Non-planar mhd model for solar flare-generated disturbances in the heliospheric equatorial plane

This publication has 20 references indexed in Scilit:

• Simulation of three-dimensional solar wind disturbances and resulting geomagnetic storms
  Space Science Reviews, 1982
• Numerical model of a two-dimensional, non-plane transient magnetohydrodynamic flow
  Computers & Fluids, 1982
• Numerical experimentation on spherically symmetric one-dimensional magnetohydrodynamic (MHD) wave propagation
  Computers & Fluids, 1982
• Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP 8 observations
  Journal of Geophysical Research, 1981
• Bi‐directional streaming of solar wind electrons >80 eV: ISEE evidence for a closed‐field structure within the driver gas of an interplanetary shock
  Geophysical Research Letters, 1981
• Spatial structure of flare‐associated perturbations in the solar wind simulated by a two‐dimensional numerical MHD model
  Journal of Geophysical Research, 1981
• The Effect of Nonzero ∇ · B on the numerical solution of the magnetohydrodynamic equations
  Journal of Computational Physics, 1980
• TWO-DIMENSIONAL, TIME-DEPENDENT MHD SIMULATION OF THE DISTURBED SOLAR WIND DUE TO REPRESENTATITVE FLARE-GENERATED AND CORONAL HOLE-GENERATED DISTURBANCES
  Geofísica Internacional, 1980
• Magnetic classification of solar wind streams
  Planetary and Space Science, 1979
• Anomalously low proton temperatures in the solar wind following interplanetary shock waves-evidence for magnetic bottles?
  Published by American Geophysical Union (AGU) ,1973