Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions-Reference-Cited by-同舟云学术

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Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions

Published:2022-05 Issue:5 Volume:297 Page:
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Zheng Ruisheng^ORCID,Zhang Liang^ORCID,Rao Changhui,Wang Bing,Chen Huadong^ORCID,Zhong Libo,Chen Yao^ORCID

Funder

NSFC

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://link.springer.com/content/pdf/10.1007/s11207-022-01969-8.pdf

Reference52 articles.

1. Antiochos, S.K., DeVore, C.R., Klimchuk, J.A.: 1999, A model for solar coronal mass ejections. Astrophys. J. 510, 485. DOI. ADS.

2. Bateman, G.: 1978, MHD Instabilities, MIT Press, Cambridge. ADS.

3. Chae, J., Wang, H., Qiu, J., Goode, P.R., Strous, L., Yun, H.S.: 2001, The formation of a prominence in active region NOAA 8668. I. SOHO/MDI observations of magnetic field evolution. Astrophys. J. 560, 476. DOI. ADS.

4. Chen, P.F.: 2011, Coronal mass ejections: models and their observational basis. Liv. Rev. Solar Phys. 8, 1. DOI. ADS.

5. Chen, P.F., Shibata, K.: 2000, An emerging flux trigger mechanism for coronal mass ejections. Astrophys. J. 545, 524. DOI. ADS.

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