Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1853
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dc.contributor.authorSubramanian, K. R-
dc.contributor.authorSawant, H. S-
dc.contributor.authorFernandes, F. C. R-
dc.contributor.authorCecatto, J. R-
dc.date.accessioned2007-10-05T11:34:00Z-
dc.date.available2007-10-05T11:34:00Z-
dc.date.issued2006-03-
dc.identifier.citationAstronomy and Astrophysics, Vol. 447, No. 3, pp.1121 - 1123en
dc.identifier.urihttp://hdl.handle.net/2248/1853-
dc.description.abstractWe observed the solar eclipse of November 3, 1994 with a 4-m diameter antenna and a radio spectrograph operating at 1.5 ± 0.05 GHz with a time resolution of 100 ms. Here we present the observations of the occultation of the solar active region AR 7798 by the lunar limb. From the derivative of the eclipse curve, we found a source with an angular size of ≈ 12 s of arc associated with this active region.en
dc.format.extent663373 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.relation.urien
dc.relation.urihttp://www.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aa/abs/2006/09/aa2857-05/aa2857-05.htmlen
dc.subjectSun: radio radiationen
dc.subjectSun: activityen
dc.subjectSunspotsen
dc.subjectSun: chromosphereen
dc.titleOccultation of a solar active region at 1.5 GHz during the eclipse of November 3, 1994en
dc.typeArticleen
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