Variation of cosmic rays and solar wind properties with respect to the heliospheric current sheet: 1, Five-GeV protons and solar wind speed

Author:

Newkirk Gordon,Fisk Lennard A.

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

Reference121 articles.

1. Solar polar coronal holes and the north-south cosmic ray gradient;Agrawal;Geophys. Res. Lett.,1978

2. Solar polar coronal holes and galactic cosmic ray intensities;Agrawal;J. Geophys. Res.,1980

3. 27-day variations of solar activity and cosmic ray intensity and the determination of the effective size of the asymmetric solar wind;Alaniya;Proc. Int. Conf Cosmic Rays, 11th,1970

4. Cosmic ray perpendicular gradient during 1962–1972;Antonucci;J. Geophys. Res.,1976

5. Phase reversals in the polar magnetic fields of the sun and in the annual and semiannual variation in cosmic-ray intensity;Antonucci;Astrophys. J.,1978

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