Hsp Stellar Occultation by Planetary Rings HSP-09A

Details Hsp Stellar Occultation by Planetary Rings HSP-09A Hsp Stellar Occultation by Planetary Rings HSP-09A

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.2771b&link_type=abstract

HST Proposal ID #2771

Other

Hst Proposal Id #2771

Scientific paper

This proposal defines the procedure for the verification of the occultation mode of observation on the HSP using the beamsplitter to simultaneously observe with both IDT#3(VIS) and the PMT. This test verifies many procedures employed by all occultation observa- tions, through observation of an occultation by a planetary ring system. The effect of the HSP motion on the predicted times of the occultation events minimal. The immersion of a star will be observed for Saturn while tracking on the star. Revision: EER 6/9/89 RPSS V 7.0 Local & RPS; asb @ MIT Jul 28, 1989 14:30; rlw @ STScI Aug 8, 1989 10:30; asb @ MIT Aug 11, 1989 15:00; SAL-M 8/15/89 RPSS V7.2 : Changed INT-ACQ to ONBRD-ACQ & other changes; Changed PMT dark target - SALM 10/12/89; asb @ MIT 19 Mar 1990 13:30: updated target list; asb @ MIT 17 May 1990 11:00: additional targets for SV; pstanley - New RPSS version 5/30/90; Fixed for aberration problem - asb @ MIT 27 July 1990; Changes to targets/observations--amanda; Fixed small syntax error (must specify cycle parameter)--BJW 5/10/91; Changes to observing strategies per 6/4/91 meeting - ps

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