| qshpang |
2007-05-05 14:30 |
Lens and images
Lens and images
z2vrV?: ts`c_hH,1' Introduction: Along with mirrors, lens complete the set of simple optical elements. Lens 2.{:PM4Z4 have been used for hundreds of years. Galileo constructed the first telescope from a pair of lens i^eU!^KF in 1609 and used it to discover, among other things, several of Jupiter’s moons. A lens forms F" FGPk images by bending the incoming light as it passes. Image formation can be understood by \HF|&@}hU treating the incoming light as rays and using a simple geometric arguments. Like much of basic zlco?Rt physics, this approach isn’t completely correct but is a good approximation. Because of the F.i*'x0u geometric nature of the approximation, one can analyze a lens with geometry. This sort of
eU&[^ approach is called ray tracing. In today’s lab, we will form images with lens and analyze the
wwE`YY system with ray tracings and with equations.
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