Comparison of MHD simulation for the February 1986 events with interplanetary observations by the spacecraft Sakigake

Details Comparison of MHD simulation for the February 1986 events with interplanetary observations by the spacecraft Sakigake Comparison of MHD simulation for the February 1986 events with interplanetary observations by the spacecraft Sakigake

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sici.symp...15s&link_type=abstract

In Alabama Univ., Huntsville. STIP Symposium on Physical Interpretation of Solar/Interplanetary and Cometary Intervals p 15 (SEE

Physics

Interplanetary Medium, Intervals, Japanese Spacecraft, Magnetohydrodynamics, Simulation, Doppler Effect, Magnetic Storms, Mathematical Models, Radiation Counters, Solar Flares, Space Plasmas

Scientific paper

During the period 3-10 February 1986 a series of major solar flares occurred on the Sun and several intense geomagnetic storms took place on the Earth. To examine the causality between the solar activity and the geomagnetic activity in this period, a magnetohydrodynamic (MHD) numerical simulation was performed using a 2 1/2 -D numerical code. In that period of February 1986, the Japanese spacecraft Sakigake was at 0.84 AU, 57 deg west of the Earth. Besides the in-situ measurements of the interplanetary plasma, Sakigake also provided Doppler scintillation observations. Comparisons between the results of the MHD simulation and the measurements made by the spacecraft Sakigake are presented.

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