Session 72. Solar Input to the Heliosphere

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

72.01 Multiple Ions Resonant Heating and acceleration by Alfvén/cyclotron Fluctuations in the corona and the solar Wind

X. Hong, L. Ofman (Catholic University of America)

72.02 Stochastic Acceleration of 3He and 4He by Parallel Propagating Plasma Waves

V. Petrosian (Dept. of Physics and Applied Physics, CSSA, Stanford Univ.), S. Liu (Dept. of Phys, CSSA, Stanford University), G. Mason (Dept. of Phys. and Institute for Physical Sciences and Technology, University of Maryland)

72.03 Determining Shock velocities that are needed for model inputs at the Sun from from ground-based radio data and space-based coronagraph data.

Z. Smith, M. Dryer (NOAA/SEC), C. D. Fry (Exploration Physic International, Inc.)

72.04 A Statistical Study on the Acceleration of CMEs

J. Zhang (George Mason University)

72.05 Contributions from Ultraviolet Spectroscopy to the Prediction of High-energy Proton Hazards from CME Shocks

J. Lin, J. C. Raymond, S. R. Cranmer, J. L. Kohl (Harvard-Smithsonian CfA)

72.06 The STEREO Science Center

W. T. Thompson, M. Kaiser, T. Kucera (NASA Goddard Space Flight Center)

72.07 A Comparison of the Mg II Index Derived from Estimated and Observed Solar Spectra

J. Morrill, C. Korendyke, K. Dere (Naval Research Laboratory)

72.08 Magnetic Effects and our Changing View of the Heliosheath

P. C. Liewer, M. Opher (Jet Propulsion Laboratory, California Institute of Technology), M. Velli (University of Florence, Italy), T. I. Gombosi, W. Manchester, D. L. DeZeeuw, G. Toth, I. Sokolov (Universtiy of Michigan)