Modeling the East‐West Asymmetry of Energetic Particle Fluence in Large Solar Energetic Particle Events Using the iPATH Model-Reference-Cited by-同舟云学术

Modeling the East‐West Asymmetry of Energetic Particle Fluence in Large Solar Energetic Particle Events Using the iPATH Model

Published:2022-06 Issue:6 Volume:127 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:JGR Space Physics

Author:

Ding Zheyi¹^ORCID,Li Gang²^ORCID,Ebert Robert W.³⁴^ORCID,Dayeh Maher A.³⁴^ORCID,Fe‐Dueñas Adolfo Santa³⁴,Desai Mihir³⁴,Xie Hong⁵^ORCID,Gopalswamy N.⁵^ORCID,Bruno A.⁵⁶^ORCID

Affiliation:

1. KU Leuven Leuven Belgium

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

3. Southwest Research Institute San Antonio TX USA

4. Department of Physics and Astronomy University of Texas at San Antonio San Antonio TX USA

5. Heliophysics Division NASA Goddard Space Flight Center Greenbelt MD USA

6. Department of Physics Catholic University of America Washington DC WA USA

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2022JA030343

Reference41 articles.

1. Empirical Model of 10 – 130 MeV Solar Energetic Particle Spectra at 1 AU Based on Coronal Mass Ejection Speed and Direction

2. The role of interplanetary shocks in the longitude distribution of solar energetic particles

3. A Consistent Method of Characteristics for Multidimensional Magnetohydrodynamics

4. Characteristics of Solar Energetic Ions as a Function of Longitude

5. Comparing Long-duration Gamma-Ray Flares and High-energy Solar Energetic Particles

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