Imaging with a thick lens Flashcards
why use cardinal points?
the basic imaging properties such as image size, location, and orientation are completely determined by the locations of the cardinal points
Where do we act like all the refractions occur at in thick lens?
principal planes
nodal points
have the property that a ray aimed at one of them will be refracted by the lens such that it appears to have come from the other. and with the same angle with respect to the optical axis
Assumptions of thin lenses
- both sides in same medium
- lens is thin, 0 thickness
- paraxial approximation
how can you tell in a thin lens, that the same medium is on both sides of the lens
equal focal lengths on either side of the lens
if the focal length is shorter on one side of the thin lens…
the short side is in a medium with higher RI
principle plane
- refraction happens at principle plane
- not really a flat surfaces
- curved
principal point
where the principle plane intersects the optical axis
Rule number 1 in thick lens
parallel then refracts at H’
rule number 3 of thick lens
goes towards N, goes straight across to N’ and then comes out of lens at the same angle as it entered lens
ANGLE PRESERVATION
there is a virtual parallel displacement from N’ to N
P=N
in a lot of thick lens systems, but not always
actual rays
are subjected to two refractions, one per refracting surface
conventional rays
change path only when encounter the prinicple planes (parallel and focal ray) or the nodal points (the nodal/radial ray)
Ray propagation in a thick lens
rays do not pass through the cardinal points, however it is very useful to follow the rules of conventional rays to find the final path of any ray
object distance in thick lens
measured from H