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A point source as imaged by a system with negative (top), zero (center), and positive (bottom) spherical aberration. Images to the left are defocused
A point source as imaged by a system with negative (top), zero (center), and positive (bottom) spherical aberration. Images to the left are defocused toward the inside, images on the right toward the outside.
The point spread function of Hubble Space Telescope's WFPC camera before corrections were applied to its optical system.
The point spread function of Hubble Space Telescope's WFPC camera before corrections were applied to its optical system.
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The MTF data versus spatial frequency is normalized by fitting a sixth order polynomial to it, making a smooth curve. The 50% cut-off frequency is det
The MTF data versus spatial frequency is normalized by fitting a sixth order polynomial to it, making a smooth curve. The 50% cut-off frequency is determined and the corresponding spatial frequency is found, yielding the approximate position of best focus.
In evaluating the ESF, an operator defines a box area equivalent to 10%[citation needed] of the total frame area of a knife-edge test target back-illu
In evaluating the ESF, an operator defines a box area equivalent to 10%[citation needed] of the total frame area of a knife-edge test target back-illuminated by a black body. The area is defined to encompass the edge of the target image.