Session 71. Large-Scale Features of the Solar Corona

SPD Poster, Thursday, June 3, 2004, 9:20am-4:00pm, Ballroom

71.01 Electron Density Inversion and Modeling of a streamer using EIT-LASCO Data of January 2004

A.F. Thernisien (Universities Space Research Association), R.A. Howard (Naval Research Lab), Ch. Marqué (Universities Space Research Association), A. Vourlidas (Naval Research Lab)

71.02 Simulation of Microwave Emissions from Helmet Streamer

S. D. Tun, D. E. Gary, J. Lee (NJIT)

71.03 Properties of Equatorial Streamers during Solar Minimum

L. Strachan, A.V. Panasyuk, M.-P. Miralles (Harvard-Smithsonian Center for Astrophysics)

71.04 Simulations of the Quiet Sun Emission at Metric and Decimetric Radio Wavelengths

C. Marqué (USRA-NRL), Y.M. Wang (NRL), A.F. Thernisien (USRA-NRL), A. Vourlidas, R.A. Howard (NRL)

71.05 Differentiating Coronal Holes from the Quiet Sun by He 1083 nm imaging spectroscopy.

O. V. Malanushenko (National Solar Observatory), H.P. Jones (NASA's GSFC)

71.06 Towards a Physical Characterization of Large Coronal Holes

M. P. Miralles, S. R. Cranmer, J. L. Kohl (Harvard-Smithsonian CfA)

71.07 Solar Irradiance Variations in the Visible and Infrared:Comparison of the SORCE SIM instrument to the RISE model

J. Harder, S. Davis, J. Fontenla, G. Rottman, O. White (LASP, University of Colorado)

71.08 The use of amateur comet images as probes of the solar wind

G. H. Jones (NASA Jet Propulsion Laboratory, California Institute of Technology), J. C. Brandt (Dept. of Physics and Astronomy, University of New Mexico)