The Solar Wind Near 70 AU in the Declining Stage of the Solar Cycle.

Details The Solar Wind Near 70 AU in the Declining Stage of the Solar Cycle. The Solar Wind Near 70 AU in the Declining Stage of the Solar Cycle.

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsh12b..06r&link_type=abstract

American Geophysical Union, Fall Meeting 2003, abstract #SH12B-06

Physics

2102 Corotating Streams, 2104 Cosmic Rays, 2124 Heliopause And Solar Wind Termination, 2162 Solar Cycle Variations (7536), 2164 Solar Wind Plasma

Scientific paper

The declining portion of the solar cycle near 35 AU was characterized by a shock-ramp structure with a period of roughly a solar rotation. We discuss the structure observed near 70 AU by Voyager 2, where the shock ramp structure is again seen but with a period of 4-5 solar rotations. At Voyager 2, merging of solar wind driven by CMEs results in correlated changes in speed, density, and magentic field magnititude and thus in dynamic pressure. These order of magnitude changes in pressure should have significant effects on the movement of the termination shock and the propagation of ACRs.

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