Specifications LV100ND

Base unit:	Maximum sample height: 38 mm (when used with LVNU5AI U5AI nosepiece and LV-S32 3x2 stage / LV-S64 6x4 stage) * 73 mm when used with one column riser 12V50W internal power source for dimmer, coarse and fine adjustment knobs Left: coarse and fine adjustment / Right: fine adjustment, 40 mm stroke Coarse adjustment: 14 mm/turn (with torque adjustment, refocusing mechanism) Fine adjustment: 0.1 mm/turn (1 μm/graduation) Stage mounting hole intervals: 70 x 94 (fixed by 4-M4 screw)
Nosepieces:	C-N6 ESD Sextuple Nosepiece ESD LV-NU5 Universal Quintuple Nosepiece ESD LV-NBD5 BD Quintuple Nosepiece ESD LV-NU5I Intelligent Universal Quintuple Nosepiece ESD
Episcopic Illuminator:	LV-UEPI-N LV-LH50PC 12V50W Precentered Lamphouse Bright/darkfield switch and linked aperture stop (centerable), field diaphragm (centerable) Accepts ø 25 mm filter (NCB11, ND16, ND4), polarizer/analyzer, plate, excitation light balancer; equipped with noise terminator LV-UEPI2 LV-LH50PC 12V50W Precentered Lamphouse HG precentered fiber illuminator: C-HGFIE (with light adjustment) *option Bright/darkfield switch and linked aperture stop (centerable), field diaphragm (centerable), automated optical element switching feature matched to brightfield, darkfield, and epi-fluorescence switch Accepts ø 25 mm filter (NCB11, ND16, ND4), polarizer/analyzer, λ plate, excitation light balancer; equipped with noise terminator
Eyepiece tubes:	LV-TI3 trinocular eyepiece tube ESD (Erected image, FOV: 22/25) LV-TT2 TT2 tilting trinocular eyepiece tube (Erected image, FOV: 22/25) C-TB binocular tube (Inverted image, FOV: 22) P-TB Binocular Tube (Inverted image, FOV: 22) P-TT2 Trinocular Tube (Inverted image, FOV: 22)
Stages:	LV-S32 3x2 stage (Stroke: 75 x 50 mm with glass plate) ESD compatible LV-S64 6x4 stage (Stroke: 150 x 100 mm with glass plate) ESD compatible LV-S6 6x6 stage (Stroke: 150 x 150 mm) ESD compatible
Eyepieces:	CFI eyepiece series
Objective lenses:	Industrial Microscope CFI60-2/CFI60 optical system Objective lens series: Combinations in accordance with the observation method
ESD performance:	1000 to 10V, within 0.2 sec. (excluding certain accessories)
Power consumption:	1.2A/75W
Weight:	Approximately 8.6kg

Specifications LV100NDA

Base unit:	Maximum sample height: 33 mm (when used with LVNU5AI U5AI nosepiece and LV-S32 3x2 stage / LV-S64 6x4 stage) * 73 mm when used with one column riser 12V50W internal power source for dimmer, coarse and fine adjustment knobs Left: coarse and fine adjustment / Right: fine adjustment, 40 mm stroke Coarse adjustment: 14 mm/turn (with torque adjustment, refocusing mechanism) Fine adjustment: 0.1 mm/turn (1 μm/graduation) Stage mounting hole intervals: 70 x 94 (fixed by 4-M4 screw)
Nosepieces:	LV-NU5 Motorized Universal Quintuple Nosepiece (High-durability motorized 5-hole universal nosepiece)
Episcopic Illuminator:	LV-UEPI2A LV-LH50PC 12V50W Precentered Lamphouse HG precentered fiber illuminator: C-HGFIE (with light adjustment: PC controlled) *option Motorized operation and control of illumination selector turret Motorized aperture stop linked to brightfield/ darkfield selector (automatic optimization matched to objective lens), field diaphragm (centerable) Accepts ø 25 mm filter (NCB11, ND16, ND4), polarizer/analyzer, λ plate, excitation light balancer; equipped with noise terminator
Diascopic Illumniator:	LV-LH50PC 12V50W Precentered Lamphouse (Fly Eye optical system) Internal aperture, field diaphragm, filter (ND8, NCB11); transmitted/ reflected selector switch; 12V100W also available (option)
Eyepiece tubes:	LV-TI3 trinocular eyepiece tube ESD (Erected image, FOV: 22/25) LV-TT2 TT2 tilting trinocular eyepiece tube (Erected image, FOV: 22/25) C-TB binocular tube (Inverted image, FOV: 22) P-TB Binocular Tube (Inverted image, FOV: 22) P-TT2 Trinocular Tube (Inverted image, FOV: 22)
Stages:	LV-S32 3x2 stage (Stroke: 75 x 50 mm with glass plate) ESD compatible LV-S64 6x4 stage (Stroke: 150 x 100 mm with glass plate) ESD compatible LV-S6 6x6 stage (Stroke: 150 x 150 mm) ESD compatible
Eyepieces:	CFI eyepiece series
Objective lenses:	Industrial Microscope CFI60-2/CFI60 optical system Objective lens series: Combinations in accordance with the observation method
ESD performance:	1000 to 10V, within 0.2 sec. (excluding certain accessories)
Power consumption:	1.2A/90W
Weight:	Approximately 10kg

Industrial Microscopes

ECLIPSE LV100ND / LV100NDA

Key Features

Motorized microscope with episcopic/diascopic illumination that enables control of objectives and light intensity from camera control unit and automatically detects observation method

A manual microscope with episcopic/diascopic illumination ,which meets the various needs of observation, inspection, research, and analysis across a wide range of industrial fields. Higher NA and a longer working distance than ever before mean superior optical performance and efficient digital imaging.
Max. sample size: 150 x 150 mm

Modularized microscope body applicable with various observations and tasks

Compatible with brightfield, darkfield, simple polarizing, DIC, epifluorescence and two-beam interferometry observations.
Furthermore, phase contrast and DIC observation with diascopic illumination are also possible.
It supports diverse and advanced research, analysis and inspection.

Compatible observation methods
	Brightfield	Darkfield	DIC	Fluorescence	Polarizing	Phase contrast	Two-beam interferometry
Episcopic	◯	◯	◯	◯	◯	—	◯
Diascopic	◯	◯	◯	—	◯	◯	—

*Select suitable lens for each observation.

Newly developed CFI60-2 series provides the ultimate in long working distance levels and the most advanced chromatic aberration in a light weight body

CFI60-2 series offers higher NA and longer working distances than ever before.

For more information, see the chart

[fig.] — Objectives for brightfield observation (epi)

Easy digital imaging

Through the combination of the Intelligent Nosepiece LV-NU5I and Nosepiece Adapter LV-INAD, information about the objective in use is detected and displayed in the monitor via the camera control unit. In addition, the information is automatically converted to appropriate calibration data when changing magnification.