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Автор Williams, D. J.
Автор Lui, A. T. Y.
Автор McEntire, R. W.
Автор Angelopoulos, V.
Автор Jacquey, C.
Автор Christon, S. P.
Автор Frank, L. A.
Автор Ackerson, K. L.
Автор Paterson, W. R.
Автор Kokubun, S.
Автор Yamamoto, T.
Автор Fairfield, D. H.
Дата выпуска 1994
dc.description The GEOTAIL satellite experienced several encounters with the magnetopause during the interval 0300 to 0600 hours on 27 October 1992 at a gsm location of (X,Y,Z) ∼(−81,−8,7.5) R<sub>e</sub>. Energetic ions of both solar wind and ionospheric origin (H<sup>+</sup>, He<sup>++</sup>, and O<sup>+</sup>) were observed streaming in the anti‐solar direction on both the lobe and magnetosheath side of the plasma mantle‐magnetosheath boundary, with maximum fluxes occurring at the boundary. Even though the mantle plasma had penetrated well into the lobe through convective drift, the energetic ions were observed only at the magnetopause and provided a clear signature of the boundary region. Using a measured convective drift velocity and observed energetic particle anisotropies, we estimated that the maximum distance from GEOTAIL that the energetic ions could have been accelerated or made contact with the boundary field lines was <8‐39 R<sub>e</sub>, implying that both solar wind and ionospheric ions are accelerated and contact the magnetopause many tens of earth radii behind the earth. We further found that the unusual magnetopause positions encountered at this time could be explained in part by solar wind aberration effects. However additional processes (e. g., magnetospheric breathing modes, convoluted tail topologies) are required to fully explain these observations.
Формат application.pdf
Копирайт Copyright 1994 by the American Geophysical Union.
Тема Initial Results of Geotail Mission
Тема Initial Results of Geotail Mission
Тема Magnetospheric Physics
Тема Magnetospheric Physics: Magnetospheric configuration and dynamics
Тема Magnetospheric Physics: Magnetotail
Тема Magnetospheric Physics: Magnetotail boundary layers
Название Magnetopause encounters in the magnetotail at distances of ∼80 R<sub>e</sub>
Тип article
DOI 10.1029/94GL01298
Electronic ISSN 1944-8007
Print ISSN 0094-8276
Журнал Geophysical Research Letters
Том 21
Первая страница 3007
Последняя страница 3010
Аффилиация Williams, D. J.; Johns Hopkins University, Applied Physics Laboratory
Аффилиация Lui, A. T. Y.; Johns Hopkins University, Applied Physics Laboratory
Аффилиация McEntire, R. W.; Johns Hopkins University, Applied Physics Laboratory
Аффилиация Angelopoulos, V.; Johns Hopkins University, Applied Physics Laboratory
Аффилиация Jacquey, C.; Johns Hopkins University, Applied Physics Laboratory
Аффилиация Christon, S. P.; University of Maryland
Аффилиация Frank, L. A.; University of Iowa
Аффилиация Ackerson, K. L.; University of Iowa
Аффилиация Paterson, W. R.; University of Iowa
Аффилиация Kokubun, S.; STEL, Nagoya University
Аффилиация Yamamoto, T.; Institute of Space and Astronomical Sciences, Sagimahara
Аффилиация Fairfield, D. H.; NASA, Goddard Space Flight Center
Выпуск 25
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Библиографическая ссылка Fairfield, D. H., Solar wind control of the distant magnetotail: ISEE 3, GSFC LEP Preprint, February 1993
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