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...
Autores principales: | , , , , |
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Formato: | Capítulo de libro |
Lenguaje: | Inglés |
Publicado: |
The American Astronomical Society
2010
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Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
Aporte de: | Registro referencial: Solicitar el recurso aquí |
LEADER | 07045caa a22010457a 4500 | ||
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001 | PAPER-8013 | ||
003 | AR-BaUEN | ||
005 | 20230711124139.0 | ||
008 | 190411s2010 xx ||||fo|||| 00| 0 eng|d | ||
024 | 7 | |2 scopus |a 2-s2.0-77949538465 | |
040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
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 | |
773 | 0 | |d Institute of Physics Publishing, 2010 |g v. 708 |h pp. L116-L120 |k n. 2 PART 2 |p Astrophys. J. Lett. |x 20418205 |t Astrophysical Journal Letters | |
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856 | 4 | 0 | |u https://doi.org/10.1088/2041-8205/708/2/L116 |x doi |y DOI |
856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_20418205_v708_n2PART2_pL116_Verdini |x handle |y Handle |
856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_20418205_v708_n2PART2_pL116_Verdini |x registro |y Registro en la Biblioteca Digital |
901 | |a PAPER |n 10 |q Margarita Zelaya | ||
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