OTA Baffle Rejection Measurement-Revised

Details OTA Baffle Rejection Measurement-Revised OTA Baffle Rejection Measurement-Revised

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3142b&link_type=abstract

HST Proposal ID #3142

Physics

Hst Proposal Id #3142

Scientific paper

Test Objective: Measure the effectiveness of the HST OTA baffle system in rejecting light of nearby bright objects. Verify that the stray light tolerance (23rd magnitude/square arcsec at the focal plane) is met with the present viewing limits established for the sun (>50 degrees), moon (>15 degrees) and the bright earth limb (>80 degrees) from the OTA axis.

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