A nearly perfect paraboloidal mirror has a residual RMS surface error of /40, where A is the wavelength of light. The mirror focuses light from a distant star on axis. What is the resulting wavefront error after the reflection from the mirror if one neglects the effect of atmospheric seeing? Find Strehl ratio for the mirror and the amount of energy concentrated in the central maximum of the star image.

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A nearly perfect paraboloidal mirror has a residual RMS surface error of /40, where A is the wavelength
of light. The mirror focuses light from a distant star on axis. What is the resulting wavefront error after
the reflection from the mirror if one neglects the effect of atmospheric seeing? Find Strehl ratio for the
mirror and the amount of energy concentrated in the central maximum of the star image.
Transcribed Image Text:A nearly perfect paraboloidal mirror has a residual RMS surface error of /40, where A is the wavelength of light. The mirror focuses light from a distant star on axis. What is the resulting wavefront error after the reflection from the mirror if one neglects the effect of atmospheric seeing? Find Strehl ratio for the mirror and the amount of energy concentrated in the central maximum of the star image.
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