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Early time interaction of lithium ions with the solar wind in the AMPTE missionThe early time interaction of an artifically injected lithium cloud with the solar wind is simulated with a one-dimensional hybrid code. Simulation results indicate that the lithium cloud presents an obstacle to the solar wind flow, forming a shock-like interaction region. Several notable features are found: (1) The magnetic field is enhanced up to a factor of about 6, followed by a magnetic cavity downstream. (2) Solar wind ions are slowed down inside the lithium cloud, with substantial upstream reflection. (3) Most of the lithium ions gradually pick up the velocity of the solar wind and move downstream. (4) Intense and short-wavelength electric fields exist ahead of the interaction region. (5) Strong electron heating occurs within the lithium cloud. (6) The convection electric field in the solar wind is modulated in the interaction region. The simulation results are in remarkable agreement with in situ spacecraft measurements made during lithium releases in the solar wind by the AMPTE (Active Magnetospheric Particle Tracer Explorers) Program.
Document ID
19860040945
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lui, A. T. Y.
(Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States)
Goodrich, C. C.
(Johns Hopkins Univ. Laurel, MD, United States)
Papadopoulos, K.
(Maryland, University College Park, United States)
Mankofsky, A.
(Science Applications International Corp. McLean, VA, United States)
Date Acquired
August 12, 2013
Publication Date
February 1, 1986
Publication Information
Publication: Journal of Geophysical Research
Volume: 91
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
86A25683
Funding Number(s)
CONTRACT_GRANT: NSF INT-83-04379
CONTRACT_GRANT: N00024-83-C-8301
CONTRACT_GRANT: NAGW-81
Distribution Limits
Public
Copyright
Other

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