Radiation belt electron precipitation due to geomagnetic storms: Significance to middle atmosphere ozone chemistry
International audience [1] Geomagnetic storms triggered by coronal mass ejections and high‐speed solar wind streams can lead to enhanced losses of energetic electrons from the radiation belts into the atmosphere, both during the storm itself and also through the poststorm relaxation of enhanced radi...
Published in: | Journal of Geophysical Research: Space Physics |
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Main Authors: | , , , , , , , |
Other Authors: | , , , , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
HAL CCSD
2010
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Subjects: | |
Online Access: | https://hal-insu.archives-ouvertes.fr/insu-01254033 https://hal-insu.archives-ouvertes.fr/insu-01254033/document https://hal-insu.archives-ouvertes.fr/insu-01254033/file/jgra20708.pdf https://doi.org/10.1029/2010JA015599 |