Solar wind magnetosonic mach number as a control variable for energy dissipation during magnetic storms
During the main phase of many magnetic storms the solar wind Mach number is low and IMF magnitude is large. Under these conditions, the ionospheric potential saturates, and it becomes relatively insensitive to further increases in the IMF magnitude. On the other hand, the dayside merging rate and th...
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| Hlavní autoři: | , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
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Frontiers Media S.A.
2022-09-01
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| Edice: | Frontiers in Astronomy and Space Sciences |
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| On-line přístup: | https://www.frontiersin.org/articles/10.3389/fspas.2022.960535/full |
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