Solar proton intensity structures in the magnetosphere during interplanetary anisotropies-Reference-Cited by-同舟云学术

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Solar proton intensity structures in the magnetosphere during interplanetary anisotropies

Published:1972-12 Issue:12 Volume:20 Page:2113-2123
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Morfill G.,Scholer M.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference23 articles.

1. Tail of the magnetosphere;Axford;J. geophys. Res.,1965

2. Transport characteristics of low energy solar cosmic rays;Balogh,1971

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

4. Geometry of the geomagnetic tail;Behannon;J. geophys. Res.,1970

5. Cooper, C. and Haskell, G. (1972). Private communication.

Cited by 16 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. Dynamics of the correlation between polar cap radio absorption and solar energetic proton fluxes in the interplanetary medium;Journal of Geophysical Research: Space Physics;2014-03

2. Magnetospheric models and trajectory computations;Space Science Reviews;2000

3. Magnetospheric Models and Trajectory Computations;Space Sciences Series of ISSI;2000

4. A static-state field-line reconnection model for the Earth's magnetosphere;Journal of Atmospheric and Terrestrial Physics;1978-03

5. Open Magnetosphere and the Auroral Oval;Astrophysics and Space Science Library;1977

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