CESE-HLL Magnetic Field-Driven Modeling of the Background Solar Wind During Year 2008-Reference-Cited by-同舟云学术

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CESE-HLL Magnetic Field-Driven Modeling of the Background Solar Wind During Year 2008

Published:2018-06 Issue:6 Volume:123 Page:4488-4509
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Li Huichao¹²^ORCID,Feng Xueshang¹²³^ORCID

Affiliation:

1. SIGMA Weather Group, 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. HIT Institute of Space Science and Applied Technology; Shenzhen China

Funder

National Natural Science Foundation of China

Specialized Research Fund for State Key Laboratories

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/2017JA025125/fullpdf

Reference97 articles.

1. Coronal pseudo-streamer and bipolar streamer observed by SOHO/UVCS in March 2008;Abbo;Solar Physics,2015

2. Low-latitude coronal holes at the minimum of the 23rd solar cycle;Abramenko;Astrophysical Journal,2010

3. Radial evolution of the three-dimensional structure in CIRs between Earth and Ulysses;Broiles;Journal of Geophysical Research: Space Physics,2013

4. Ensemble modeling of the 23 July 2012 coronal mass ejection;Cash;Space Weather,2015

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4. A New Numerical Implementation for Solar Coronal Modeling by an HLL Generalized Riemann Problem Solver;The Astrophysical Journal Supplement Series;2023-01-01

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