experiment 8 - aberrations Flashcards
what is spacial resolution limited by ?
spatial resolution is limited by diffraction , higher order aberrations and scattered light
what happens to rays close to the axis ?
rays close to the axis focus at the paraxial region
what happens as we increase aperture size?
rays no longer focus in the paraxial image plane
why do we need a spherical ideal wave front ?
- the paraxial rays which originate very close to axis they appear to be part of a spherical surface which is paraxial wave front
- only a spherical surface sends all the rays to the same point because they are simply radii of curvature and they all point to centre of sphere
what happens when increase ray height ?
- we move from the paraxial wavefront to the real wavefront , the two no longer coincide
- the real wavefront is displaced with respect to paraxial wavefront
- when object is on axis the real wavefront is displaced symmetrically
what is the wavefront aberration function ?
𝛿W(x,y) maps the difference between the ideal wavefront surface ( which is always a perfect sphere ) and the actual wavefront surface( which encodes the aberrations in the lens)
what does the distortions you have on real wavefront surface compared to ideal wavefront surface encode ?
- the distortions you have on real wavefront surface compared to ideal wavefront surface encode all the aberrations
what should 𝛿W be for every point if system is aberration free ?
- if system is free from any aberrations then 𝛿W ( wavefront )for every point should be zero
- real wavefront matches ideal wavefront and you end up with ideal image formation
how do astronomers probe the universe ?
by getting the best possible image with optical instruments
what does presence of spherical aberration do in terms of spacial resolution ?
the presence of spherical aberrations reduces spacial resolution that can be achieved in the absence of aberration
what are the key parameters affecting optical aberrations ?
1- (β ) object field angle - if object is on axis , object field angle will be 0 and image will be on axis
2- (θ )specifies meridian in exit pupil plane
3-(h) specifies ray height in exit pupil plane
what are the key parameters affecting optical aberrations ?
1- (β ) object field angle - if object is on axis , object field angle will be 0 and image will be on axis
2- (θ )specifies meridian in exit pupil plane
3-(h) specifies ray height in exit pupil plane
what is spherical aberration ?
- proportional to the 4th power of ray height
- b determines how much spherical aberration you have
- no β - which means that spherical aberration is a large on axis as off axis
- spherical aberration independent of object field angle
- big aperture = lot of spherical aberration
what is coma ?
- proportional to object field angle
- proportional to value of cosine of angle θ
- when object is on-axis , the coma will be 0
- absent on axis
what is astigmatism ?
- proportional to the square of object field angle
- proportional to β so no on-axis astigmatism
- off axis
what is field curvature ?
- best plane for off-axis object point is closer to the lens
- quality of image isn’t affected by field curvature
what is distortion ?
- quality of image point is not affected by distortion
- images generated are no longer geometrically similar to objects that generate those images
- proportional to the third power of object field angle
what does b1,b2,b3,b4,b5 means ?
- constants that determine the size of each aberration term
what are the effects of primary seidel aberrations ?
. expanded size for a point image ( spherical aberration ,coma and astigmatism ) as they affect the quality of the image
. curved image plane ( field curvature )
. extended images are no longer geometrically similar to the object ( distortion )