Solar Cycle Variations in the Composition of the Suprathermal Heavy-Ion Population near 1 AU-Reference-Cited by-同舟云学术

Solar Cycle Variations in the Composition of the Suprathermal Heavy-Ion Population near 1 AU

Published:2006-06-27 Issue:1 Volume:645 Page:L81-L84
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Desai M. I.,Mason G. M.,Mazur J. E.,Dwyer J. R.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference31 articles.

1. The suprathermal seed population for corotating interaction region ions at 1 AU deduced from composition and spectra of H+, He++, and He+observed on Wind

2. Cohen, C. M. S., etal 2000, in AIP Conf. Proc. 528, Acceleration and Transport of Energetic Particles Observed in the Heliosphere, ed. R. A. Mewaldt et al. (Melville, NY: AIP), 55

3. Evidence for a Suprathermal Seed Population of Heavy Ions Accelerated by Interplanetary Shocks near 1 AU

4. Acceleration of [TSUP]3[/TSUP]H[CLC]e[/CLC] Nuclei at Interplanetary Shocks

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