Using APART for wall visibility calculations in the calibration channel of wide field planetary camera II

Details Using APART for wall visibility calculations in the calibration channel of wide field planetary camera II Using APART for wall visibility calculations in the calibration channel of wide field planetary camera II

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993spie.1753..244s&link_type=abstract

In: Stray radiation in optical systems II; Proceedings of the Meeting, San Diego, CA, July 20-22, 1992 (A93-55176 24-74), p. 244

Computer Science

Cameras, Charge Coupled Devices, Instrument Compensation, Light Scattering, Wide Angle Lenses, Image Processing, Pixels, Visibility

Scientific paper

The cone visibility from the CCD detector array plane in the calibration channel of wide field planetary camera II (WFPC II) is analyzed, using APART, for three representative wavelengths as characterized by indices of refraction. The light pipe walls are visible from the corners of the equivalent CCD detector array when imaging with the smallest index of refraction, n = 1.375. Painting the inside of the light pipe walls will result in a decrease in their visibility.

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