Acceleration of the solar wind as a result of the reconnection of open magnetic flux with coronal loops-Reference-Cited by-同舟云学术

Acceleration of the solar wind as a result of the reconnection of open magnetic flux with coronal loops

Published:2003 Issue:A4 Volume:108 Page:
ISSN:0148-0227
Container-title:Journal of Geophysical Research
language:en
Short-container-title:J. Geophys. Res.

Author:

Fisk L. A.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

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4. Reducing heliospheric magnetic flux from coronal mass ejections without disconnection;Crooker;J. Geophys. Res.,2002

5. Morphology of the quiet solar upper atmosphere in the 4 · 104 < Te < 1 · 4 · 106 K temperature regime;Feldman;Astrophys. J.,1999

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