Development of the 3-D MHD model of the solar corona-solar wind combining system-Reference-Cited by-同舟云学术

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

Published:2009-07 Issue:A7 Volume:114 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:

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

Cited by 98 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Machine Learning‐Based Emulator for the Physics‐Based Simulation of Auroral Current System;Space Weather;2024-01

2. Time-dependent boundary conditions for electric-field-driven global coronal simulations;CHINESE J GEOPHYS-CH;2023

3. A mutually embedded perception model for solar corona;Monthly Notices of the Royal Astronomical Society;2023-05-19

4. The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 2003;Solar Physics;2023-05

5. Numerical modeling of solar wind and coronal mass ejection in the inner heliosphere: A review;Frontiers in Astronomy and Space Sciences;2023-03-16