STEREO's in-situ perspective on the solar minimum solar wind structure

Details STEREO's in-situ perspective on the solar minimum solar wind structure STEREO's in-situ perspective on the solar minimum solar wind structure

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agusmsh34a..04l&link_type=abstract

American Geophysical Union, Spring Meeting 2007, abstract #SH34A-04

Physics

2102 Corotating Streams, 2134 Interplanetary Magnetic Fields, 2164 Solar Wind Plasma, 2169 Solar Wind Sources

Scientific paper

STEREO multipoint measurements of the solar wind structure with the IMPACT and PLASTIC investigations, near Earth but off the Sun-Earth line, allow its sources and structure to be examined at solar minimum when such studies are particularly straightforward. With the aid of 3D models of the heliosphere available at the CCMC, we map the in-situ observations to their solar sources using a combination of the open field regions inferred from the SECCHI EUVI imagers and SOHO EIT, and the magnetogram-based models of the corona and solar wind. Our ultimate goal is the continuous tracking of solar wind source regions as the STEREO mission progresses, as well as the use of the mappings to deduce the distinctive properties of solar wind from different types of sources

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