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| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.provenance | Facultad de Ciencias Exactas y Naturales de la UBA | - |
| dc.contributor | Verdini, A. | - |
| dc.contributor | Velli, M. | - |
| dc.contributor | Matthaeus, W.H. | - |
| dc.contributor | Oughton, S. | - |
| dc.contributor | <div class="autor_fcen" id="2615">Dmitruk, P.</div> | - |
| dc.creator | Verdini, A. | - |
| dc.creator | Velli, M. | - |
| dc.creator | Matthaeus, W.H. | - |
| dc.creator | Oughton, S. | - |
| dc.creator | <div class="autor_fcen" id="2615">Dmitruk, P.</div> | - |
| dc.date.accessioned | 2018-05-04T21:58:55Z | - |
| dc.date.accessioned | 2018-05-28T15:49:33Z | - |
| dc.date.available | 2018-05-04T21:58:55Z | - |
| dc.date.available | 2018-05-28T15:49:33Z | - |
| dc.date.issued | 2010 | - |
| dc.identifier.uri | http://10.0.0.11:8080/jspui/handle/bnmm/68664 | - |
| dc.description | 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.. | - |
| dc.description | Fil:Dmitruk, P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.rights | info:eu-repo/semantics/openAccess | - |
| dc.rights | http://creativecommons.org/licenses/by/2.5/ar | - |
| dc.source | Astrophys. J. Lett. 2010;708(2 PART 2):L116-L120 | - |
| dc.source.uri | http://digital.bl.fcen.uba.ar/Download/paper/paper_20418205_v708_n2PART2_pL116_Verdini.pdf | - |
| dc.subject | MHD | - |
| dc.subject | Solar wind | - |
| dc.subject | Turbulence | - |
| dc.subject | Waves | - |
| dc.title | A turbulence-driven model for heating and acceleration of the fast wind in coronal holes | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:ar-repo/semantics/artículo | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| Aparece en las colecciones: | FCEN - Facultad de Ciencias Exactas y Naturales. UBA | |
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