Solar cycle dependence of the radial gradient of cosmic ray intensity
Author:
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
http://www.agu.org/journals/gl/v015/i013/GL015i013p01527/GL015i013p01527.pdf
Reference11 articles.
1. The structure of the heliospheric current sheet: 1978-1982;Hoeksema;J. Geophys. Res.,1983
2. Solar cycle evolution of solar wind speed structure between 1973 and 1985 observed with the interplanetary scintillation method;Kojima;J. Geophys. Res.,1987
3. Interplanetary cosmic ray latitudinal gradient in 1984 to 1987 using IMP 8 and Voyager data;Lockwood;J. Geophys. Res.,1988
4. Modulation of Galactic Cosmic Rays in the Heliosphere
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2. Neon produced by solar cosmic rays in ordinary chondrites;Meteoritics & Planetary Science;2017-03-27
3. THE EMPIRICAL MODE DECOMPOSITION TO STUDY THE QUASI-BIENNIAL MODULATION OF SOLAR MAGNETIC ACTIVITY AND SOLAR NEUTRINO FLUX;Advances in Adaptive Data Analysis;2012-04
4. QUASI-BIENNIAL MODULATION OF SOLAR NEUTRINO FLUX AND SOLAR AND GALACTIC COSMIC RAYS BY SOLAR CYCLIC ACTIVITY;The Astrophysical Journal;2009-12-29
5. The radial distribution of cosmic rays in the heliosphere at solar maximum;Advances in Space Research;2003-08
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