Physics
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986p%26ss...34..987m&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 34, Oct. 1986, p. 987-989, 991, 992.
Physics
3
Interplanetary Magnetic Fields, Magnetospheric Instability, Brightness Distribution, Magnetohydrodynamic Flow, Simulation, Solar Wind, Time Dependence
Scientific paper
The interaction between the IMF Bz and the magnetosphere is simulated by
a laboratory method. The results show that the amount of solar-wind
plasma which enters and is subsequently trapped in the magnetosphere
depends on the IMF Bz. In this steady IMF study, no notable
time-dependent instability was observed.
Akasofu Syun-Ichi
Minami Shigeyuki
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