Parametric study of interaction effects of fast and slow co-rotating solar wind streams-Reference-Cited by-同舟云学术

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Parametric study of interaction effects of fast and slow co-rotating solar wind streams

Published:1994-01 Issue:1 Volume:42 Page:27-40
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Rudenko G.V.,Fainshtein V.G.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference41 articles.

1. Energy coupling between the solar wind and the magnetosphere;Akasofu;Space Sci. Rev.,1981

2. Solar wind helium and hydrogen structure near the heliosphcric current sheet: a signal of coronal streamers at 1 AU;Borrini;J. geophys. Rev.,1981

3. Corotating structure in the solar wind;Carovillano;Solar Phys.,1969

4. Corona and solar wind in a quasi-dipole magnetic field;Chashei;Astronomichesky zhurnal,1992

5. Solar-wind properties at the Earth as predicted by one-fluid models;Durney;J. geophys. Rev.,1972

Cited by 1 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. Coronal Field Geometry and Solar Wind Speed;Universe;2022-12-05

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