Revisiting two-step Forbush decreases

Author:

Jordan A. P.1,Spence H. E.1,Blake J. B.2,Shaul D. N. A.3

Affiliation:

1. Institute for the Study of Earth, Oceans, and Space; University of New Hampshire; Durham New Hampshire USA

2. The Aerospace Corporation; El Segundo California USA

3. High Energy Physics Group, Department of Physics; Imperial College London; London UK

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

Reference29 articles.

1. The large-scale magnetic field configuration associated with Forbush decreases;Barnden;Conf. Pap. Int. Cosmic Ray Conf. 13th,1973

2. Anisotropic cosmic radiation fluxes of solar origin;Bartley;J. Geophys. Res.,1966

3. Flux tube texture of the solar wind: Strands of the magnetic carpet at 1 AU?;Borovsky;J. Geophys. Res.,2008

4. Solar wind temperature and speed.;Burlaga;J. Geophys. Res.,1973

5. Cosmic ray decreases and magnetic clouds;Cane;J. Geophys. Res.,1993

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