A simple concept for modeling cosmic ray modulation in the inner heliosphere during solar cycles 20–23

Author:

Wibberenz G.

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

Reference60 articles.

1. Large scale modulation: View from Earth;Belov;Space Sci. Rev.,2000

2. Long-term variations of galactic cosmic rays and their relation to the solar magnetic parameters;Belov;Proc. Int. Conf. Cosmic Rays,2001

3. Rigidity dependence of cosmic-ray proton latitudinal gradients measured by the Ulysses spacecraft: Implications for the diffusion tensor;Burger;J. Geophys. Res.,2000

4. Magnetic field strength distributions and spectra in the heliosphere and their significance for cosmic ray modulation: Voyager 1, 1980–1994;Burlaga;J. Geophys. Res.,1998

5. Cosmic ray modulation and turbulent interaction regions near 11 AU;Burlaga;J. Geophys. Res.,1985

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