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Evidence for a Second Martian Dynamo from Electron Reflection MagnetometryPresent-day Mars does not possess an active core dynamo and associated global magnetic field. However, the discovery of intensely magnetized crust in Mars Southern hemisphere implies that a Martian dynamo has existed in the past. Resolving the history of the Martian core dynamo is important for understanding the evolution of the planet's interior. Moreover, because the global magnetic field provided by an active dynamo can shield the atmosphere from erosion by the solar wind, it may have influenced past Martian climate. Additional information is included in the original extended abstract.
Document ID
20050170997
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
Lillis, R. J.
(California Univ. Berkeley, CA, United States)
Manga, M.
(California Univ. Berkeley, CA, United States)
Mitchell, D. L.
(California Univ. Berkeley, CA, United States)
Lin, R. P.
(California Univ. Berkeley, CA, United States)
Acuna, M. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2005
Publication Information
Publication: Lunar and Planetary Science XXXVI, Part 12
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Public Use Permitted.
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