论文信息 - Analysis of EIT/LASCO Observations Using Available MHD Models: Initiation Propagation and Geoeffectiveness

Analysis of EIT/LASCO Observations Using Available MHD Models: Initiation Propagation and Geoeffectiveness

FINAL REPORTNAG5-9508Analysis of EIT/LASCO Observations Using Available MHD Models:Initiation Propagation and GeoeffectivenessInvestigation of CMEPeriod of Performance: June l, 2000 - May 31,2001ByS. T. WuCenter for Space Plasma and Aeronomic ResearchDepartment of Mechanical & Aerospace EngineernigThe University of Alabama in HuntsvilleHuntsville, AL 35899 USA

S. Wu

[1] G. Simnett. The relationship between prominence eruptions and coronal mass ejections , 2000 .

[2] Barbara June Thompson,et al. Relationship of halo coronal mass ejections, magnetic clouds, and magnetic storms , 2000 .

[3] B. Low,et al. Magnetostatic structures of the solar corona. 2: The magnetic topology of quiescent prominences , 1995 .

[4] C. Cyr,et al. A Revised and Expanded Catalogue of Mass Ejections Observed by the Solar Maximum Mission Coronagraph , 1993 .

[5] S. Suess,et al. The steady global corona , 1982 .

[6] F. Mariani,et al. Magnetic loop behind an interplanetary shock: Voyager, Helios and IMP-8 observations , 1981 .

[7] S. Wu,et al. Magnetohydrodynamic models of coronal transients in the meridional plane. I - The effect of the magnetic field , 1978 .

[8] R. MacQueen,et al. Mass ejections from the Sun: A view from Skylab , 1974 .