The shapes of galactic cosmic ray intensity maxima and the evolution of the heliospheric current sheet-Reference-Cited by-同舟云学术

The shapes of galactic cosmic ray intensity maxima and the evolution of the heliospheric current sheet

Published:1993 Issue:A10 Volume:98 Page:17435
ISSN:0148-0227
Container-title:Journal of Geophysical Research
language:en
Short-container-title:J. Geophys. Res.

Author:

Cliver E. W.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Link

http://www.agu.org/journals/ja/v098/iA10/93JA01420/93JA01420.pdf

Reference36 articles.

1. Quadrupole distortions of the heliospheric current sheet in 1976 and 1977;Bruno;J. Geophys. Res.,1982

2. The coronal and interplanetary current sheet in early 1976;Burlaga;J. Geophys. Res.,1981

3. Solar activity in May 1987 at the onset of the new cosmic ray modulation cycle;Cliver;Proc. 22nd Int. Cosmic Ray Conf.,1991

4. Coronal mass ejections, polar crown filaments, and cosmic ray modulation, 1979–1989;Cliver;Proc. 23rd Int. Cosmic Ray Conf.,1993

5. Historical evidence for the existence of the solar cycle;Eddy,1977

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