Two-fluid model for heating of the solar corona and acceleration of the solar wind by high-frequency Alfvén waves

Solar Physics

Volumn 171, Issue 2, 1997, Pages 363-391

  Tu, C Y ^a,b   Marsch, E ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b PEKING UNIVERSITY   (China)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0031503448     PISSN: 00380938     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1004968327196     Document Type: Article

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