Determination of shock parameters for the very fast interplanetary shock on 29 October 2003-Reference-Cited by-同舟云学术

Determination of shock parameters for the very fast interplanetary shock on 29 October 2003

Published:2005-09 Issue:A9 Volume:110 Page:
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Terasawa T.¹,Nakata K.¹,Oka M.¹,Saito Y.²,Mukai T.²,Hayakawa H.²,Matsuoka A.²,Tsuruda K.²,Ishisaka K.³,Kasaba K.²,Kojima H.⁴,Matsumoto H.⁴

Affiliation:

1. Department of Earth and Planetary Science; University of Tokyo; Tokyo Japan

2. Institute of Space and Astronautical Science; Japan Aerospace Exploration Agency; Sagamihara Japan

3. Toyama Prefectural University; Toyama Japan

4. Research Institute for Sustainable Humanosphere; Kyoto University; Uji Japan

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

Reference35 articles.

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2. The source region of an interplanetary type II radio burst;Bale;Geophys. Res. Letters,1999

3. Deceleration of the solar wind upstream from the Earth's bow shock and the origin of diffuse upstream ions;Bame;J. Geophys. Res.,1980

4. Backstreaming ions outside the Earth's bow shock and their interaction with the solar wind;Bonifazi;J. Geophys. Res.,1980

5. Deceleration of the solar wind in the Earth foreshock region: ISEE 2 and IMP 8 observations;Bonifazi;J. Geophys. Res.,1980

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