Physics
Scientific paper
Jan 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991srtoh..11..131k&link_type=abstract
Sci. Rep. Tôhoku Univ., Eighth Ser., Vol. 11, Nos. 2/3, p. 131 - 136
Physics
1
Scientific paper
The authors discuss a numerical treatment of the resistive MHD winds which are driven by strongly magnetized, rotating stars. For simplicity, the axis of rotation is assumed to coincide with that of magnetization. It is shown that rotation-driven wind solutions surely exist, to the set of resistive MHD equations even when the stellar magnetic fields remain of closed type.
Kaburaki Osamu
Kudoh Takahiro
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