Magnetic quenching of turbulent diffusivity: Reconciling mixing-length theory estimates with kinematic dynamo models of the solar cycle

Astrophysical Journal Letters

Volumn 727, Issue 1 PART II, 2011, Pages

  Muñoz Jaramillo, Andrés ^a,b   Nandy, Dibyendu ^c   Martens, Petrus C H ^a,b  

^a MONTANA STATE UNIVERSITY   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c INDIAN INSTITUTE OF SCIENCE EDUCATION AND RESEARCH KOLKATA   (India)

Author keywords

Sun: activity; Sun: dynamo; Sun: interior

Indexed keywords

EID: 79960273093     PISSN: 20418205     EISSN: 20418213     Source Type: Journal    
DOI: 10.1088/2041-8205/727/1/L23     Document Type: Article

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