Polarizing Microscope IMP-1100 Series equipped with a high degree of sensitivity and best suited for anisotropic (mineral) specimens such as geology, minerals, metallurgy, university teaching laboratories, and other sectors. Built-in bertrand lens, polarizer, and analyzer, 360° rotatable round stage, filter, condenser, etc. The binocular and trinocular viewing head with wild field eyepieces and has an excellent strain-free infinite plan: 4X, 10X, 20X(S), 40X(S) with optional choice 60X(S) objectives, and each eye tube has interpupillary adjustment. This series is capable of providing strong images with a broad field of
Description
Specification
Technical
Polarizing Microscope IMP-1100 Series equipped with a high degree of sensitivity and best suited for anisotropic (mineral) specimens such as geology, minerals, metallurgy, university teaching laboratories, and other sectors. Built-in bertrand lens, polarizer, and analyzer, 360° rotatable round stage, filter, condenser, etc. The binocular and trinocular viewing head with wild field eyepieces and has an excellent strain-free infinite plan: 4X, 10X, 20X(S), 40X(S) with optional choice 60X(S) objectives, and each eye tube has interpupillary adjustment. This series is capable of providing strong images with a broad field of view, the multipurpose, and perfect for basic studies of samples properties. Come with 6V/20W halogen lamp lights, allowing samples to be illuminated for a more comprehensive field of view. Accomplished with the help of particular devices known as retardation plates and optical compensators. The first-order retardation plate is used in optical path differences ranging from a fraction of a wavelength up to several wavelengths. This flexible and multipurpose tool is known by different names, comprising a red plate, red-one plate, lambda (λ) plate, gypsum plate, selenite plate, sensitive violet, or simply a color tint plate and quartz wedge plate is a simple, semi-quantitative optical compensator used to examine optical path differences in a wide range of samples by the quartz wedge. Built-in a crystalline block of quartz provides a parallel or perpendicular optical axis to the edge of the birefringent crystal.
Accomplished with the help of particular devices known as retardation plates and optical compensators.
Strain-free infinite plan objective, and adjustable quadruple nosepiece
Gypsum λ Slip, First Class Red, 1/4λ Slip, (â… -â…£ Class) Quartz Wedge optical compensate system
Wild field WF 10×/18mm, WF 10×/18mm with reticule 0.1mm eyepieces
Coaxial coarse & fine focusing knobs, travel range of length 26 mm, Scale:2 um
360° rotatable round stage, center adjustable, division 1°, vernier division, lockable, stage of 146 mm
Abbe N.A. 1.25 Strain-free condenser
6V/20W Halogen Lamp light source
Different filters including Blue(optional:Amber,Green,Neutral) filters
Binocular 30° inclined and a 360° rotatable head with interpupillary distance 48 to 75 mm and trinocular 30° inclined and a 360° rotatable head with interpupillary distance 48 to 75 mm
Small foot print and light weight
Easy operating with ergonomic design
Excellent image quality with color corrected infinite optical system
Optional accessories C-mount, Filter
6V/30W Halogen Lamp Illumination as an optional accessories
Built-in a crystalline block of quartz provide parallel or perpendicular optical axis to the edge of the birefringent crystal