Grb 021211 as a faint analogue of grb 990123: exploring the similarities and differences in their optical afterglows... Ifthis is the case then it is possible that most of the energy of the burst is inanother form such as a frozen magnetic field, supernova ejecta, or a second jetcomponent....
Role of interchange instability in flux transfer event origin... Newcolder plasma of the magnetosheath with a frozen magnetic field replaces thehotter EPL plasma, and the process of EPL formation and destruction repeatsitself.The...
Application of advanced computational procedures for modeling solar-wind interactions with venus: theory and computer code... The procedures, which consist of finite difference codes to determine the gasdynamic properties and a variety of special purpose codes to determine the frozen magnetic field, streamlines, contours, plots, etc....
Development of a global 3-d magnetohydrodynamic computational model for solar wind/cometary and planetary studies... Activities described include enhancements to the present Level 1 model, development of the 3-D gas dynamic flow field solvers for the Level 2 model, and continued development of the 3-D frozen magnetic field solver for the Level 2 model