Double‐peaked core field of flux ropes during magnetic reconnection-Reference-Cited by-同舟云学术

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Double‐peaked core field of flux ropes during magnetic reconnection

Published:2017-06 Issue:6 Volume:122 Page:6374-6384
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Liu Chaoxu¹,Feng Xueshang¹^ORCID,Nakamura Rumi²^ORCID,Guo Jianpeng¹³,Wang Rongsheng⁴^ORCID

Affiliation:

1. State Key Laboratory of Space Weather, National Space Science CenterChinese Academy of Sciences Beijing China

2. Space Research InstituteAustrian Academy of Sciences Graz Austria

3. Planetary and Space Physics Group, Department of AstronomyBeijing Normal University Beijing China

4. Key Laboratory of Geospace Environment, Department of Geophysics and Planetary ScienceUniversity of Science and Technology of China Hefei China

Funder

National Natural Science Foundation of China

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2017JA024233

Reference56 articles.

1. Substorm topology in the ionosphere and magnetosphere during a flux rope event in the magnetotail

2. Evolution of the thin current sheet in a substorm observed by Geotail

3. The Cluster Magnetic Field Investigation: overview of in-flight performance and initial results

4. Observations of magnetic flux ropes during magnetic reconnection in the Earth's magnetotail

5. Observation of energetic electrons within magnetic islands

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1. Cosmic ray origin: Why cosmic ray (Astroparticle) phenomenon is universal in the Universe? What is the main driver of cosmic ray particle generation?;Advances in Space Research;2019-12

2. Dynamic patterns of self-organization inflow in collisionless magnetic reconnection;Astrophysics and Space Science;2019-08

3. Interplanetary Physics in Mainland China;Chinese Journal of Space Science;2018

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