Hybrid simulations of solar wind interaction with magnetized asteroids: General characteristics-Reference-Cited by-同舟云学术

Hybrid simulations of solar wind interaction with magnetized asteroids: General characteristics

Published:2002-12 Issue:A12 Volume:107 Page:SSH 12-1-SSH 12-10
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Omidi N.¹²,Blanco-Cano X.³,Russell C. T.⁴,Karimabadi H.¹,Acuna M.⁵

Affiliation:

1. Department of Electrical and Computer Engineering; University of California, San Diego; La Jolla California USA

2. California Space Institute; University of California, San Diego; La Jolla California USA

3. Instituto de Geofisica; Universidad Nacional Autonoma de Mexico; Mexico City Mexico

4. Institute of Geophysics and Planetary Physics; University of California, Los Angeles; Los Angeles California USA

5. NASA Goddard Space Flight Center; Greenbelt Maryland USA

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

Reference14 articles.

1. NEAR magnetic field observations at 433 Eros: First measurements from the surface of an asteroid;Acuna;Icarus,2002

2. Solar wind response to a magnetized asteroid: Linear theory;Baumgartel;Icarus,1997

3. Cyclic behavior at collisionless quasi-parallel shocks;Burgess;Geophys. Res. Lett.,1989

4. Near-Earth asteroid rendezvous: Mission overview;Cheng;J. Geophys. Res.,1997

5. Spectroscopic evidence for undifferentiated S-type asteroids;Feierberg;Astrophysical J.,1982

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