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Overview of the Martian atmospheric submillimetre sounder FIRE
National Institute of Information and Communication Technology, Tokyo.
National Institute of Information and Communication Technology, Tokyo.
Institute of Space and Astronautical Science, Chuoku, Sagamihara, Kanagawa.
Osaka Prefecture University, Naka, Sakai.
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2012 (English)In: Planetary and Space Science, ISSN 0032-0633, E-ISSN 1873-5088, Vol. 63-64, 62-82 p.Article in journal (Refereed) Published
Abstract [en]

We propose a submillimetre-wave atmospheric emission sounding instrument, called Far-InfraRed Experiment (FIRE), for the Japanese Martian exploration programme Mars Exploration with Lander-Orbiter Synergy (MELOS). The scientific target of FIRE/MELOS is to understand the dust suspended meteorology of the Mars. FIRE will provide key meteorological parameters, such as atmospheric temperature profiles for outside and inside dust storms, the abundance profile of the atmospheric compositions and their isotopes, and wind velocity profiles. FIRE will also provide the local time dependency of these parameters. The observational sensitivity of FIRE/MELOS is discussed in this paper. FIRE will explore the meteorological system of the Martian atmosphere including the interaction between its surface and atmosphere

Place, publisher, year, edition, pages
2012. Vol. 63-64, 62-82 p.
National Category
Aerospace Engineering
Research subject
Space Technology
Identifiers
URN: urn:nbn:se:ltu:diva-2972DOI: 10.1016/j.pss.2011.10.013Local ID: 0b79c322-b38b-420e-a31f-a61e6bf47e61OAI: oai:DiVA.org:ltu-2972DiVA: diva2:975827
Note
Validerad; 2012; 20111114 (ysko)Available from: 2016-09-29 Created: 2016-09-29 Last updated: 2017-11-21Bibliographically approved

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