Modeling proton intensity gradients and radiation dose equivalents in the inner heliosphere using EMMREM: May 2003 solar events

Author:

Dayeh M. A.1,Desai M. I.12,Kozarev K.3,Schwadron N. A.4,Townsend L. W.5,PourArsalan M.5,Zeitlin C.6,Hatcher R. B.5

Affiliation:

1. Space Science and Engineering Division; Southwest Research Institute; San Antonio Texas USA

2. Department of Physics and Astronomy; University of Texas at San Antonio; San Antonio Texas USA

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

4. Institute for the Study of Earth, Oceans, and Space; University of New Hampshire; Durham New Hampshire USA

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

6. Space Studies Department; Southwest Research Institute; Boulder Colorado USA

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Reference63 articles.

1. A first step towards proton flux forecasting;Aran;Adv. Space Res.,2005

2. Fluxes and fluences of SEP events derived from SOLPENCO;Aran;Ann. Geophys.,2005

3. The magnetic field investigation on the ULYSSES mission-Instrumentation and preliminary scientific results;Balogh;Astron. Astrophys. Suppl. Ser.,1992

4. THE ULYSSES SOLAR WIND PLASMA INVESTIGATION: EXPERIMENT DESCRIPTION AND INITIAL IN-ECLIPTIC RESULTS

5. Three-dimensional interplanetary stream magnetism and energetic particle motion;Barouch;J. Geophys. Res.,1976

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