The Distributions of Iron Average Charge States in Small Flux Ropes in Interplanetary Space: Clues to Their Twisted Structures

Author:

Huang Jia1ORCID,Liu Yong C.-M.1ORCID,Peng Jun12ORCID,Qi Zhaohui12,Li Hui1ORCID,Klecker Berndt3ORCID,Song Hongqiang4,Zheng Jinlei5,Hu Qiang5ORCID

Affiliation:

1. State Key Laboratory of Space Weather, National Space Science Center; Chinese Academy of Sciences; Beijing China

2. College of Earth Sciences; University of Chinese Academy of Sciences; Beijing China

3. Max-Planck-Institut für Extraterrestrische Physik; Garching Germany

4. Institute of Space Sciences; Shandong University; Weihai China

5. Department of Space Science and CSPAR; University of Alabama in Huntsville; Huntsville AL USA

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference68 articles.

1. Slow solar wind: Observations and modeling;Abbo;Space Science Reviews,2016

2. Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP 8 observations;Burlaga;Journal of Geophysical Research,1981

3. Comparison of small-scale flux rope magnetic properties to large-scale magnetic clouds: Evidence for reconnection across the HCS?;Cartwright;Journal of Geophysical Research,2008

4. Intrinsic instability of coronal streamers;Chen;Astronomy Journal,1936

5. On the prevalence of small-scale twist in the solar chromosphere and transition region;De Pontieu;Science,2014

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