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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/251
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dc.contributor.authorBagchi, J-
dc.contributor.authorSubramanian, K. R-
dc.contributor.authorEbenezer, E-
dc.contributor.authorGowda, N-
dc.contributor.authorAbdul Hameed, A. T-
dc.date.accessioned2005-01-28T05:32:16Z-
dc.date.available2005-01-28T05:32:16Z-
dc.date.issued1997-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 13, pp. 133-141en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/251-
dc.description.abstractThe interpretation of the lunar occultation data recorded at the microwave frequencies of 2025, 3.80 and 4.20 GHz from two stations during the October 24, 1995 solar eclipse in India is presented.en
dc.format.extent629401 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectSolar eclipseen
dc.subjectLunar occultationen
dc.subjectMicrowave emissionen
dc.subjectActive regionsen
dc.subjectX-ray emissionen
dc.titleLunar Occultation Observations of the Microwave Sun During the Eclipse of October 24, 1995en
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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