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Magnetically Induced Rotating Rayleigh-Taylor Instability
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Magnetosheath Jet Occurrence Rate in Relation to CMEs and SIRs

Florian Koller1, Manuela Temmer1, Luis Preisser2

  • 1Institute of Physics University of Graz Graz Austria.

Journal of Geophysical Research. Space Physics
|July 22, 2022
PubMed
Summary

Magnetosheath jets, crucial for solar wind-magnetosphere coupling, decrease during coronal mass ejections (CMEs) but increase with high-speed streams (HSSs). This study analyzes jet production during these solar wind events.

Keywords:
CMEHSSMagnetosheath JetsSIR

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