Drift Shell Tracing and Secular Variation of Inner Radiation Environment in the SAA Region-Reference-Cited by-同舟云学术

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Drift Shell Tracing and Secular Variation of Inner Radiation Environment in the SAA Region

Published:2002 Issue: Volume: Page:353-358
ISSN:0964-2749
Container-title:Solar-terrestrial Magnetic Activity and Space Environment - Proceedings of the COSPAR Colloquium on Solar-Terrestrial Magnetic Activity and Space Environment (STMASE) held in the NA OC in Beijing, China September 10-12, 2001
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Author:

Pu Z.Y.,Xie L.,Fang X.H.,Jiao W.X.,Fu S.Y.,Zong Q.G.

Publisher

Elsevier

Reference19 articles.

1. Proton Induced Upsets in the Low Altitude Polar Orbit;Adams;IEEE Trans. Nucl. Sci. N-S36,1989

2. Geomagnetic models from satellite surveys;Cain;Rev. Geophys. Space Phys.,1971

3. Effects of the recular magnetic variation on the distribution function of inner-zone protons;Farley;J. Geophys. Res.,1972

4. Recent development in the NASA trapped radiation models;Fung,1996

5. Response of trapped particles to a collapsing dipole moment;Heckman;J. Geophys. Res.,1972

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1. Geomagnetic secular variation consequences on the trajectories of radiation belt trapped particles;Astrophysics and Space Science;2022-06

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