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Mariner 9 Ultraviolet Spectrometer Experiment
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This article is published in Astronomy and Astrophysics.The article was published on 1973-11-01 and is currently open access. It has received 29 citations till now. The article focuses on the topics: Spectrometer.read more
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The Global Topography of Mars and Implications for Surface Evolution
David E. Smith,Maria T. Zuber,Maria T. Zuber,Sean C. Solomon,Roger J. Phillips,James W. Head,James B. Garvin,W. Bruce Banerdt,Duane O. Muhleman,Gordon H. Pettengill,Gregory A. Neumann,Gregory A. Neumann,Frank G. Lemoine,James B. Abshire,Oded Aharonson,C. David,Brown,Steven A. Hauck,Anton B. Ivanov,Patrick J. McGovern,H. Jay Zwally,Thomas C. Duxbury +21 more
TL;DR: Elevations measured by the Mars Orbiter Laser Altimeter have yielded a high-accuracy global map of the topography of Mars, which includes the low northern hemisphere, the Tharsis province, and the Hellas impact basin.
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The Mars Observer laser altimeter investigation
Maria T. Zuber,David E. Smith,Sean C. Solomon,Duane O. Muhleman,James W. Head,James B. Garvin,James B. Abshire,Jack L. Bufton +7 more
TL;DR: The Mars Observer laser altimeter (MOLA) was used to determine globally the topography of Mars at a level suitable for addressing problems in geology and geophysics as mentioned in this paper.
Journal ArticleDOI
Physical properties of the particles composing the Martian dust storm of 1971–1972
TL;DR: In this article, the infrared interferometric spectrometer (IRIS) data collected by the Mariner 9 spacecraft during the global Martian dust storm of 1971-1972 is analyzed to study the particle sizes in detail, estimate the dust particle size distribution, and determine the dust optical depth.
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Thermal structure of the Martian atmosphere during the dissipation of the dust storm of 1971
TL;DR: In this paper, the authors examined the secular variation of the thermal structure of the Martian atmosphere during the dissipation phase of the 1971 dust storm using temperatures obtained by the infrared spectroscopy investigation on Mariner 9.
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Mars aerosol studies with the MGS TES emission phase function observations: Optical depths, particle sizes, and ice cloud types versus latitude and solar longitude
TL;DR: In this paper, TES solar band and infrared (IR) spectral EPF sequences were analyzed to obtain first-time seasonal/latitudinal distributions of visible optical depths, particle sizes, and single scattering phase functions.