On the identification of time interval threshold in the twin-CME scenario-Reference-Cited by-同舟云学术

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On the identification of time interval threshold in the twin-CME scenario

Published:2014-03 Issue:3 Volume:119 Page:1463-1475
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Ding Liu-Guan¹,Li Gang²,Dong Li-Hua³,Jiang Yong⁴,Jian Yi⁴,Gu Bin¹

Affiliation:

1. School of Physics and Optoelectronic Engineering; Nanjing University of Information Science and Technology; Nanjing China

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

3. School of Media Technology; Communication University of China Nanjing; Nanjing China

4. College of Math and Statistics; Nanjing University of Information Science and Technology; Nanjing China

Funder

UAH by NSF

NUIST by NSFC

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2013JA019745/fullpdf

Reference23 articles.

1. Classes of sloar energetic particle events associated with impulsive and long-duration soft X-ray flares;Cane;Astrophys. J.,1986

2. The “twin-CME” scenario and large solar energetic particle events in solar cycle 23;Ding;Astrophys. J.,2013

3. Alfven profile in the lower corona: Implication for shock formation;Evans;Astrophys. J.,2008

4. Intensity variation of large solar energetic particle events associated with coronal mass ejections;Gopalswamy;J. Geophys. Res.,2004

5. Coronal mass ejections and solar energetic particle events;Kahler;AIP Conference Proceedings,1996

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