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The martian plasma environment: Electric field and Langmuir probe diagnostics
KTH, Tidigare Institutioner, Alfvénlaboratoriet. KTH, Skolan för elektro- och systemteknik (EES), Rymd- och plasmafysik.
KTH, Skolan för elektro- och systemteknik (EES), Rymd- och plasmafysik. KTH, Tidigare Institutioner, Alfvénlaboratoriet.
2003 (engelsk)Inngår i: IEEE Transactions on Plasma Science, ISSN 0093-3813, E-ISSN 1939-9375, Vol. 31, nr 6, s. 1232-1236Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

The plasma environment of Mars has been studied by a small handful of spacecraft. From the sparse observations that exist, one may conclude that the solar wind-Martian magnetosphere interaction is different in significant ways from the solar wind's interaction with Earth's magnetosphere. Mars offers an opportunity to make significant advances in our understanding of the fundamentals of the solar wind's interaction with cold celestial bodies, with suitable plasma instrumentation orbiting the planet. We briefly review what is known about Mars' plasma environment and address some scientific topics that can be studied by proper plasma instrumentation in Mars' vicinity, in particular the scientific potential of Langmuir probe measurements. Finally, we exemplify how the studies may contribute to an enhanced understanding not only of the plasma surrounding Mars, but also of the planet itself and its neutral atmosphere.

sted, utgiver, år, opplag, sider
2003. Vol. 31, nr 6, s. 1232-1236
Emneord [en]
extraterrestrial plasmas, ionosphere, planetary atmospheres, planets, plasma measurements, phobos observations, solar-wind, bow shock, 1st measurements, magnetic-field, mars, mission, magnetosphere, planet, waves
HSV kategori
Identifikatorer
URN: urn:nbn:se:kth:diva-23180DOI: 10.1109/tps.2003.821353ISI: 000189019500010OAI: oai:DiVA.org:kth-23180DiVA, id: diva2:341878
Merknad
QC 20100525 NR 20140804Tilgjengelig fra: 2010-08-10 Laget: 2010-08-10 Sist oppdatert: 2017-12-12bibliografisk kontrollert

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