Interplanetary hydromagnetic clouds as flare-generated spheromaks

Details Interplanetary hydromagnetic clouds as flare-generated spheromaks Interplanetary hydromagnetic clouds as flare-generated spheromaks

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...98..379i&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 98, Aug. 1985, p. 379-386.

Physics

16

Force-Free Magnetic Fields, Interplanetary Medium, Plasma Clouds, Solar Flares, Spheromaks, Interplanetary Magnetic Fields

Scientific paper

Solar flare-generated interplanetary clouds are proposed to be treated as oblate spheromaks (oblamaks) with predominantly force-free magnetic field. The solution found for a force-free field equation in spheroidal coordinates makes it possible to describe the spheromak magnetic fields by a series of spheroidal wave functions. Comparison between theoretical and experimental results is shown in the case of the hydromagnetic cloud from the November 22, 1977 flare (STIP Interval IV).

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