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dc.date.accessioned | 2020-06-22T14:43:16Z | |
dc.date.available | 2020-06-22T14:43:16Z | |
dc.date.issued | 1973 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/98724 | |
dc.description.abstract | We discuss the observations of two eruptive prominences, and the formation of condensations during the phenomena. The density and intensity variations of the condensations are analyzed spectroscopically in one of the events. Some hypotheses about the magnetic field configuration have been used in order to explain the observational data. The paper in full will be published in Solar Physics. | en |
dc.language | es | es |
dc.subject | Galaxias | es |
dc.title | Analysis of two active prominences | en |
dc.type | Articulo | es |
sedici.identifier.issn | 1669-9521 | es |
sedici.creator.person | Machado, M.E. | es |
sedici.subject.materias | Astronomía | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Asociación Argentina de Astronomía | es |
sedici.subtype | Comunicacion | es |
sedici.rights.license | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
sedici.relation.journalTitle | Boletín de la Asociación Argentina de Astronomía | es |
sedici.relation.journalVolumeAndIssue | no. 17 | es |