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| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.provenance | Facultad de Ciencias Exactas y Naturales de la UBA | - |
| dc.contributor | <div class="autor_fcen" id="2288">Dasso, S.</div> | - |
| dc.contributor | <div class="autor_fcen" id="3802">Gómez, D.</div> | - |
| dc.contributor | <div class="autor_fcen" id="5317">Mandrini, C.H.</div> | - |
| dc.creator | <div class="autor_fcen" id="2288">Dasso, S.</div> | - |
| dc.creator | <div class="autor_fcen" id="3802">Gómez, D.</div> | - |
| dc.creator | <div class="autor_fcen" id="5317">Mandrini, C.H.</div> | - |
| dc.date.accessioned | 2018-05-04T21:55:36Z | - |
| dc.date.accessioned | 2018-05-28T15:48:19Z | - |
| dc.date.available | 2018-05-04T21:55:36Z | - |
| dc.date.available | 2018-05-28T15:48:19Z | - |
| dc.date.issued | 2002 | - |
| dc.identifier.uri | http://10.0.0.11:8080/jspui/handle/bnmm/68465 | - |
| dc.description | We perform a statistical study of the decay times for the recovery phase of the 300 most intense magnetic storms that occurred from 1 January 1957 to 31 December 1998. The Dst index in the decaying stage has been fitted by an exponential function, and a very good correlation has been obtained for most of the storms. Statistically representative values for the decay time (τ) are obtained by averaging the most reliable τ values, which resulted from applying a least squares method to the Dst index time series during every recovery phase. The mean value of τ turned out to be ∼14 ±4 hours. We have also found that for very intense storms (Dstmin < -250 nT) the values of τ tend to decrease as the intensity of the storm increases. Copyright 2002 by the American Geophysical Union. | - |
| dc.description | Fil:Dasso, S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. | - |
| dc.description | Fil:Gómez, D. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. | - |
| dc.description | Fil:Mandrini, C.H. 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 | J. Geophys. Res. A. Space Phys. 2002;107(A5) | - |
| dc.source.uri | http://digital.bl.fcen.uba.ar/Download/paper/paper_01480227_v107_nA5_p_Dasso.pdf | - |
| dc.subject | Decay time | - |
| dc.subject | Dst index | - |
| dc.subject | Intense magnetic storm | - |
| dc.subject | Recovery phase | - |
| dc.subject | Ring current | - |
| dc.title | Ring current decay rates of magnetic storms: A statistical study from 1957 to 1998 | - |
| 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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