Numerical simulation of propagation and overlap of interplanetary shock.

Details Numerical simulation of propagation and overlap of interplanetary shock. Numerical simulation of propagation and overlap of interplanetary shock.

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992chjss..12..249g&link_type=abstract

Chin. J. Space Sci., Vol. 12, No. 4, p. 249 - 257

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Scientific paper

A time dependent, two-dimensional magnetohydrodynamic model is used to simulate the flare-associated shock waves and their subsequent disturbances in the equatorial plane between 0.1 AU and 1.1 AU. It is simulated that the shocks associated with a disturbed interplanetary medium by two flares, erupted one after another with a delay of several hours. The result shows that interactions between shocks depends on the time interval of the two flares. These interactions can be classified into four types, (1) strong interaction, (2) middle interaction, (3) weak interaction, (4) no interaction, according to the interval of flares. The result shows that interplanetary magnetic fields in the first case are similar to those in the second case, 44 hours after the introduction of the disturbances. The parameters of the solar wind measured at 1.0 AU along the flare normal also have the similar time profiles in the two cases.

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