Using transient decreases of cosmic rays observed at Voyagers 1 and 2 to estimate the location of the heliospheric termination shock

Author:

Webber W. R.,Lockwood J. A.,McDonald F. B.,Heikkila B.

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

Reference21 articles.

1. Merged interaction regions observed by Voyagers 1 and 2 during 1998;Burlaga;J. Geophys. Res.,2000

2. Solar energetic particles from the April 1998 activity: Observations from 1 to 72 AU;Decker;Proc. Int. Conf. Cosmic Rays, 26th,1999

3. Global merged interaction regions, the heliospheric termination shock, and time-dependent cosmic ray modulation;le Roux;J. Geophys. Res.,1999

4. The recovery phase of the cosmic ray modulation cycle. The role of GMIRs and of hysterisis effects;McDonald;Proc. Int. Conf. Cosmic Rays, 23rd,1993

5. Effects of the intense solar activity of March/June 1991 observed in the outer heliosphere;McDonald;J. Geophys. Res.,1994

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