Flare Induced Shocks and Corotating Streams in the Interplanetary Medium-Reference-Cited by-同舟云学术

Flare Induced Shocks and Corotating Streams in the Interplanetary Medium

Published:1972-03 Issue:2 Volume:2 Page:79-82
ISSN:1323-3580
Container-title:Publications of the Astronomical Society of Australia
language:en
Short-container-title:Publ. Astron. Soc. Aust.

Author:

Wiseman M.,Dennison P. A.

Abstract

Geomagnetic storm sudden commencements (ssc) and sudden increases (si) can be caused by either a propagating discontinuity (i.e. a hydromagnetic shock or blast wave) in the interplanetary plasma or by the convection past the Earth of a discontinuity in the ambient solar plasma flow.

Publisher

Cambridge University Press (CUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference11 articles.

1. Morphology of a solar-terrestrial event in March 1966

2. The structure of the solar plasma flow generated by solar flares

3. The transport of flare plasma from the Sun to the Earth

Cited by 13 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. Radio Wave Propagation in the Heliosphere;Physica Scripta;1987-01-01

2. Doppler scintillation observations of interplanetary shocks within 0.3 AU;Journal of Geophysical Research: Space Physics;1985-01-01

3. Observations of shock formation and evolution in the solar atmosphere;Collisionless Shocks in the Heliosphere: Reviews of Current Research;1985

4. Radio-scintillation observations of interplanetary disturbances;Advances in Space Research;1984-01

5. Interplanetary scintillation at large elongation angles: Response to solar wind density structure;Journal of Geophysical Research;1978