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Ring current development during high speed streams
Authors:V.K. Jordanova  H. Matsui  P.A. Puhl-Quinn  M.F. Thomsen  K. Mursula  L. Holappa
Affiliation:1. Los Alamos National Laboratory, Los Alamos, NM 87545, USA;2. Space Science Center, University of New Hamsphire, Durham, NH 03824, USA;3. Department of Physical Sciences, University of Oulu, Oulu, Finland;1. Department of Physics, P.O. Box 64, University of Helsinki, Finland;2. Space Sciences Laboratory, University of California, Berkeley, CA, USA;3. Department of Astronomy, University of Maryland, College Park, MD, USA;4. Heliophysics Science Division, NASA/Goddard Space Flight Center, Greenbelt, MD, USA;5. Institute of Geophysics and Planetary Physics, UCLA, Los Angeles, CA, USA;1. Department of Space Physics, School of Electronic Information, Wuhan University, Wuhan, Hubei, China;2. State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China;1. Space Science & Applications, Los Alamos National Laboratory, Los Alamos, NM, USA;2. New Mexico Consortium, Los Alamos, NM, USA;1. Department of Space Physics, School of Electronic Information, Wuhan University, Wuhan, Hubei, China;2. Department of Earth, Planetary and Space Sciences, University of California, Los Angeles, CA, USA;3. Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, CA, USA
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