Modeling proton intensity gradients and radiation dose equivalents in the inner heliosphere using EMMREM: May 2003 solar events-Reference-Cited by-同舟云学术

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

Published:2010-11 Issue:11 Volume:8 Page:n/a-n/a
ISSN:1542-7390
Container-title:Space Weather
language:en
Short-container-title:Space Weather

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

Link

http://www.agu.org/journals/sw/sw1011/2009SW000566/2009SW000566.pdf

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

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