HR: 17:05h
AN: SH34A-04    [Abstracts]
TI: STEREO's in-situ perspective on the solar minimum solar wind structure
AU: * Luhmann, J G
EM: jgluhman@ssl.berkeley.edu
AF: Space Sciences Laboratory, University of California, Berkeley, CA 94720, United States
AU: Larson, D
EM: davin@ssl.berkeley.edu
AF: Space Sciences Laboratory, University of California, Berkeley, CA 94720, United States
AU: Schroeder, P
EM: peters@ssl.berkeley.edu
AF: Space Sciences Laboratory, University of California, Berkeley, CA 94720, United States
AU: Lee, C O
EM: clee@ssl.berkeley.edu
AF: Space Sciences Laboratory, University of California, Berkeley, CA 94720, United States
AU: Sauvaud, J
EM: sauvaud@cesr.fr
AF: CESR, CNRS, Toulouse, France
AU: Acuna, M H
EM: mha@lepmom.gsfc.nasa.gov
AF: NASA, Goddard Space Flight Center, Greenbelt, MD 20771, United States
AU: Galvin, A B
EM: toni.galvin@unh.edu
AF: SSC, University of New Hampshire, Durham, NH 03824, United States
AU: Russell, C T
EM: ctrussel@igpp.ucla.edu
AF: IGPP, UCLA, Los Angeles, CA 90095, United States
AU: Jian, L
EM: jlan@igpp.ucla.edu
AF: IGPP, UCLA, Los Angeles, CA 90095, United States
AU: Arge, C N
EM: nick.arge@hanscom.af.mil
AF: AFRL, Hanscom AFB, MA 01731, United States
AU: Odstrcil, D
EM: dusan.odstrcil@noaa.gov
AF: CIRES and, NOAA SEC, Boulder, CO 80303, United States
AU: Riley, P
EM: pete.riley@saic.com
AF: SAIC, San Diego, CA 92121, United States
AU: Howard, R A
EM: russ.howard@nrl.navy.mil
AF: Naval Research, Laboratory, Washington, DC 20375, United States
AU: Aschwanden, M
EM: aschwanden@lmsal.com
AF: LMSAL, Lockheed, Palo Alto, CA 94304, United States
AU: MacNeice, P
EM: pmacneic@pop900.gsfc.nasa.gov
AF: CCMC, GSFC, Greenbelt, MD 20771, United States
AU: Chulaki, A
EM: achulaki@nasa.gov
AF: CCMC, GSFC, Greenbelt, MD 20771, United States
AB: 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
DE: 2102 Corotating streams
DE: 2134 Interplanetary magnetic fields
DE: 2164 Solar wind plasma
DE: 2169 Solar wind sources
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2007 Joint Assembly