[Comment on “Explosive magnetic reconnection: Puzzle to be solved as the energy supply process for magnetospheric substorms?” by Syun-Ichi Akasofu] Explosive magnetic reconnection in solar flares and type III bursts-Reference-Cited by-同舟云学术

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[Comment on “Explosive magnetic reconnection: Puzzle to be solved as the energy supply process for magnetospheric substorms?” by Syun-Ichi Akasofu] Explosive magnetic reconnection in solar flares and type III bursts

Published:1985 Issue:32 Volume:66 Page:581
ISSN:0096-3941
Container-title:Eos, Transactions American Geophysical Union
language:en
Short-container-title:Eos Trans. AGU

Author:

Chubb Talbot A.

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences

Reference10 articles.

1. Explosive magnetic reconnection: Puzzle to be solved as the energy supply process for magnetospheric substorms?;Akasofu;Eos Trans. AGU,1985

2. Currents in the solar atmosphere and a theory of solar flares;Alfvén;Solar Phys.,1967

3. ATM observations on the XUV emission from solar flares;Brueckner;Philos. Trans. R. Soc. London Ser. A,1976

4. Observations of a kink instability in a solar flare;Cheng;Astrophys. J.,1977

5. A phenomenological model of solar flares;Colgate;Astrophys. J.,1978

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. ULF geomagnetic power at cusp latitudes in response to upstream solar wind conditions;Journal of Geophysical Research;1987

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