OPTICS PHYSICS LAB Lab Equipment Manufacturer, Supplier and Exporter in India

It is used for taking For Taking Direct Wavelength 

 It separates the different colors of light so that we can discover the composition of an object.

It is used to to determine the thickness of a glass plate using a spherometer and to determine the radius of curvature of a given spherical surface using a spherometer.

It is used to to determine the thickness of a glass plate using a spherometer and to determine the radius of curvature of a given spherical surface using a spherometer.

It Consist of  a convex lens 38 mm diameter & 150 mm focal length, placed in a plastic tube 400 x 50 mm diameter, & a double convex lens 50 mm diameter & 500mm focal length, placed in a tube 400 x 55 mm diameter

In this telescope the TV camera functions as the eye, so what the eye sees can be viewed on a monitor or the rear projection screen. A 5 cm convex lens acts as the eyepiece and a 20 cm convex lens is the objective lens, with the TV camera focused at infinity (relaxed eye). The rule is positioned across the lecture hall (at infinity) from the telescope.

It consist of  a convex lens 38 mm diameter & 150 mm focal length, mounted in a plastic tube 400 x 50 mm diameter, & a double convex lens 50 mm diameter & 500mm focal length, mounted in a tube 400 x 55 mm diameter. The smaller tube is located in the large tube by means of foam plastic rings which provide an effective sliding light seal, with plano concave eye piece lens to provide erect image.. 

It is invented for general laboratory work. The telescope is placed on 18 mm diameter, pillar 450 mm long fitted on a heavy tripod base

It Uses a single positive lens to obtain parallel rays, creating a source (stars) at infinity. The long focal length concave mirror is used as the telescope mirror. Before the focal point of the concave mirror, a small plane mirror is inserted, shifting the focus to a point below the incoming light beam. The small mirror can actually be either plane, concave or convex, producing different types of reflecting telescopes, or it can be eliminated fully, with the observer or film at the focus of the primary mirror.

A travelling microscope is used to determine small distance to an accuracy of 0.001 cm. The measurement principle is based on the principle of vernier. In a typical travelling microscope, the main scale divisions are of magnitude 0.05 cm (0.5 mm) each and the vernier scale contains 50 divisions.