Modeling solar energetic particle transport in 3D background solar wind: Influences of the compression regions
Authors:
- Wenwen WeiWWWenwen Wei
- Fang ShenFang Shen
- Zicai YangZYZicai Yang
- Lulu ZhaoLZLulu Zhao
- Yang WangYWYang Wang
- Pingbing ZuoPZPingbing Zuo
- Jie ZhangJZJie Zhang
- 1 January 2019
- journal article
- research article
- Published by Elsevier in Journal of Atmospheric and Solar-Terrestrial Physics
- Vol. 182, 155-164
Abstract
No abstract availableKeywords
Funding Information
- National Natural Science Foundation of China (41374188, 41474152, 41231068, 41531073, 41774184)
- Specialized Research Fund
- National Program
This publication has 49 references indexed in Scilit:
- SHOCK CONNECTIVITY IN THE 2010 AUGUST AND 2012 JULY SOLAR ENERGETIC PARTICLE EVENTS INFERRED FROM OBSERVATIONS AND ENLIL MODELINGThe Astrophysical Journal, 2016
- A NEW THREE-DIMENSIONAL SOLAR WIND MODEL IN SPHERICAL COORDINATES WITH A SIX-COMPONENT GRIDThe Astrophysical Journal Supplement Series, 2014
- SIP-CESE MHD model of solar wind with adaptive mesh refinement of hexahedral meshesComputer Physics Communications, 2014
- THREE-DIMENSIONAL SOLARWINDMODELING FROM THE SUN TO EARTH BY A SIP-CESE MHD MODEL WITH A SIX-COMPONENT GRIDThe Astrophysical Journal, 2010
- A Class of TVD Type Combined Numerical Scheme for MHD Equations With a Survey About Numerical Methods in Solar Wind SimulationsSpace Science Reviews, 2003
- Particle Acceleration in Solar Wind Compression RegionsThe Astrophysical Journal, 2002
- Proton and electron mean free paths: The Palmer consensus revisitedThe Astrophysical Journal, 1994
- Shock acceleration of energetic particles in corotating interaction regions in the solar windThe Astrophysical Journal, 1980
- The diffusive idealization of charged-particle transport in random magnetic fieldsThe Astrophysical Journal, 1974
- Continual Acceleration of Solar Protons in the MeV RangePhysical Review Letters, 1965