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Detailed Reference Information |
Mihalov, J.D. and Gazis, P.R. (1998). Interstellar pickup hydrogen observations at large heliocentric distances. Geophysical Research Letters 25: doi: 10.1029/97GL03785. issn: 0094-8276. |
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Possible signatures of interstellar pickup hydrogen have been identified in data from the Pioneer 10 and 11 Ames plasma analyzers at locations out to beyond the orbit of Saturn, and at a wide range of longitudes in the heliosphere, both upstream and downstream in the interstellar wind. These signatures provide an extension of pickup ion observations out to beyond 15 AU heliocentric distance, including near where the maximum pickup hydrogen flux is expected. A depletion of interstellar pickup hydrogen downstream from the Sun in the interstellar flow may be indicated. These signatures are consistent with Ulysses pickup ion measurements. ¿ 1998 American Geophysical Union |
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BACKGROUND DATA FILES |
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Abstract |
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Keywords
Interplanetary Physics, Pickup ions, Interplanetary Physics, Interstellar gas, Space Plasma Physics, Charged particle motion and acceleration, Space Plasma Physics, Instruments and techniques |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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