Motion of the heliospheric termination shock:, 2. Energy loss due to energetic particle acceleration-Reference-Cited by-同舟云学术

Motion of the heliospheric termination shock:, 2. Energy loss due to energetic particle acceleration

Published:1994 Issue:A4 Volume:99 Page:6553
ISSN:0148-0227
Container-title:Journal of Geophysical Research
language:en
Short-container-title:J. Geophys. Res.

Author:

Barnes Aaron

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Link

http://www.agu.org/journals/ja/v099/iA04/94JA00262/94JA00262.pdf

Reference20 articles.

1. The structure of cosmic ray shocks;Axford;Astron. Astrophys.,1982

2. Motion of the heliospheric termination shock: A gasdynamic model;Barnes;J. Geophys. Res.,1993

3. Prospects for detection of the heliospheric terminal shock: ARC plasma analyzer aboard Pioneer 10;Barnes;Eos, Trans. AGU,1991

4. Solar wind conditions in the outer heliosphere and the distance to the termination shock;Belcher;J. Geophys. Res.,1993

5. The steady-state and dynamical structure of a cosmic-ray-modified termination shock;Donohue;J. Geophys. Res.,1993

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