The occultation of Epsilon GEM by Mars as observed from Agassiz Station

Details The occultation of Epsilon GEM by Mars as observed from Agassiz Station The occultation of Epsilon GEM by Mars as observed from Agassiz Station

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978icar...35..395l&link_type=abstract

Icarus, vol. 35, Sept. 1978, p. 395-399.

Physics

1

Atmospheric Temperature, Mars Atmosphere, Stellar Occultation, Temperature Profiles, Density (Number/Volume), Light Curve, Temperature Measurement, Light Curve, Occultations, Structure, Mars, Waves, Observations, Temperatures, Atmosphere, Density, Photometry, Light (Visible Radiation), Refraction, Epsilon Geminorum

Scientific paper

Observations of the April 8, 1976, occultation of Epsilon Gem by Mars made at the Agassiz Station of the Harvard College Observatory have been analyzed to yield temperature profiles of the Martian atmosphere for number densities between 10 to the 13th and 10 to the 15th power per cu cm. Pronounced wavelike structure is evident in both immersion and emersion profiles, with a peak-to-peak variation of up to 50 K and a vertical scale of 20 km.

Affiliated with

Also associated with

No associations

Rating

The occultation of Epsilon GEM by Mars as observed from Agassiz Station does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The occultation of Epsilon GEM by Mars as observed from Agassiz Station, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The occultation of Epsilon GEM by Mars as observed from Agassiz Station will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-941792