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Martian bow shock - Phobos observationsData obtained with the Magma magnetometer on the subsolar passes of the Phobos spacecraft during its 3 elliptic orbits reveals a turbulent bow shock with a strong foot consistent with the reflection of solar wind protons. The bow shock lies at a subsolar distance of 1.47 + or - .03 R(M). The circular orbit phase of the mission reveals a bow shock with a highly varying location. The median terminator crossing lies at 2.72 Mars radii. The location of the bow shock in the terminator plane is sensitive to neither the EUV flux nor to planetary longitude.
Document ID
19900047793
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Schwingenschuh, K.
(Institut fuer Weltraumforschung Graz, Austria)
Riedler, W.
(Institut fuer Weltraumforschung Graz, Austria)
Lichtenegger, H.
(Oesterreichische Akademie der Wissenschaften Institut fuer Weltraumforschung, Graz, Austria)
Eroshenko, E.
(IZMIRAN Troitsk, Ussr)
Sauer, K.
(AdW der DDR Institut fuer Kosmosforschung, Berlin, German Democratic Republic)
Date Acquired
August 14, 2013
Publication Date
May 1, 1990
Publication Information
Publication: Geophysical Research Letters
Volume: 17
ISSN: 0094-8276
Subject Category
Lunar And Planetary Exploration
Accession Number
90A34848
Funding Number(s)
CONTRACT_GRANT: NAGW-1753
Distribution Limits
Public
Copyright
Other

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