Modeling the young Sun's solar wind and its interaction with Earth's paleomagnetosphere-Reference-Cited by-同舟云学术

Modeling the young Sun's solar wind and its interaction with Earth's paleomagnetosphere

Published:2011-01 Issue:A1 Volume:116 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:

Sterenborg M. Glenn¹,Cohen O.²,Drake J. J.²,Gombosi T. I.³

Affiliation:

1. Department of Earth and Planetary Sciences; Harvard University; Cambridge Massachusetts USA

2. Harvard Smithsonian Center for Astrophysics; Cambridge Massachusetts USA

3. Department of Atmospheric, Oceanic, and Space Sciences; University of Michigan; Ann Arbor Michigan 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

Link

http://www.agu.org/journals/ja/ja1101/2010JA016036/2010JA016036.pdf

Reference56 articles.

1. Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates;Arge;J. Geophys. Res.,2000

2. Evolution of the solar ionizing flux;Ayres;J. Geophys. Res.,1997

3. A semiempirical magnetohydrodynamical model of the solar wind;Cohen;Astrophys. J. Lett.,2007

4. Validation of a synoptic solar wind model;Cohen;J. Geophys. Res.,2008

5. Stellar coronal abundances. V. Evidence for the first ionization potential effect in Alpha Centauri;Drake;Astrophys. J.,1997

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