100xobjective lens offers 0.85 high NA, while enabling high-contrastimaging of cells and patterns without being affected by thecoverglass.

Environment FriendlyThe eco glass used in the CFI LU Plan Fluor and L Plan EPI CRseries does not contain harmful substances such as lead andarsenic.

Model Magnification NA Working Distance (mm)CFI L Plan EPI 2.5X 0.075 8.8CFI LU Plan Fluor EPI 5X 0.15 23.5

10X 0.30 17.520X 0.45 4.550X 0.80 1.0100X 0.90 1.0

CFI LU Plan EPI ELWD 20X 0.40 13.050X 0.55 10.1100X 0.80 3.5

CFI L Plan EPI SLWD 20X 0.35 24.050X 0.45 17.0100X 0.70 6.5

CFI LU Plan Apo EPI 100X 0.95 0.4150X 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

10X 0.30 15.020X 0.45 4.550X 0.80 1.0100X 0.90 1.0

CFI LU Plan BD ELWD 20X 0.40 13.050X 0.55 9.8100X 0.80 3.5

CFI LU Plan Apo BD 100X 0.90 0.51150X 0.90 0.4

Model Magnification NA Working Distance Glass Thickness (mm) (mm) Correction Range

CFI L Plan EPI CR 20x 0.45 10.9-10.0 0-1.2mmCFI L Plan EPI CR 50x 0.7 3.9-3.0 0-1.2mmCFI L Plan EPI CRA 100x 0.85 1.2-0.85 0-0.7mmCFI L Plan EPI CRB 100x 0.85 1.3-0.95 0.6-1.3mm

CFI60 Series ObjectivesBrightfield

With correction mechanism

Bright/darkfield

Product Name NA W.D. (mm)

LWD Achromat condenser 0.65 10.2C-C Slide Achromat condenser 2-100X 0.9 1.2-2.2C-C Abbe condenser 0.9 1.9C-C Achromat condenser 0.85 4.2Darkfield (dry) condenser 0.8-0.95 4

Condensers

Impr

oved

Per

form

ance

Overall performance has been improved with better durability and rigidity.

Improved Performance

Highly Rigid, Vibration-Free Body The use of structural analysis during the design processhas improved rigidity and anti-vibration parameters toyield clear images even at high magnification.

Tilting Trinocular Eyepiece Tube

LV-TT2 Tilting Trinocular EyepieceTubeThe newly developed LV-TT2 tilting trinoculareyepiece tube (erect image) offers comfort to allusers, regardless of their stature or viewingpositions. The optical path changeover of100:0/20:80 allows simultaneous use of monitor.

*C-mount adapter 0.55x can be directly mounted to LV-TT2and LV-TI3 for the DS-2M series.

Highly Durable Motorized UniversalNosepieces

LV-NU5A and LV-NU5AC Nosepieces Two types of motorized universal quintuplenosepieces are available. The LV-NU5A boastsgreater durability thanks to a new click mechanismand control system. The LV-NU5AC comes with acentering mechanism that suppresses image driftduring objective changeover. These nosepieces cannot only be configured with the LV150A or LV100Amicroscope, but also incorporated into otherdevices in combination with the LV-NCNTnosepiece controller and LV-ECON controller.

Manual Nosepiece A variety of manual control nosepieces areavailable to suit all needs.

Thorough ESD Protection

All parts of the microscope that might be touched,including the body, tube and stage, have beeninsulated. This improves anti-contamination andprevents samples from being harmed byelectrostatic, 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)

1110

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, LV-NU5A Motorized Universal Nosepiece, LV-NU5AC Motorized Universal Nosepiece with centering mechanism, and LV-ECON EController—to give you greater flexibility in configuring a system best suited to your purpose.

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-IMA IM Module A (motorized)/LV-IM IM Module (manual)

LV100DA, Focusing Module

An example configuration of the LV-IMA

LV-IMA IM Module A

LV-IM IM 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 externallycontrolled 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 anosepiece up/down mechanism that has an ultra-long vertical stroke of 68mm—it facilitates operations such as semiconductorprobe inspections.

LV-FMA FM Module A (motorized)/LV-FM FM Module (manual)

An example configuration of the LV-FMA

Nosepiece moves up and down. LV-FMA FM Module A

LV-FM FM Module

Among performance requirements demanded of amicroscope, those associated with digital imaging—digital image capture, analysis, and databaseformation—are growing faster than ever before. TheLV100DA motorized system squarely addresses thesedemands and now comes equipped with a mechanismthat automatically optimizes observation technique andillumination—and these settings can be quantitativelycontrolled from external devices.

Auto Optimization of IlluminationIn configuration with the LV-UEPI2A motorizeduniversal illuminator, the system automatically setsoptimum illumination conditions for the objective andobservation technique in use, for quick recall ofobservation conditions.

Motorized universal illuminator

USB1.1

High-intensity mercury fiberilluminator

TE2-PS 100W power supply (simultaneous epi/dia illumination)

Motorized universal illuminator

Synchronized control window (setup software)

Objective lens window (setup software)

LV100DA Interface

An example configuration of the LV100DA

A motorized system that optimizes image capturing conditions— Focusing Modules and Controller Amply Support Motorized Control

12 13

LV-ECON E Controller This controller provides interface to externally control the light source, motorized illuminator, nosepiece, focusing moduleand other motorized units from the connected PC and other devices. Communication between this and the PC is establishedvia 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

An example configuration of the LV150A

(Episcopic Illumination Type)

L150A controls

CFI-Series Eyepiece

An illuminator that can beused for brightfield,darkfield, simplepolarizing and DICobservations.

LV-UEPI

A universal motorizednosepiece that is 10 timesmore durable than itspredecessors.

LV-NU5A Nosepiece

These objective lenses featurehigh NA, long working distancesand improved transmission ratein the UV range.

CFI LU Plan Fluor Series

The LV150 and LV150Amicroscopes are used forepiscopic illumination.

A trinocular tube with anoptical path changeoverof 100:0/0:100.

LV150/LV150A

An episcopic illuminationstage capable of inspecting150mm wafers. (With 6”wafer holder)

LV-S6 6x6 Stage

LV-TI3 Trinocular TubeA low power-consumption 12V-50Whalogen light source equivalent to orhigher than the 12V-100W type.

LV-LH50PC Precentered Lamphouse

Motorized nosepiece controls

LV-ECON Controller

LV-UEPI2A Motorized Universal Illuminator

LV-IMA IM Module A

LV-FMA FM Module A

LV-NU5ANosepiece

LV-NU5ACNosepiece

LV-EPILED White LED Illuminator

(Episcopic/Diascopic Illumination Type) (Episcopic/Diascopic Illumination Type)

CFI-Series Eyepiece

This illuminator controlsthe illuminationchangeover turret andaperture diaphragm via amotor. The diaphragm isautomatically optimizedaccording to the objectivein use.

LV-UEPI2A

The LV-NU5AC motorizednosepiece comes with acentering mechanism thatminimizes image driftduring objectivechangeover.

Nosepiece

These objective lensesfeature high NA, longworking distances andimproved transmission ratein the UV range.


Compatible with bothepiscopic and diascopicillumination and supportsthe LV-UEPI2A motorizeduniversal epi-illuminatorand motorized nosepiece.

The LV-TT2 is a tilting trinoculartube that has an optical pathchangeover of 100:0/20:80.

LV100DA

Compatible with bothepiscopic and diascopicillumination, this stageaccommodates samples upto 150 x 100mm.

LV-S64 6�4 Stage

LV-TT2 Tilting Trinocular Tube

A low power-consumption 12V-50Whalogen light source equivalent to orhigher than the 12V-100W type.

LV-LH50PC 12V-50W Lamphouse

LV100DA controls

Enable motorized control of motorized nosepiece,illumination changeover turrets, aperture diaphragm,light source (epi/dia), etc.

An example configuration of the LV100DA

14 15

CFI-Series Eyepiece

The LV-UEPI2 illuminatorenables brightfield,darkfield, DIC, simplepolarizing, and UVexcitation epi-fluorescenceobservations.

LV-UEPI2

Selectable from C-N6(brightfield), L-NBD5(bright/darkfield) and L-NU5 (universal) nosepieces.

Nosepiece

These objective lenses featurehigh NA, long working distancesand improved transmission ratein the UV range.


The LV-TT2 is a tilting trinocular tubethat has an optical path changeover of100:0/20:80.

This small, industrial-usestage has a triple-platedesign and can be used forepiscopic and diascopicillumination.

LV-S32 3x2 Stage


A low power-consumption 12V-50Whalogen light source equivalent to orhigher than the 12V-100W type.

LV-LH50PC 12V-50W Lamphouse

The LV100D microscope iscapable of episcopic anddiascopic illumination.

LV100D

An example configuration of the LV100D

LV-�P� Plate

BrightfieldThe antiflare design appliedto the objective lenses andlight source ensures bright,and high-contrast images.

DarkfieldNikon’s unique “Fly-eyeLens” used in the darkfieldilluminator yields athreefold increase inbrightness over previousmodels. This allows high-sensitivity detection ofdefects and height gaps insamples.

Nomarski DIC

Standard or high contrast DICsliders can be selected to suit

the sample. Thismethod is usefulfor the surfaceobservations ofvarious devicesand precisionmolds.

Epi-FluorescenceUV, V, BV, B or G excitationfluorescence filter blocks canbe selected. This method isperfect for the observation ofOLED, ion migration andother substrate uses.

L-DIC DIC Prism (standard) L-DIHC DIC Prism (high contrast) Brightfield Epi-fluorescence B-2A

Fluorescence filter blocks

Simple PolarizingIn addition to simplepolarizing, a lambda platecan be inserted into theoptical path to achieve first-order red compensatorobservation. This is usefulfor liquid crystalinspections (when used incombination with the LV-UEPI 2).

Double-Beam Interferometry Equipment(measures nano scale height gaps)

Michelson (TI) and Mirau (DI)types of episcopic double-beam interferometry can becarried out. A filar micrometereyepiece can be used toexamine or measure sampleswhile avoiding direct contact.

Diascopic IlluminationDiascopic illumination isused to observe opticalparts, FPD and other samplesthat transmit light.

Episcopic double-beam InterferometryEquipment TI/DI

Condensers

Observation Methods

YM-POPolarizer

LV-UVPOPolarizer

LV-FLAN FLAnalyzer

L-ANAnalyzer

LV-PO Polarizer

LV-FLAN FL Analyzer

L2-DIC DIC Prism

L-DIHCHigh-contrastDIC Prism

YM-POPolarizer

L-ANAnalyzer

16 17

Applications

LV-PAB PACube

PCB

LCD (conductive particle) Test reticle Spodumene Carbon Paper

Nodular Graphite Cast Iron Tourmaline

Epi-fluorescence

DIC Diascopic brightfield DIC Brightfield

DIC Brightfield

Semiconductor (wafer) Semiconductor (wafer) MEMS (optical switch)

Brightfield Darkfield Brightfield Brightfield

Simple polarizing Brightfield Brightfield Epi-fluorescence

Brightfield

Micro Bump

Compact Disc (CD) Image Sensors (CCD) PCB (ion migration) PCB (ion migration)

PCB LCD (color filter)

Diascopic brightfieldDIC

Precision Mold

Tourmaline Tourmaline

DIC Double-beam interferometry

18

100100

ININ

0

0 0

100100

OUTOUT

Eyepiece Tubes

Nosepieces

Objective Adapters

Objective Lenses

Diascopic Illumination Condensers

LV-TI3 Trinocular Eyepiece Tube LV-TT2 Tilting Trinocular Eyepiece Tube

C-N6 Nosepiece(Brightfield)

L-NBD5 Nosepiece(Bright/darkfield)

L-NU5 Nosepiece(Universal)

C-OA 15mm AdapterLU Objective Adapter M32-25

LV-NU5AMotorizedNosepiece(Universal)

LV-NU5AC MotorizedNosepiece (Universal; withcentering mechanism)

Modular DesignLWDAchromat

C-C Abbe Darkfield(Dry)

SlideAchromat2-100x

C-C Achro

CFI LU PLAN FLUOR EPI series

CFI LU PLAN FLUOR BD series

CFI L PLAN EPI CR series

Double Port

White LED Illuminator Polarizing/DIC accessories

Substages (for LV150/LV150A)

Substages (LV150/LV150A)

Arm

Holders

Y-IDP Double Port(Ratio 100:0/55:45)Y-IDP Double Port 0/100(Ratio 100:0/0:100)

LV-SUB Stage LV-SUB Stage 2

LV-S6 6x6 Stage LV-S64 6x4 Stage LV-S32 3x2 Stage

L-S6WH WaferHolder

LV-ARM Basic Arm

Focusing Modules

LV-FMA FM Module(motorized)

LV-FM FM Module(manual)

Bases

LV-EPI Epi Base

For LV-S6 6x6 Stage For LV-S32 3x2 Stage

L-S6PL ESDPlate

LV-S32SGH SlideglassHolder

LV-S32PL ESDPlate

Simple Polarizing UV Polarizing with Epi-Fluorescence

YM-POPolarizer

LV-UV PO UV Polarizer L2-DICDIC Prism

L-DIHC DICPrism HC

L-ANAnalyzer

YM-POPolarizer

L-ANAnalyzer

LV-POPolarizer

LV-FLAN FLAnalyzer

LV-�P � Plate

Observation with First-Order RedCompensator

DIC

LV-UEPI

LV-UEPI2

LV-UEPI2A

LV-EPILED

Illuminators

LV-PAB PA Cube

19

Model F.O.V. Remarks

CFI 10x 22

CFI 10xM 22 Photomask included

CFI 10xCM: 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 mmMain scale: 0.1 mm/incrementsSub scale: 0.01 mm/increments

Eyepieces

LV-DIA Dia Base

21

Digital Cameras for Microscopes

A camera head and a control unit can be flexibly configured according to the workpiece and

observation purpose.

Operations from capture and display of live images, image processing

and analysis are all operated from a PC. The DS-U2 can be used

flexibly for a wide range of applications.

Simple, high-speed USB 2.0 connectionPC connection via USB 2.0 interface allows comfortable operation.

With a built-in high-definition largeLCD monitor and versatilefunctions, the DS-L2 eliminates thenecessity of PC connection andallows easy operation.

With a high-definition 5.0-megapixelcolor CCD, wide dynamic range andexcellent red sensitivity, the DS-Fi1 issuitable for imaging of brightfield,darkfield and Nomarski DIC observation.

Camera Heads

PC-use Control Unit

Standalone Control Unit

Large monitor displays high-quality imagesA high-definition 1024 x 768 pixel, 8.4-in. color TFT LCD monitor isincorporated.

On-screen menu allows easy controlWith an OSD system, camera control, state confirmation and settingscan be manipulated by keyboard operation or simple mouse click onicons or the onscreen menu.

Storage and print functions for a wide range of applicationsSaving the data on an USB memory stick, CompactFlash card,Microdrive and transferring them to other networked PCs is possible.Direct print with a PictBridge printer is possible as standard. “Real 10”modes that allow setting and adjustment of printing magnification areincorporated.

Easy-to-use shortcut menuFrequently used functions can be displayed as buttons. They can beoperated without impeding the display of captured images. It is alsopossible to customize the buttons.

Two-pane display suitablefor comparative observationThe capability to simultaneouslydisplay stored and live images isconvenient for comparativeobservation.

Shortcut menu example (left: Short/right: Large)

Stored image Live image

Imaging mode provides optimal photography with easeOptimal imaging parameters are preset for three different sampletypes. Also, up to seven custom modes can be set.

Various measuring tools• Measurement/positioning functionWith calibration of reference length (up to seven can be registered),measuring and positioning can be conducted.

• Drawing functionsInput and display of lines and comments arepossible.. Free straight line (arrowed line setting possible). Free curved line. Count mark. Text input. Super imposition (translucent imagefor comparison)

Scale display/positioning functions

Wafer IC-chip

With a high frame rate, 2.0-megapixelcolor CCD, the DS-2Mv enables thesmooth display of live images andprovides high quality images.

For more information, see the Digital Sight series catalog.

Digital Cameras for Microscopes

Large monitor (external output)

Projector (external output)

Network server (web, FTP, TelNet)

PC (mass storage class)

PictBridge printer (direct print)

Dedicated camera cable (3m)

Universal type ACpower adapter

USB keyboard

Microscope (control license necessary)

USB mouse

USB memory stick

DS series camera headCamera control unit

CompactFlash card/Microdrive

Dedicated remote controller,flash lamp, etc.

DVI-ILAN (Ethernet)USB (D)USB (H)USB (H)

Standard set Option Microscope PC (Windows® XP)

USB (D)

Dedicated camera cable (3m)

Universal type AC power adapter

DS series camera headCamera control unit

Circle(perimeter/diameter) AreaPerpendicularDistance Distance betweencircle centers

Grid

Angle

XY scale XY measurement

Pitch

ScaleScreen pattern

(crossline/concentric circle)

Metal Ceramic Circuit Board

Measurement functions

Newly developed imaging software NIS-ElementsThe NIS-Elements is employed as control software. It conducts from basic image

capture to measurement, analysis and management of captured images. It is also

possible to add plug-ins to meet specific needs and applications.

Free bundle

NIS-Elements F packageDisplay of the scale on a live image and full-screen image display are possible. Imagesare captured easi ly using the simpleoperation screen.

Standard

NIS-Elements DocumentationThis package provides measurement andreport generation functions. It can beuniversally used for microscopy imageacquisition in the industrial field. Expandedfunctionality is possible through the additionof optional plug-ins, such as EDF anddatabase plug-ins.

Option

NIS-Elements Basic ResearchIn addition to the measurement and reportgeneration functions of NIS-Elements D,automatic measurement, including objectextraction of binary images, is possible.Expanded functionality is possible throughthe addition of optional plug-ins, such asEDF and database plug-ins.

Operating environmentThe following PC environment is recommendedto achieve optimal performance of NIS-Elements.

Operation screen Screen layout can be flexibly selecteddepending on requirements.

MeasurementMeasurement of the object number, length,radius, angle, area and brightness profile ispossible.

Report generatorReports can be easily created using capturedimages and links to measured data. PDF filescan be created directly from NIS-Elements. Itis also possible to create PDF files directlyfrom NIS-Elements.

Extended Depth of Focus

With this plug-in, images that have beencaptured in a different Z-axis can be used tocreate an all-in-focus image and virtual 3Dimage.

CPU Intel® Pentium® IV processor, 3.2GHz ormore

RAM 1GB or more

OS Microsoft® Windows® XP SP2(Japanese/English version)

HDD 600MB or more required for installation

Display 1280 x 1024 or higher (TrueColor mode)

F

D

Br

D Br

D

Full screen Organizer screen

Br

DOption Br

D Br

For the PC-use control unit, the DXM1200C digital camera with a super high 12.6 megapixel output is also available. For more information, see the DXM1200C catalog.

Docked control screen

High-definition ColorCamera Head High-speed Color Camera Head

2322

Dimensional Diagrams

LV-UEPI Universal Epi-Illuminator LV-UEPI2 Universal Epi-Illuminator 2

100

IN

0

0

100

OUT

96

26790

508.5

387.2

326

193

78341

457

134.5

36

250

JAPAN

341

484

495

391

326

193

92

15176

250

140.5

25.5

96

Cable length 220mm (cord bush exit to connector exit)

336

295

27660

13

130

61

25

105

95

LV150A/LV150

LV100D

LV100DA

115 190

495

391

326

193

92

484250341

140.5

96

Screw depth: less than 9mm from �A surface

Vertical stroke: up 19, down 1

Eyepiece tube port

Nosepiece port

49(48～68)

138.8

25

120±0.1

9

65.5

2

8742

60

80±0.1

8depth 3.4

4280±0.1

55

95

471702-M4 深8

80±0.1

4-M6 depth 10

11495±0.1

2-φ9 depth 3.4

62±0.118

4-M6

+0.015

0

(2-R4) φ8H7

depth 3.4

+0.0150

□

10

A

LV-IMA IM Module A (motorized)

Vertical stroke: up 29, down 1

Nosepiece port

Eyepiece tube port

120±0.1

9

2-φ9 depth 3.4

8depth 3.4

80±0.1

62±0.118

(2-R4)

4-M6

120.710411495±0.1

4-M6 depth 10

95

55

138.8

65.5

2

49(48～78)25

87

4260 80±0.1

42

170 47

80±0.12-M4 depth 8

+0.015

0

φ8H7

depth 3.4

+0.0150

0

10

20

30

40

50

60

70

80

90

10

□A

Screw depth: less than 9mm from �A surface

LV-IM IM Module (manual)

Nosepiece portVertical stroke: up 19 down 1

2-φ9 depth 3.4

depth 3.4

+0.015

0

φ8H7

Fixed plate thickness

φ8

8depth 3.4

+0.015

0

+0.001 0.041

Screw depth: less than

9mm from �A surface

30848

Eyepiece tube port

25 28

4-M4 depth 8

114

31163.5

113

2618

225(224～244)

55

95260

114

126.5±0.180±0.1

80±0.1

□A

4-M6

62±0.1 18

(2-R4)

10

80±0.1

LV-FMA FM Module A(motorized)

Eyepiece tube port

Vertical stroke: up 18.5 down 1

Nosepiece port

2-φ9 depth 3.4

depth 3.4

+0.015

0

φ8H7

Fixed plate thickness

8 depth 3.4

+0.015

0

Screw depth: less than

9mm from �A surface

30848

25

225(224～254)

163.5

3128

113

1826

26095

55

□Aφ8-0.001-0.041

4-M4 depth 8

114

80±0.1

126.5±0.180±0.1

4-M662±0.1 18

10

80±0.1

(2-R4)

104120.7

114

LV-FM FM Module(manual)

Unit: mm

Cable length 220mm (cord bush exit to connector exit)

510370 25.5

110

79.5

81.3

655 105

16

φ40 40113.3

32400

φ51

φ21

95

45°

2524

LV-NU5A NosepieceLV-NU5AC Nosepiece

(182)

Cable length: 160mm from connection point

6915

φ127φ43.5

15°

14993.755.7(

89)

48

88

φ70

62

45°

34

54

221

LV-NCNT Nosepiece Controller

110

28

111

10°48

(182)

Cable length160mm

6915

φ127φ43.5

15°

14993.755.7(

89)

48

88

φ70

62

45°

34

54

221

LV-EPI Epi Base

167

φ60

φ62

95245

78 71 77 101

26

79 55341

250

58250114

R125

73.5115116

LV-ECON E Controller

USB

UEPI2A LV-FMA LV-DICA

C-HGFIE LV-AF TE2-PS100W

NOSEPIECE

TE2-PS100WDIA EPI

100-240V～　1.0Ａ　50／60Hz

165

210

95109

14

55.8

LV-ARM Basic Arm

90

1-φ6H7 +0.0120

6+0.012

0

50+0.2

+0.1

Tooling hole 25

28

3

1148060

0.5

3-φ7Counter boring φ13 depth 9(6 positions)

9011813248

260308

Eyepiece tube port

0.50.5

25Main arm reference planeNosepiece port

3

30

60°

R170

4525

φ72

LV-UEPI2A Motorized Universal Epi-Illuminator 2 LV-EPIELD White LED Illuminator266.7

207 25 6.358

φ8.8586

65.5

9450

5

22.5

φ86

φ51.2

LV-DIA Dia Base

122 122

76.5

88 88

26.5

5 4.7

155

114

35

245

341

100

250

φ62

φ60

171.5

167.5

80 71 77 101

26

79 55

367

115 73.5116

95R125

250114

JAPAN

JAPAN

205

317

317

109

φ34

357

40 31 217 25.5

129 299

205.5

205.5

140.5

188

188

φ34

45.5

25.5

299

φ34 φ34109 109

140.5227

181

186

174

31 25.5

174

111

129

45.5

φ34

8445.5

25.5

134

134

φ34

140.5

100

IN

0

0

100

OUT

118

100

153

192.7 65.5

20°

20°

96.8

φ10

E.P.

137.3 138.3

φ60φ50

φ51 φ51

60 67 202.5

118

73.7103

92.582

54.5

5

59

E.P.

264.6 66 31

φ52104

98.5

75

35 26.544

70 74 507430.5 13

8-M4

4-M4

( 39)

100

50

3054106

94

1206696

LV-TI3 TrinocularTube ESD

LV-TT2 TiltingTrinocular Tube

LV-CR Column Riser 35

LV-S6 6x6 Stage LV-S64 6x4 Stage

LV-SUB Stage LV-SUB Stage 2 LV-S32PLESD Plate

LV-S32SGH SlideGlass Holder

LV-S32 3x2 Stage

510370 25.5

110

79.5

68

5423

10032

400Cable length 220mm (cord bush exit to connector exit)

105

95

φ21

φ51

16655

45°

26 27

LV150/150A

Main Specifications

Main body Baseless type (column riser insertable between arm and stand); Max. sample height 47mm (when configured with 3x2 stage/6x4stage), 82mm with column riser, 116.5mm with Suruga Seiki B23-60CR; 12V-50W brightness control transformer built in

Focusing mechanism Coaxial coarse/fine focus knob, left: coarse/fine, right: fine; Stroke 40mm, coarse 14.0mm/rotation (torque adjustable, withrefocusing 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, withflare prevention)

Episcopic illuminator 12V-50W high-intensity halogen lamp; Field (centerable) and aperture diaphragms synchronized with B/D changeover; LV-U EPI ø25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer insertable

Episcopic illuminator 12V-50W high-intensity halogen lamp; 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; 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 (invertedimage, 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

LV100DMain 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


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; Field (centerable) and aperture diaphragms synchronized with B/D changeover; LV-U EPI ø25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer insertable

Episcopic illuminator 12V-50W high-intensity halogen lamp; High-intensity mercury-fiber illuminator (with brightness control, no centering necessary);LV-U EPI2 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)


Stage LV-S32 3x2 Stage (stroke: 75x50 mm including glass plate)LV-S64 6x4 Stage (stroke: 150x100 mm including glass plate)





Weight (main body) Approx. 9.4kg

Polarizers/Analyzers/�Plate

YM-PO Polarizer LV-PO Polarizer

LV-FLAN FL Analyzer LV-�P �Plate

LV-UVPO Polarizer L-AN Analyzer

47113.5

79

903030

30

36.5

7.5

307.5

10

45°±'

λ plate direction

6.5

6.5

90

30

85.479

85.4 85.479

30

φ29

φ20 φ17.5 φ9

φ23.8

φ29

φ23.8

φ29

φ23.8M25x0.75 M25x0.75 M25x0.75

M25x0.75 M25x0.75

36.5

60.2

60.2

60.1

60.3

(0.5)

(0.5)

(0.7)

49.1

42 45

35

51

60 60

3 3

60 60 60

54 54

0.2

0.2

0.2

0.5

0.5

6.7

3.95

56.1

58.7

10.8

14.5

14.3

1322

6.2

25

(0.7)

14.3

1322

6.4

1.8

15.5

6.5

3.13

11.7

13

21.1

5

55

55.5

5

595

595

5 5

42.5

55.5 59 5947.5

47.5

4.5

4.5

2.3

3.5

5 5 5

45°

50°

45°30°

W.D.=23.5

W.D.=17.5

W.D.=4.5

60 60 60

60 60

CFI LU Plan Fluor EPI 5X CFI LU Plan Fluor EPI 10X

45°

CFI LU Plan Fluor EPI 20X φ30

φ23.8

φ30

φ23.8

40°

30°W.D.=1

W.D.=1

φ17.5φ21.8

φ24

CFI LU Plan Fluor EPI 50X

φ8.5

φ18φ21.8

φ24

φ8.8

CFI LU Plan Fluor EPI 100X

φ35

φ36φ34φ30.8

φ36φ34φ30.8

φ36φ34

φ35φ35

φ40φ40

φ30.8 φ30.8φ30.8

φ35.5φ25 φ26.2 (φ28.4) (φ28.4)

φ37 φ37φ33.5

φ27.6

φ33.5 φ35.5 φ35.5

φ19.8φ24.8

φ27φ32.5

φ29.5 φ29.5φ28.5φ23.8

φ28.5

φ34 φ34

φ13φ18.8φ23.3

φ31.5φ26

φ32φ29φ27φ23.8

φ33.5φ29.5

φ31.5

φ20

φ27.5

0.6(CG)

0.6(CG)

0.3(CG)

0.9(CG)

W.D.=10.5

W.D.=3.5

W.D.=1.1

58.2

5W.D.=1.2

11°

(45°）

CFI L PLAN EPI 20XCR

M25x0.75

CFI L PLAN EPI 50XCR

M25x0.75-6g M25x0.75

(7°)

45°

30°

(16°)

45°

6.5

25°

(16°)

45°

6.5

26°

φ11.5

φ19.8φ24.8

φ32.5φ27

φ14.5

CFI L PLAN EPI 100XCRA CFI L PLAN EPI 100XCRB

W.D.=18

W.D.=15

W.D.=4.5

W.D.=1

W.D.=1

M32x0.75 M32x0.75 M32x0.75 M32x0.75 M32x0.75

45°

45°

35°

35°

40.4(Over head screw) 40.4

(Over head screw)

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

CFI LU PLAN FLUOR

CFI L PLAN EPI CR

CFI LU PLAN FLUOR BD

JAPANJAPANJAPANJAPAN

JAPANJAPANL.UL.U

L.UL.U

L.UL.U23.5WD

15A5X /

JAPANJAPAN

L.UL.U

18WD15A5X /

JAPANJAPAN

L.UL.U

15WD30A10X /

JAPANJAPAN

L.UL.U

4.5WD45 A20X /

JAPANJAPAN

L.UL.U

1.0WD90 A100X /

JAPANJAPAN

L.UL.U

1.0WD80 A50X /

17.5WD30A10X /

4.5WD45A20X /

JAPANJAPAN

L.UL.U

1.0WD80A50X /

JAPANJAPANJAPANJAPAN JAPANJAPAN

L 100X / 0.35JAPANJAPAN

L 100X / 0.35L 50X / 0.70L 20X / 0.45

JAPANJAPAN

L.UL.U

1.0WD90A100X /

Objective Lenses

2928

100DA

Main Specifications

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 flareprevention), LV-NU5AC Nosepiece (high-durability motorized universal quintuple, with flare prevention and centering mechanism)

Episcopic illuminator 12V-50W high-intensity halogen lamp; Field (centerable) and aperture diaphragms synchronized with B/D changeover; LV-UEPI ø25mm filter (NCB11, ND16, ND4) insertable; Polarizer/analyzer insertable

Episcopic illuminator 12V-50W high-intensity halogen lamp; High-intensity mercury-fiber illuminator (with brightness control, manual control/PC LV-UEPI2 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 12V-50W high-intensity halogen lamp; High-intensity mercury-fiber illuminator (with brightness control, PC control); LV-U EPI2A 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 (invertedimage, F.O.V 22/25), Y-TT Trinocular (inverted image, F.O.V 22/25), TV tube lens unit 0.5x, 1x




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 ControllerInterface 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-FMAHalogen lamphouse (powered by TE2-PS 100W power source): LV-LH50PC PC (USB1.1) *Software Development Kit (SDK) is available.

Main body Baseless type (column riser insertable between arm and stand); Max. sample height 29mm (with LV-S32 3x2 Stage or LV-S64 6x4Stage), 64mm with column riser; 12V-50W brightness control transformer built in


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 12V-50W high-intensity halogen lamp; High-intensity mercury-fiber illuminator (with brightness control, PC control); LV-UEPI2A 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)


Stage LV-S32 3x2 Stage (stroke: 75x50 mm including glass plate)LV-S64 6x4 Stage (stroke: 150x100 mm including glass plate)





Weight (main body) Approx. 9.9kg

System Diagram

LV150/LV150A

FE

AB

FE

B

II’

I’

F E

P

P'

T

Q

Q'

R

*Not necessary on the LV150A as the operation unit has been built into the main body.

Fiber

S

POWER

MIN. MAX.

PhotomicrographicSystem FX-III Series

Camera Mount

V-T Photo Adapter

Projection LensesPLI 2xPLI 2.5xPLI 4xPLI 5x

ENG-mount CCTV Adapters0.45x0.6x

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 Adapters0.35x0.45x0.6x0.7x

C-mount CCTV AdapterVM2.5x

C-mount CCTV AdapterVM4x

C-mount Direct CCTV Adapter C-mount

Adapter A0.7x

LV-TV TV Tube

0.5x 2nd Objective

Other Eclipse series eyepiece tubes can be used.

LV-TI3 Trinocular Tube ESD


Eyepiece Tubes

LV-SUB Substage

Surugaseiki B23-60CR LV-SUB

Substage 2


C-ER Eyelevel Riser

Y-IDP Double Port (100:0 / 55:45)


LV-UEPI Universal Epi-Illuminator

LV-UEPI2 Universal Epi-Illuminator 2

Intermediate Modules

Episcopic Illuminators

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

StagesLV-LH50PC Precentered Lamphouse

D-LH 12V-100W Precentered Lamphouse (Requires TE2 External Power Supply)

LV-HGFA Fiber Adapter

LV-HL50W 12V-50W-LL Halogen Lamp

12V-100W Lamp

TE2-PS100W Power Supply (YM-EPI3 3-pin extension cord is required)

Lamphouses

L2-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 AdapterM32-25

C-OA 15MM Adapter

DI Objective

TI Objective Adapter

Nosepieces

High-intensity Mercury Fiber Light SourceX-CITE120 (with LV-150)X-CITE120PC (with LV-150A)

AW

W W WLV-NU5ACU5AC Nosepiece(with LV150A)

LED Controller

O

I’

Q S

O

T Q'

R

S


I

P

P'I

ND4ND16

NCB11

λOUT

IN

O P

P'

TQ

Q' R

C-FL Fluorescence Filter Block

LV-PAB Cube

L-AN Analyzer

YM-PO Polarizer

LV-FLAN FL Analyzer

LV-�P �Plate

LV-PO Polarizer

LV-UVPO Polarizer

D-FB Excitation Light Balancer

NCB Slider

ND SliderS

JAPAN

JAPAN

DXM1200C

DS-Fi1Series

DS-2MSeries

CFI UW10x

CFI UW10x M

F.N.ø25F F.N.ø22 E

C-CTCentering

Telescope CFI15x

CFI12.5x

CFI10xCM

CFI10xM

CFI10x

L-W10xESD

Filar Micrometer10xN

Adapter

ENG-mount CCTV Camera C-mount CCTV Camera

Filter Blocks and Sliders

Eyepieces

C-mount Adapter0.55x

30 31

System Diagram

LV100D LV100DA/LV-FMA/LV-FM/LV-IMA/LV-IM

FE

FE

B

Q S

I’O

T Q'

R

S

LV-S32 3x2 Stage

I

P

P'

A

B

I

C

L2-DIC DIC Prism

L-DIHC High Contrast DIC Prism L-NU5 U5

NosepieceL-NBD5 DB5 Nosepiece

C-N C-N6 Nosepiece

P-N P-N5 Nosepiece

Adapter




C-OA 15MM Adapter

DI Objective

TI Objective Adapter

Nosepieces


Camera Mount

V-T Photo Adapter




Relay Lens 1x


Zooming Lens



Relay Lens 1x





Adapter A0.7x

LV-TV TV Tube

0.5x 2nd Objective




Eyepiece Tubes

C-SP Simple Polarizing Polarizer


C-ER Eyelevel Riser








LV-S32PL ESD Plate

LV-S64 6x4 Stage

Stages




12V-100W Lamp


Lamphouses

DF (dry)D-C Abbe

C-C Achromat

LWD Achromat

Slide Achromat 2-100x

Condensers

FiberLV-HGFA Fiber Adapter

F

C

A

Q S

I’O

T Q'

R

S

I

I

P

P'

I

POWER

MIN. MAX.

II’

I’


LED Controller

High-intensity Mercury Fiber Light SourceX-CITE120 (with LV-150)X-CITE120PC (with LV-150A)

ND4ND16

NCB11

λOUT

IN

O P

P'

TQ

Q' R


LV-PAB Cube

L-AN Analyzer

YM-PO Polarizer

LV-FLAN FL Analyzer

LV-�P �Plate

LV-PO Polarizer

LV-UVPO Polarizer


NCB Slider

ND SliderS

JAPAN

JAPAN

DXM1200C

DS-Fi1Series

DS-2MSeries

CFI UW10x

CFI UW10x M


C-CTCentering

Telescope CFI15x

CFI12.5x

CFI10xCM

CFI10xM

CFI10x

L-W10xESD


Adapter



Eyepieces


FE

A

FE

B

W

W WW

I’

I’

I’

Q S

O

O

T Q'

R

R

S

ST Q'

LV-ARM Basic Arm

LV-FMAFM Module A

LV-FMFM Module

LV-IMAIM Module A

LV-IMIM Module

LV-EPI Epi Base LV-DIA Dia Base


LV-UEPI2AMotorized Universal Epi-illuminator 2

A

K

A

K

K

B

(See page 28 for interface)

LV-NU5ACU5AC Nosepiece

E Controller

I

P

P'

P'

FL2FL1DFBF

FL1 FL2

I

I

A

A

K

K

A

KB

DD

I

C

A

K

B

I

C

C

C-SPSimple Polarizing Polarizer

D

I

POWER

MIN. MAX.

II’


LV-TV TV Tube

0.5x 2nd Objective




Eyepiece Tubes

*Not necessary on the LV150A as the operation unit has been built into the main body.

L2-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




C-OA 15MM Adapter

DI Objective TI Objective Adapter

Nosepieces

INTENSILIGHT

DF (dry)D-C Abbe

C-C Achromat

LWD Achromat

Slide Achromat 2-100x

Condensers


V-T Photo Adapter




Relay Lens 1x


Zooming Lens



Relay Lens 1x





Adapter A0.7x

C-ER Eyelevel Riser





Camera Mount



LV-SUB Substage

Surugaseiki B23-60CR LV-SUB

Substage 2


L-S6WH Wafer Holder

L-S6PL ESD Plate


LV-S32PL ESD Plate

LV-S6 6x6 Stage

LV-S64 6x4 Stage

LV-S32 3x2 Stage

Stages

Fiber



LV-HGFA Fiber Adapter


12V-100W Lamp


Lamphouses

LED Controller

ND4ND16

NCB11

λOUT

IN

O P

P'

TQ

Q' R


LV-PAB Cube

L-AN Analyzer

YM-PO Polarizer

LV-FLAN FL Analyzer

LV-�P �Plate

LV-PO Polarizer

LV-UVPO Polarizer


NCB Slider

ND SliderS

JAPAN

JAPAN

DXM1200C

DS-Fi1Series

DS-2MSeries

CFI UW10x

CFI UW10x M


C-CTCentering

Telescope CFI15x

CFI12.5x

CFI10xCM

CFI10xM

CFI10x

L-W10xESD


Adapter



Eyepieces


En

Specifications and equipment are subject to change without any notice or obligation on the part of the manufacturer. January 2007. ©2007 NIKON CORPORATION

This brochure is printed on recycled paper made from 40% used material.

WARNINGTO ENSURE CORRECT USAGE, READ THE CORRESPONDING MANUALS

CAREFULLY BEFORE USING YOUR EQUIPMENT.

Printed in Japan (0701-03)T Code No. 2CE-KVKH-3

NIKON CORPORATIONParale Mitsui Bldg., 8, Higashida-cho, Kawasaki-ku,Kawasaki, Kanagawa 210-0005, Japanphone: +81-44-223-2175 fax: +81-44-223-2182 http://www.nikon-instruments.jp/eng/

NIKON INSTRUMENTS INC.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: +1-631-547-0306http://www.nikonusa.com/

NIKON INSTRUMENTS EUROPE B.V.P.O. Box 222, 1170 AE Badhoevedorp, The Netherlandsphone: +31-20-44-96-222 fax: +31-20-44-96-298http://www.nikon-instruments.com/

NIKON INSTRUMENTS (SHANGHAI) CO., LTD.CHINA phone: +86-21-5836-0050 fax: +86-21-5836-0030(Beijing office) phone: +86-10-5869-2255 fax: +86-10-5869-2277(Guangzhou office) phone: +86-20-3882-0552 fax: +86-20-3882-0580

NIKON SINGAPORE PTE LTDSINGAPORE 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: +82-2-2186-8410 fax: +82-2-555-4415

NIKON CANADA INC.CANADA phone: +1-905-625-9910 fax: +1-905-625-0103

NIKON FRANCE S.A.S.FRANCE phone: +33-1-45-16-45-16 fax: +33-1-45-16-00-33

NIKON GMBHGERMANY 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 AGSWITZERLAND 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 GMBH AUSTRIA AUSTRIA phone: +43-1-972-6111-00 fax: +43-1-972-6111-40

NIKON BELUXBELGIUM phone: +32-2-705-56-65 fax: +32-2-726-66-45

Documents

Industrial Microscopes LV Focusing Moduleszootos.com/home_data/standard/LV150.pdf · 2013. 4. 11. · the shape of a crossed Nicol prism, this cube is used for DIC observations. It