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Chronology and Evolution of Mars pp 411–424Cite as

The Atmosphere of Mars as Constrained by Remote Sensing

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Part of the book series: Space Sciences Series of ISSI ((SSSI,volume 12))

Abstract

In addition to the Viking in-situ mass spectrometry measurements, our knowledge of the Martian atmosphere comes from remote sensing spectroscopy from the ground and from space. In particular, infrared measurements from the Mariner 9, Viking, Phobos and MGS orbiters have provided information upon the thermal profile, the chemical composition, the stratospheric winds, some isotopic ratios, and the properties of suspended dust. However, further remote sensing monitoring is still needed for a better understanding of the water cycle, a more accurate knowledge of the minor species and the aerosol composition, an improved measurement of the hydrogen and oxygen isotopic ratios, and for a full mapping of the middle altitude winds. Some of these information will be provided with the Mars Express mission.

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  1. DESPA, Observatoire de Paris, 92195, Meudon, France

    Therese Encrenaz

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  1. Therese Encrenaz
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Correspondence to Therese Encrenaz .

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  1. International Space Science Institute, Bern, Switzerland

    Reinald Kallenbach  & Johannes Geiss  & 

  2. Planetary Science Institute, Tucson, USA

    William K. Hartmann

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Encrenaz, T. (2001). The Atmosphere of Mars as Constrained by Remote Sensing. In: Kallenbach, R., Geiss, J., Hartmann, W.K. (eds) Chronology and Evolution of Mars. Space Sciences Series of ISSI, vol 12. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1035-0_16

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  • DOI: https://doi.org/10.1007/978-94-017-1035-0_16

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