Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/272
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dc.contributor.authorJaaffrey, S. N. A-
dc.contributor.authorJain, Rajmal-
dc.contributor.authorPandya, Alok-
dc.contributor.authorBharti, Lokesh-
dc.date.accessioned2005-01-31T05:49:00Z-
dc.date.available2005-01-31T05:49:00Z-
dc.date.issued1997-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 13, pp. 235-240en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/272-
dc.description.abstractWe report the first observations of absorption and enhancement in flux of high energy photons during thte total solar eclipse of October 24, 1995. For the purpose of these observations, we employed a scintillation counter to detect high energy radiation in the energy range of 10 KeV to 5 MeV. The scintillation detector was coupled with ADCAM 100 ORTEC computer for data acquition and analysis. We interpret the absorption in the fluw below 300 Ke V due to the passage of the Moon between the Sun and the Earth, while enhancement above 300 Ke V could have occurred due to the production of secondary radiations from high energy photons.en
dc.format.extent144611 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectTotal solar eclipseen
dc.subjectHigh energy photonsen
dc.subjectSecondary radiationsen
dc.titleHigh Energy Photons detection using Scintillation Counter during Total Solar Eclipse of October 24, 1995en
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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