Fluid versus simulation model of solitons in solar wind: Application to Ulysses observations-Reference-Cited by-同舟云学术

Fluid versus simulation model of solitons in solar wind: Application to Ulysses observations

Published:2007-12 Issue:A12 Volume:112 Page:n/a-n/a
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Baumgärtel K.¹,Sauer K.²,Mjølhus E.³,Dubinin E.⁴

Affiliation:

1. Astrophysikalisches Institut Potsdam; Potsdam Germany

2. Department of Physics; University of Alberta; Edmonton, Alberta Canada

3. Department of Mathematics and Statistics; University of Tromsø; Tromsø Norway

4. Max Planck Institute for Solar System Research; Katlenburg-Lindau Germany

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

Reference25 articles.

1. Large-amplitude hydromagnetic waves;Barnes;J. Geophys. Res.,1974

2. Soliton approach to magnetic holes;Baumgärtel;J. Geophys. Res.,1999

3. Solar wind magnetic holes: Signatures of slow-mode type MHD solitons;Baumgärtel;Adv. Space Res.,1997

4. Towards understanding magnetic holes: Hybrid simulations;Baumgärtel;Geophys. Res. Lett.,2003

5. Kinetic slow-mode type solitons;Baumgärtel;Nonlin. Proc. Geophys.,2005

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