Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | Cristiani, Germán Diego | - |
| dc.creator | Giménez de Castro, C. G. | - |
| dc.creator | Mandrini, Cristina Hemilse | - |
| dc.creator | Machado, Marcos Emilio | - |
| dc.creator | Rovira, Marta Graciela | - |
| dc.date | 2017-09-25T18:39:21Z | - |
| dc.date | 2017-09-25T18:39:21Z | - |
| dc.date | 2009-11 | - |
| dc.date | 2017-09-20T13:40:28Z | - |
| dc.date.accessioned | 2019-04-29T15:43:48Z | - |
| dc.date.available | 2019-04-29T15:43:48Z | - |
| dc.date.issued | 2017-09-25T18:39:21Z | - |
| dc.date.issued | 2017-09-25T18:39:21Z | - |
| dc.date.issued | 2009-11 | - |
| dc.date.issued | 2017-09-20T13:40:28Z | - |
| dc.identifier | Cristiani, Germán Diego; Giménez de Castro, C. G.; Mandrini, Cristina Hemilse; Machado, Marcos Emilio; Rovira, Marta Graciela; Asymmetric precipitation in a coronal loop as explanation of a singular observed spectrum; Elsevier; Advances in Space Research; 44; 11; 11-2009; 1314-1320 | - |
| dc.identifier | 0273-1177 | - |
| dc.identifier | http://hdl.handle.net/11336/25052 | - |
| dc.identifier | CONICET Digital | - |
| dc.identifier | CONICET | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/300515 | - |
| dc.description | Almost 10 years of solar submillimeter observations have shown new aspects of solar activity, such as the presence of rapid solar spikes associated with the launch of coronal mass ejections and an increasing submillimeter spectral component in flares. We analyse the singular microwave-submillimeter spectrum of an M class solar flare on 20 December, 2002. Flux density observations measured by Sun patrol telescopes and the Solar Submillimeter Telescope are used to build the radio spectrum, which is fitted using Ramaty´s code. At submillimeter frequencies the spectrum shows a component different from the microwave classical burst. The fitting is achieved proposing two homogeneous sources of emission. This theoretical fitting is in agreement with differential precipitation through a magnetically asymmetric loop or set of loops. From a coronal magnetic field model we infer an asymmetric magnetic structure at the flare location. The model proposed to quantify the differential precipitation rates due to the asymmetry results in a total precipitation ratio Q2/Q1≈104-105, where Q1(Q2) represents the total precipitation in the loop foot with the high (low) magnetic field intensity. This ratio agrees with the electron total number ratio of the two sources proposed to fit the radio spectrum. | - |
| dc.description | Fil: Cristiani, Germán Diego. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina | - |
| dc.description | Fil: Giménez de Castro, C. G.. Escola de Engenharia; Brasil | - |
| dc.description | Fil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina | - |
| dc.description | Fil: Machado, Marcos Emilio. Universidade Presbiteriana Mackenzie. Escola de Engenharia; Brasil | - |
| dc.description | Fil: Rovira, Marta Graciela. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | Elsevier | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1016/j.asr.2009.06.012 | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0273117709003913 | - |
| dc.rights | info:eu-repo/semantics/restrictedAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | - |
| dc.source | reponame:CONICET Digital (CONICET) | - |
| dc.source | instname:Consejo Nacional de Investigaciones Científicas y Técnicas | - |
| dc.source | instacron:CONICET | - |
| dc.subject | Sol | - |
| dc.subject | ACTIVIDAD | - |
| dc.subject | EYECCIONES DE MASA CORONAL | - |
| dc.subject | SUBMILIMETRICO | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | Asymmetric precipitation in a coronal loop as explanation of a singular observed spectrum | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| Aparece en las colecciones: | CONICET | |
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