Long‐Term Variations in Solar Wind Parameters, Magnetopause Location, and Geomagnetic Activity Over the Last Five Solar Cycles-Reference-Cited by-同舟云学术

Long‐Term Variations in Solar Wind Parameters, Magnetopause Location, and Geomagnetic Activity Over the Last Five Solar Cycles

Published:2019-06 Issue:6 Volume:124 Page:4049-4063
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Samsonov A. A.¹^ORCID,Bogdanova Y. V.²^ORCID,Branduardi‐Raymont G.¹^ORCID,Safrankova J.³^ORCID,Nemecek Z.³^ORCID,Park J.‐S.⁴^ORCID

Affiliation:

1. Mullard Space Science Laboratory University College London London UK

2. RAL Space, STFC Rutherford Appleton Laboratory UK Research and Innovation Oxford UK

3. Faculty of Mathematics and Physics Charles University Prague Czech Republic

4. Shandong Provincial Key Laboratory of Optical Astronomy and Solar‐Terrestrial Environment, Institute of Space Sciences Shandong University Weihai China

Funder

Grantová Agentura České Republiky

Natural Environment Research Council

Central Laser Facility, Science and Technology Facilities Council

UK Space Agency

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2018JA026355

Reference63 articles.

1. The solar wind helium abundance: Variation with wind speed and the solar cycle

2. Differences between CME-driven storms and CIR-driven storms

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5. On the low correlation between long-term averages of solar wind speed and geomagnetic activity after 1976

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