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Plasma instabilities near Mars
Swedish Institute of Space Physics / Institutet för rymdfysik.
Luleå University of Technology, Department of Engineering Sciences and Mathematics, Material Science.
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2006 (English)In: Ikke angivet, Committee on Space Research , 2006, p. 2338-Conference paper, Meeting abstract (Other academic)
Abstract [en]

It has been suggested in the literature that the Kelvin-Helmholtz instability can be responsible for significant ion loss at Mars through the detachment of ionospheric plasma clouds Clouds of detached ionospheric plasma were observed at Venus by the Pioneer Venus orbiter The conditions at Mars differ somewhat from those at Venus The ratio between the ion gyro radius and the radius of the planet is larger at Mars than at Venus since Mars is a smaller planet and the solar wind magnetic field is weaker at Mars than at Venus It is therefore interesting to study instabilities at Mars and to compare the results from Mars with those from Venus We search the ion and electron data from the ASPERA-3 instrument on the Mars Express spacecraft for signatures of instabilities at Mars We present data indicative of instabilities in the magnetosheath and the induced magnetosphere boundary downstream of the planet

Place, publisher, year, edition, pages
Committee on Space Research , 2006. p. 2338-
National Category
Other Physics Topics
Research subject
Fysik
Identifiers
URN: urn:nbn:se:ltu:diva-27763Local ID: 14d40190-f18e-11db-bb1b-000ea68e967bOAI: oai:DiVA.org:ltu-27763DiVA, id: diva2:1000952
Conference
COSPAR Scientific Assembly : 16/07/2006 - 23/07/2006
Note
Godkänd; 2006; Bibliografisk uppgift: Meeting abstract from the CDROM, #2338; 20070423 (ysko)Available from: 2016-09-30 Created: 2016-09-30 Last updated: 2017-11-25Bibliographically approved

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Carlsson, Ella

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