作者: Ed Sittler , Madhullika Guhathakurta , Ruth Skoug
DOI: 10.1007/978-94-017-3230-7_7
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摘要: We have developed a semi-empirical 2-D MHD model of the solar corona and wind for which major data inputs are white light coronagraph plasma magnetic field from Ulysses spacecraft. With regard to we used Spartan 201–05 construct our empirical models electron density field. then use conservations laws mass, momentum energy compute estimates flow velocity, effective temperature heat flux as function radial distance latitude. will compare with that other theoretical models. An example, is WKB contribution Alfven waves flux. also investigated importance conduction in context past present preliminary description conduction.