HR: 0830h
AN: SP51B-05    [Abstracts]
TI: The Complexity of Equatorial Coronal Holes
AU: * McIntosh, S W
EM: mcintosh@boulder.swri.edu
AF: DoSS, Southwest Research Institute, 1050 Walnut St., Suite 400, Boulder, CO 80302 United States
AU: Davey, A R
EM: ard@boulder.swri.edu
AF: DoSS, Southwest Research Institute, 1050 Walnut St., Suite 400, Boulder, CO 80302 United States
AU: Hassler, D M
EM: hassler@boulder.swri.edu
AF: DoSS, Southwest Research Institute, 1050 Walnut St., Suite 400, Boulder, CO 80302 United States
AB: We will investigate the multi-thermal intensities, flow structures and extrapolated magnetic structures in an massive equatorial coronal holes that crossed the solar disk in early November of 1999. We will use a large suite of observations from the MDI and SUMER instruments on SOHO. We will use the insight developed from our understanding of the multi-thermal coronal hole topography to propose a consistent picture of solar wind structure at the base of the Sun-Earth Connection.
DE: 7500 SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY
DE: 7511 Coronal holes
DE: 7524 Magnetic fields
DE: 7546 Transition region
SC: Solar Physics Division - AAS [SP]
MN: 2005 Joint Assembly