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Field dipolarization in Saturn's magnetotail with planetward ion flows and energetic particle flow bursts: Evidence of quasi‐steady reconnection
External Source
chorus
Document Type
Version of Record
Authors
C. M. Jackman (School of Physics and Astronomy University of Southampton Southampton UK)
M. F. Thomsen (Planetary Science Institute Tucson Arizona USA)
D. G. Mitchell (The Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA)
N. Sergis (Academy of Athens Athens Greece)
C. S. Arridge (Department of Physics Lancaster University Bailrigg UK)
M. Felici (Department of Physics Lancaster University Bailrigg UK)
S. V. Badman (Department of Physics Lancaster University Bailrigg UK)
C. Paranicas (The Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA)
X. Jia (Atmospheric, Oceanic and Space Sciences University of Michigan Ann Arbor Michigan USA)
G. B. Hospodarksy (Department of Physics and Astronomy University of Iowa Iowa City Iowa USA)
M. Andriopoulou (Space Research Institute Austrian Academy of Sciences Graz Austria)
K. K. Khurana (Institute of Geophysics and Planetary Physics University of California Los Angeles California USA)
A. W. Smith (School of Physics and Astronomy University of Southampton Southampton UK)
M. K. Dougherty (Blackett Laboratory Imperial College London London UK)
Date Acquired
February 10, 2024
Publication Date
May 19, 2015
Publication Information
Publication: Journal of Geophysical Research: Space Physics
Publisher: American Geophysical Union (AGU)
Volume: 120
Issue: 5
Issue Publication Date: May 1, 2015
ISSN: 2169-9380
e-ISSN: 2169-9402
DOI: 10.1002/2015ja020995
Funding Number(s)
funding: 1243218
Distribution Limits
Public
Keywords
space and planetary science
geophysics

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