Large-scale heliospheric structure in 2004-2006 and its solar origin

Details Large-scale heliospheric structure in 2004-2006 and its solar origin Large-scale heliospheric structure in 2004-2006 and its solar origin

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsh44a..01r&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SH44A-01

Other

2102 Corotating Streams, 2109 Discontinuities (7811), 2162 Solar Cycle Variations (7536), 2164 Solar Wind Plasma, 2169 Solar Wind Sources

Scientific paper

As solar activity has begun to decline, the large-scale structure of the heliosphere has begun to turn simpler again. Large coronal holes and a more quiet streamer belt are structuring the heliosphere. Ulysses, on its unique orbit, has again begun to measure recurrent high-speed streams originating in coronal holes alternating with slow wind from other regions. Here, we use simple back-mapping techniques to identify the source regions of the solar wind measured by Ulysses. We relate the observed stream interfaces to solar features and give a complete list of stream interfaces for 2004 - 2006.

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