Session 36. The Magnetic Structure of CMEs

Display, Tuesday, June 4, 2002, 10:00am-6:30pm, SW Exhibit Hall

36.01 3-dimensional Evolution of an Emerging Flux Tube in the Sun

T. Magara, D. W. Longcope (Montana State University)

36.02 Effects of Topology on CME Kinematic Properties

W. Liu, X. P. Zhao (W. W. Hansen Experimental Physics Laboratory, Stanford University), S. T. Wu (Center for Space Plasma and Aeronomic Research, The University of Alabama in Huntsville), P. H. Scherrer (W. W. Hansen Experimental Physics Laboratory, Stanford University)

36.03 Emergence of twisted magnetic flux into the corona

S. Gibson, B.C. Low, Y. Fan (NCAR/HAO), L. Fletcher (University of Glasgow)

36.04 Do locations of CME source regions relative to the HSB determine the appearance of the CME?

Y. Li, J. G. Luhmann (SSL, University of California, Berkeley ), X. P. Zhao (Solar physics group, Stanford University)

36.05 Acceleration of Coronal Mass Ejections in the Low Corona and Association with Surface Activity

W.M. Neupert (NOAA/SEC)

36.06 Orientation of Magnetic Fields in Erupted Solar Filaments and Geoeffectiveness of Coronal Mass Ejections

V. B. Yurchyshyn (Big Bear Solar Obs., NJIT)

36.07 A Study On Relationship Of Active Regions And Large-Scale Field

Y. Liu (HEPL, Stanford University)

36.08 Helicity driven sigmoid evolution

D. Alexander, R. Nightingale, T. R. Metcalf (Lockheed Martin Solar and Astrophysics Lab.), D. Brown (University of St. Andrews)

36.09 A Search For A Relationship Between Flare Duration and Its Associated Activated Coronal Volume

G. L. Slater (Lockheed Martin Solar and Astrophysics Laboratory), A. M. Title (Stanford Lockheed Research Institute)

36.10 Multiwavelength Study of a Coronal Mass Ejection: Eruption from AR#9393

P.K. Manoharan (Astronomy Department, University of Maryland; Physics Department, Catholic University of America), M.R. Kundu (Astronomy Department, University of Maryland)