Solar wind‐magnetosphere coupling efficiency during ejecta and sheath‐driven geomagnetic storms-Reference-Cited by-同舟云学术

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Solar wind‐magnetosphere coupling efficiency during ejecta and sheath‐driven geomagnetic storms

Published:2016-05 Issue:5 Volume:121 Page:4378-4396
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Myllys M.¹,Kilpua E. K. J.¹,Lavraud B.²³,Pulkkinen T. I.⁴^ORCID

Affiliation:

1. Department of Physics University of Helsinki Helsinki Finland

2. Institut de Recherche en Astrophysique et Plantologie Toulouse France

3. Centre National de la Recherche Scientifique Toulouse France

4. Aalto University School of Electrical Engineering Aalto Finland

Funder

Suomen Akatemia

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016JA022407

Reference62 articles.

1. Energy coupling between the solar wind and the magnetosphere

2. Magnetospheric impulse response for many levels of geomagnetic activity

3. The rudiments of a theory of solar wind/magnetosphere coupling derived from first principles

4. Role of solar wind turbulence in the coupling of the solar wind to the Earth's magnetosphere

5. Polar cap potential saturation, dayside reconnection, and changes to the magnetosphere

Cited by 28 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Solar Wind‐Magnetosphere Coupling Efficiency and Its Dependence on Solar Activity During Geomagnetic Storms of 23–24 Solar Cycles;Journal of Geophysical Research: Space Physics;2024-08

2. Planar Magnetic Structures Downstream of Coronal Mass Ejection–driven Shocks in the Inner Heliosphere;The Astrophysical Journal;2023-07-01

3. Solar events and solar wind conditions associated with intense geomagnetic storms;Earth, Planets and Space;2023-05-23

4. Dependence of radiation belt flux depletions at geostationary orbit on different solar drivers during intense geomagnetic storms;Frontiers in Astronomy and Space Sciences;2022-10-21

5. Solar wind magnetosonic mach number as a control variable for energy dissipation during magnetic storms;Frontiers in Astronomy and Space Sciences;2022-09-30

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