Intensities of galactic cosmic rays of ∼1.5 GV rigidity at Earth versus the heliospheric current sheet tilt

Author:

Lockwood J. A.1,Webber W. R.2

Affiliation:

1. Space Science Center; University of New Hampshire; Durham New Hampshire USA

2. Department of Astronomy; New Mexico State University; Las Cruces New Mexico USA

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

Reference20 articles.

1. Field gradient and curvature drifts and cosmic ray transport into the solar system;Barnden;Proc. Int. Conf. Cosmic Rays 14th,1975

2. The effect of large heliospheric current sheet tilt angles in numerical modulation models: A theoretical assessment;Burger;Proc. Int. Conf. Cosmic Rays 26th,1999

3. Cosmic ray modulation and the solar magnetic field;Cane;Geophys. Res. Lett.,1999

4. 22 year patterns in the relationship of sunspot number and tilt angle to cosmic-ray intensity;Cliver;Astrophys. J.,2001

5. Modulation over a 22-year cosmic ray cycle: On the tilt angles of the heliospheric current sheet;Ferreira;Adv. Space Res.,2003

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