Structure of the Martian atmosphere from ε-Gem occultation observations

W. B. Hubbard

doi:10.1016/0273-1177(82)90110-7

Structure of the Martian atmosphere from ε-Gem occultation observations

W. B. Hubbard

Lunar and Planetary Lab

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

Abstract

We have collected information about Martian atmospheric scale heights derived from observations of the occultation of ε{lunate} Gem by Mars on April 8, 1976. The observations give data in the altitude range ∼50 to 80 km. A rough, unweighted average of results so far available yields a temperature of ∼165°K. Excursions of ∼±40°K about this mean may be present as a function of both altitude and areographic coordinates.

Original language	English (US)
Pages (from-to)	103-106
Number of pages	4
Journal	Advances in Space Research
Volume	2
Issue number	2
DOIs	https://doi.org/10.1016/0273-1177(82)90110-7
State	Published - 1982

ASJC Scopus subject areas

Aerospace Engineering
Astronomy and Astrophysics
Geophysics
Atmospheric Science
Space and Planetary Science
General Earth and Planetary Sciences

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10.1016/0273-1177(82)90110-7

Cite this

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title = "Structure of the Martian atmosphere from ε-Gem occultation observations",

abstract = "We have collected information about Martian atmospheric scale heights derived from observations of the occultation of ε{lunate} Gem by Mars on April 8, 1976. The observations give data in the altitude range ∼50 to 80 km. A rough, unweighted average of results so far available yields a temperature of ∼165°K. Excursions of ∼±40°K about this mean may be present as a function of both altitude and areographic coordinates.",

author = "Hubbard, {W. B.}",

note = "Funding Information: Supported in part by NASA Grant NSG-7045.",

year = "1982",

doi = "10.1016/0273-1177(82)90110-7",

language = "English (US)",

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N1 - Funding Information: Supported in part by NASA Grant NSG-7045.

PY - 1982

Y1 - 1982

N2 - We have collected information about Martian atmospheric scale heights derived from observations of the occultation of ε{lunate} Gem by Mars on April 8, 1976. The observations give data in the altitude range ∼50 to 80 km. A rough, unweighted average of results so far available yields a temperature of ∼165°K. Excursions of ∼±40°K about this mean may be present as a function of both altitude and areographic coordinates.

AB - We have collected information about Martian atmospheric scale heights derived from observations of the occultation of ε{lunate} Gem by Mars on April 8, 1976. The observations give data in the altitude range ∼50 to 80 km. A rough, unweighted average of results so far available yields a temperature of ∼165°K. Excursions of ∼±40°K about this mean may be present as a function of both altitude and areographic coordinates.

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ER -

Structure of the Martian atmosphere from ε-Gem occultation observations

Abstract

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