Development of the 3-D MHD model of the solar corona-solar wind combining system

Author:

Nakamizo A.123,Tanaka T.13,Kubo Y.23,Kamei S.34,Shimazu H.23,Shinagawa H.23

Affiliation:

1. Department of Earth and Planetary Sciences, Faculty of Sciences; Kyushu University; Fukuoka Japan

2. National Institute of Information and Communications Technology; Tokyo Japan

3. Core Research for Evolutional Science and Technology; Japan Science and Technology Agency; Saitama Japan

4. Department of Earth and Planetary Sciences, Graduated School of Sciences; Kyushu University; Fukuoka 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

Reference49 articles.

1. Solar wind acceleration caused by gradient of Alfvén wave pressure;Alazraki;Astron. Astrophys.,1971

2. Magnetic fields and structure of solar corona: I. Methods of calculating coronal fields;Altschuler;Sol. Phys.,1969

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

4. Acceleration of the solar wind;Barnes;Rev. Geophys.,1992

5. Constraints on solar wind acceleration mechanisms from Ulysses plasma observations: The first polar pass;Barnes;Geophys. Res. Lett.,1995

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