Energetic protons associated with a forward-reverse interplanetary shock pair at 1 A.U.

Author:

Balogh A.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference30 articles.

1. Low energy proton measurements in interplanetary space on board the HEOS-1 satellite;Balogh,1970

2. Evidence for interplanetary acceleration of nucleons in corotating interaction regions;Barnes;Astrophys. J. Lett.,1976

3. Large amplitude Alfvén waves in the interplanetary medium, 2;Belcher;J. geophys. Res.,1971

4. Interplanetary stream interfaces;Burlaga;J. geophys. Res.,1974

5. Energy transfer at colliding streams in the solar wind;Burlaga;Astrophys. J.,1971

Cited by 4 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. On one mechanism for the generation of a reverse solar wind shock in the magnetosheath in front of the Earth’s magnetosphere;Astronomy Letters;2011-11-26

2. On the origin of the MeV energy nucleon flux associated with CIRs;Journal of Geophysical Research;1981

3. Propagation of solar particles in the interplanetary medium;Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences;1980-07-29

4. Acceleration of particles by shocks in a cosmic plasma;Space Science Reviews;1980-06

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