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Comet Halley-solar wind interaction from electron measurements aboard GiottoThe Giotto probe's three-dimensional electron spectrometer has obtained data that illustrate the complex interactions between comet Halley and the solar wind. As Giotto approached the comet, it traversed several regions exhibiting different plasma characteristics: a large upstream region, a foreshock, a bow wave whose apex lies at about 400,000 km, a transition region, a region permanently and strongly contaminated by cometary ions, a collision pause, and various inner regions up to the inner coma, including a region of depleted hot plasma.
Document ID
19860056174
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Reme, H.
(Centre d'Etude Spatiale des Rayonnements Toulouse, France)
Sauvaud, J. A.
(Centre d'Etude Spatiale des Rayonnements Toulouse, France)
Duston, C.
(Centre d'Etude Spatiale des Rayonnements Toulouse, France)
Cotin, F.
(Centre d'Etude Spatiale des Rayonnements Toulouse, France)
Cros, A.
(CNRS Centre d'Etude Spatiale des Rayonnements, Toulouse, France)
Date Acquired
August 12, 2013
Publication Date
May 15, 1986
Publication Information
Publication: Nature
Volume: 321
ISSN: 0028-0836
Subject Category
Astrophysics
Accession Number
86A40912
Funding Number(s)
CONTRACT_GRANT: CNES-1212
CONTRACT_GRANT: BMFT-01-OF-052
CONTRACT_GRANT: NASW-3575
Distribution Limits
Public
Copyright
Other

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