A STEADY-STATE PICTURE OF SOLAR WIND ACCELERATION AND CHARGE STATE COMPOSITION DERIVED FROM A GLOBAL WAVE-DRIVEN MHD MODEL
The higher charge states found in slow (<400 km s[superscript −1]) solar wind streams compared to fast streams have supported the hypothesis that the slow wind originates in closed coronal loops and is released intermittently through reconnection. Here we examine whether a highly ionized slow win...
Main Authors: | Landi, E. (Author), Holst, B. van der (Author), Lepri, Susan T. (Author), Nuevo, F. A. (Author), Frazin, R. (Author), Manchester, W. (Author), Sokolov, I. (Author), Gombosi, T. I. (Author), Oran, Rona (Contributor), Vasquez, A. M. (Author) |
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Other Authors: | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor) |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2015-09-03T16:49:21Z.
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Subjects: | |
Online Access: | Get fulltext |
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