A turbulence-driven model for heating and acceleration of the fast wind in coronal holes

A model is presented for generation of fast solar wind in coronal holes, relying on heating that is dominated by turbulent dissipation of MHD fluctuations transported upward in the solar atmosphere. Scale-separated transport equations include large-scale fields, transverse Alfvénic fluctuations, and...

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Detalles Bibliográficos
Autores principales: Verdini, A. (Autor, autor), Velli, M. (autor), Matthaeus, W.H (autor), Oughton, S. (autor), Dmitruk, P. (autor)
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: The American Astronomical Society 2010
Acceso en línea:Registro en Scopus
DOI
Handle
Registro en la Biblioteca Digital
Aporte de:Registro referencial: Solicitar el recurso aquí
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100 1 |a Verdini, A.  |4 aut  |e autor 
245 1 2 |a A turbulence-driven model for heating and acceleration of the fast wind in coronal holes 
260 |b The American Astronomical Society  |c 2010 
270 1 0 |m Verdini, A.; Observatoire Royale de Belgique, 3 Avenue Circulaire, Bruxelles 1180, Belgium; email: verdini@oma.be 
506 |2 openaire  |e Política editorial 
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520 3 |a A model is presented for generation of fast solar wind in coronal holes, relying on heating that is dominated by turbulent dissipation of MHD fluctuations transported upward in the solar atmosphere. Scale-separated transport equations include large-scale fields, transverse Alfvénic fluctuations, and a small compressive dissipation due to parallel shears near the transition region. The model accounts for proton temperature, density, wind speed, and fluctuation amplitude as observed in remote sensing and in situ satellite data. © 2010. The American Astronomical Society. All rights reserved..  |l eng 
593 |a Observatoire Royale de Belgique, 3 Avenue Circulaire, Bruxelles 1180, Belgium 
593 |a Dipart. di Astronomia e Scienza Dello Spazio, Univ. di Firenze, Largo E. Fermi 3, 50125, Firenze, Italy 
593 |a Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, United States 
593 |a Department of Physics and Astronomy, University of Delaware, DE 19716, United States 
593 |a Department of Mathematics, University of Waikato, Hamilton, New Zealand 
593 |a Depart. Física, Facultad de Ciencias Exactas y Naturales, Univ. de Buenos Aires-Conicet, Argentina 
690 1 0 |a MHD 
690 1 0 |a SOLAR WIND 
690 1 0 |a TURBULENCE 
690 1 0 |a WAVES 
700 1 |a Velli, M.  |4 aut  |e autor 
700 1 |a Matthaeus, W.H.  |4 aut  |e autor 
700 1 |a Oughton, S.  |4 aut  |e autor 
700 1 |a Dmitruk, P.  |g ID autor FCEN: 2615  |9 2615  |4 aut  |e autor 
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