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| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.provenance | Facultad de Ciencias Exactas y Naturales de la UBA | - |
| dc.contributor | Greco, A. | - |
| dc.contributor | Matthaeus, W.H. | - |
| dc.contributor | D'Amicis, R. | - |
| dc.contributor | Servidio, S. | - |
| dc.contributor | <div class="autor_fcen" id="2615">Dmitruk, P.</div> | - |
| dc.creator | Greco, A. | - |
| dc.creator | Matthaeus, W.H. | - |
| dc.creator | D'Amicis, R. | - |
| dc.creator | Servidio, S. | - |
| dc.creator | <div class="autor_fcen" id="2615">Dmitruk, P.</div> | - |
| dc.date.accessioned | 2018-05-04T22:08:20Z | - |
| dc.date.accessioned | 2018-05-28T15:47:35Z | - |
| dc.date.available | 2018-05-04T22:08:20Z | - |
| dc.date.available | 2018-05-28T15:47:35Z | - |
| dc.date.issued | 2012 | - |
| dc.identifier.uri | http://10.0.0.11:8080/jspui/handle/bnmm/68320 | - |
| dc.description | The formation of coherent structures in turbulence is a signature of a developing cascade and therefore might be observable by analyzing inner heliospheric solar wind turbulence. To test this idea, data from the Helios 2 mission, for six streams of solar wind at different heliocentric distances and of different velocities, were subjected to statistical analysis using the partial variance of increments (PVI) approach. We see a clear increase of the PVI distribution function versus solar wind age for higher PVI cutoff, indicating development of non-Gaussian coherent structures. The plausibility of this interpretation is confirmed by a similar behavior observed in two-dimensional magnetohydrodynamics simulation data at corresponding dimensionless nonlinear times. © 2012. 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. 2012;749(2) | - |
| dc.source.uri | http://digital.bl.fcen.uba.ar/Download/paper/paper_0004637X_v749_n2_p_Greco.pdf | - |
| dc.subject | magnetohydrodynamics (MHD) | - |
| dc.subject | solar wind | - |
| dc.subject | turbulence | - |
| dc.title | Evidence for nonlinear development of magnetohydrodynamic scale intermittency in the inner heliosphere | - |
| 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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