The occultation of Epsilon Geminorum by Mars as observed at Princeton

Details The occultation of Epsilon Geminorum by Mars as observed at Princeton The occultation of Epsilon Geminorum by Mars as observed at Princeton

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978aj.....83..442g&link_type=abstract

Astronomical Journal, vol. 83, Apr. 1978, p. 442-446. Research supported by the Alfred P. Sloan Foundation, NSF, and NASA.

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2

Astronomical Photometry, Atmospheric Temperature, Mars Atmosphere, Occultation, Aerial Reconnaissance, Airborne Equipment, Atmospheric Models, Electrophotometry, Scintillation, Temperature Profiles

Scientific paper

Results are reported for two-color (red and blue) high-speed photometric observations of the April 8, 1976, occultation of Epsilon Gem by Mars. The observing system is briefly described, fits to an isothermal atmospheric model of the event are presented, and the blue data are used to derive temperature profiles of the Martian atmosphere in the manner of Wasserman and Veverka (1973). The results are compared with those of Elliot et al. (1977), which were obtained from the NASA Kuiper Airborne Observatory.

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