Statistics – Computation
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988p%26ss...36..669a&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 36, July 1988, p. 669-675.
Statistics
Computation
2
Computational Astrophysics, Interplanetary Space, Shock Wave Interaction, Solar Activity Effects, Astronomical Models, Solar Flares, Solar Wind, Statistical Analysis
Scientific paper
Three interplanetary shock events during the first week of April 1979 are modeled by the method developed originally by Hakamada and Akasofu (1982). There occurred a large number of weak and medium intensity solar flares during this period. However, solar wind observations at three points, the Earth (ISEE-3), Helios A and B, enabled the authors to choose three solar flares and their parameters in such a way that the simulated arrival times and the speed jumps of the shock waves at the three points are in fair agreement with the observations.
Akasofu Syuh-Ichi
Lee Li-Her
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