Submission of Earth-based ring occultation observations to the NASA planetary data system rings discipline node

Details Submission of Earth-based ring occultation observations to the NASA planetary data system rings discipline node Submission of Earth-based ring occultation observations to the NASA planetary data system rings discipline node

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993well.rept.....f&link_type=abstract

Technical Report, 1 Jul. 1992 - 30 Jun. 1993 Wellesley Coll., MA.

Computer Science

Planetary Rings, Stellar Occultation, Data Systems, Uranus (Planet)

Scientific paper

This is a technical report summarizing our progress in our program of contributing high quality Earth-based occultation observations to NASA's Planetary Data System (PDS) Rings Node. During our first year of funding, we selected five data sets for eventual inclusion in the PDS Rings Node. These were Uranus occultation observations obtained by the PI and co-workers from the IRTF of event stars U34 (26 April 1986), U1052 (5 May 1988), U65 (21 June 1990), U7872 (25 June 1991), and U7808 (28 June 1991). In our original proposal, we described four tasks: data sets to a common format; documentation of the occultation observations and associated calibrations; calculation of the occultation geometry for each event; establish prototype PDS templates. As discussed in our renewal proposal, submitted 8 June 1993, we have completed the first three tasks, and are working on the fourth. As an indication of our progress to date, we provide information about each of the data sets, their formats, the documentation, and the method used for reconstructing the occultation geometry.

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