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dc.date.accessioned | 2020-06-22T14:18:39Z | |
dc.date.available | 2020-06-22T14:18:39Z | |
dc.date.issued | 1973 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/98719 | |
dc.description.abstract | Macroscopic velocity fields have been studied in a solar prominence. The spectra and monochromatic images were analysed, and the existence of a contracting motion, possibly due to a pinch effect, is discussed. A helical shape of the prominence is proposed. The paper in full will be published in Solar Physics | en |
dc.language | es | es |
dc.subject | Galaxias | es |
dc.title | Macroscopic motions in prominences I, the prominence of 26th March, 1971 | en |
dc.type | Articulo | es |
sedici.identifier.issn | 1669-9521 | es |
sedici.creator.person | Machado, M.E.. | es |
sedici.creator.person | Grossi-Gallegos, H | 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 |