Intensity Variation of Photons During the Solar Eclipse

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/292

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DC Field	Value	Language
dc.contributor.author	Chandole, S. V	-
dc.contributor.author	Shah, S. S	-
dc.date.accessioned	2005-02-03T05:06:44Z	-
dc.date.available	2005-02-03T05:06:44Z	-
dc.date.issued	1980-06	-
dc.identifier.citation	BASI, Vol. 8, Nos. 2&3, pp. 91-92	en
dc.identifier.uri	http://hdl.handle.net/2248/292	-
dc.description.abstract	The study was aimed to determine the variation of intensity of photons from the Sun during solar eclipse at Aurangabad (altitude 586 meters, latitude 19 degree 5' and longitude 95 degree 24'). It was carried out with the help of photoconductive cells and G. M . counter. Quantitative estimate of decrease in intensity of photons mostly in eV range has been done. In all the three experiments performed with the help of two photoconductive cells and G. M. counter, the decrease in the intensity of photons is found to be of the order of two and we found many other interesting results in this study.	en
dc.format.extent	227582 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Tata Institute of Fundamental Research, Bombay	en
dc.subject	Total Solar Eclipse	en
dc.subject	Intensity Variation	en
dc.subject	Intersity Variation of Photons	en
dc.title	Intensity Variation of Photons During the Solar Eclipse	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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