Modeling the 2003 Halloween events with EMMREM: Energetic particles, radial gradients, and coupling to MHD

Author:

Kozarev K.1,Schwadron N. A.1,Dayeh M. A.2,Townsend L. W.3,Desai M. I.2,PourArsalan M.3

Affiliation:

1. Department of Astronomy; Boston University; Boston Massachusetts USA

2. Southwest Research Institute; San Antonio Texas USA

3. Department of Nuclear Engineering; University of Tennessee; Knoxville Tennessee USA

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Reference44 articles.

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2. Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates;Arge;J. Geophys. Res.,2000

3. Space environment of Mercury at the time of the first MESSENGER flyby: Solar wind and interplanetary magnetic field modeling of upstream conditions;Baker;J. Geophys. Res.,2009

4. The magnetic field investigation on the Ulysses mission: Instrumentation and preliminary scientific results;Balogh;Astron. Astrophys. Suppl. Ser.,1992

5. The Ulysses solar wind plasma experiment;Bame;Astron. Astrophys. Suppl. Ser.,1992

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