Published online by Cambridge University Press: 14 March 2018
The traditional polarizing microscope equipped with crossed linear polarizers shows a picture in which the image contrast of a birefringent object depends on both the amount of relative retardation induced by the object and the orientation of its principal axis. For example, if the orientation of the principal axis is parallel to one of the polarizers, then the birefringent object becomes invisible. For best visibility, the principal axis must be oriented at 45° to the polarizers. In addition, the image intensity of the object is proportional to the square of the sine of the relative phase shift between the ordinary and the extraordinary ray passing through the object. The addition of a waveplate as compensator to the optical train provides the opportunity to improve the contrast and measure the relative retardation, but the principal restrictions of orientation dependence and non-linear image contrast remains.