Extended MHD modeling of the steady solar corona and the solar wind
نویسندگان
چکیده
منابع مشابه
Mhd-driven Kinetic Dissipation in the Solar Wind and Corona
Mechanisms for the deposition of heat in the lower coronal plasma are discussed, emphasizing recent attempts to reconcile the Ñuid and kinetic perspectives. Structures at magnetohydrodynamic (MHD) scales may drive a nonlinear cascade, preferentially exciting high perpendicular wavenumber Ñuctuations. Relevant dissipative kinetic processes must be identiÐed that can absorb the associated energy ...
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ژورنال
عنوان ژورنال: Living Reviews in Solar Physics
سال: 2018
ISSN: 2367-3648,1614-4961
DOI: 10.1007/s41116-018-0014-4