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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.
Vise andre og tillknytning
2012 (engelsk)Inngår i: Planetary and Space Science, ISSN 0032-0633, E-ISSN 1873-5088, Vol. 63-64, s. 62-82Artikkel i tidsskrift (Fagfellevurdert) 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

sted, utgiver, år, opplag, sider
2012. Vol. 63-64, s. 62-82
HSV kategori
Forskningsprogram
Rymdteknik
Identifikatorer
URN: urn:nbn:se:ltu:diva-2972DOI: 10.1016/j.pss.2011.10.013ISI: 000302672200009Scopus ID: 2-s2.0-84858073318Lokal ID: 0b79c322-b38b-420e-a31f-a61e6bf47e61OAI: oai:DiVA.org:ltu-2972DiVA, id: diva2:975827
Merknad
Validerad; 2012; 20111114 (ysko)Tilgjengelig fra: 2016-09-29 Laget: 2016-09-29 Sist oppdatert: 2018-07-10bibliografisk kontrollert

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