DO oblique ALFVéN/ion-cyclotron or fast-mode/whistler waves dominate the dissipation of solar wind turbulence near the proton inertial length?

Astrophysical Journal Letters

Volumn 745, Issue 1, 2012, Pages

  He, Jiansen ^a,b   Tu, Chuanyi ^a   Marsch, Eckart ^c   Yao, Shuo ^d  

^a PEKING UNIVERSITY   (China)

^b INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

^c MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^d CHINA UNIVERSITY OF GEOSCIENCES   (China)

Author keywords

solar wind; turbulence; waves

Indexed keywords

EID: 84855696928     PISSN: 20418205     EISSN: 20418213     Source Type: Journal    
DOI: 10.1088/2041-8205/745/1/L8     Document Type: Article

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