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dc.date.accessioned | 2020-06-22T15:19:16Z | |
dc.date.available | 2020-06-22T15:19:16Z | |
dc.date.issued | 1973 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/98735 | |
dc.description.abstract | The Leighton methods supplies with a bidimensional map of the longitudinal component of the magnetic field. The principles of this method are used for measuring fields in facular zones, using the line Fe 6302.5. Qualitatively good photos have been obtained, with a spacial resolution of 3" - 4". | en |
dc.language | es | es |
dc.subject | Galaxias | es |
dc.title | Medición de campos magnéticos solares | es |
dc.type | Articulo | es |
sedici.identifier.issn | 1669-9521 | es |
sedici.creator.person | Silva, F.A. | 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 |