Solar Ultraviolet Flux Variation in the Biological Band during the Total Solar Eclipse of October 24, 1995

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/259

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DC Field	Value	Language
dc.contributor.author	Niranjan, K	-
dc.contributor.author	Thulasiraman, S	-
dc.contributor.author	Reddy, Y. S	-
dc.date.accessioned	2005-01-28T07:26:15Z	-
dc.date.available	2005-01-28T07:26:15Z	-
dc.date.issued	1997	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 179-182	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/259	-
dc.description.abstract	Solar UV B Flux measurements have been made at four discrete wavelengths of 290, 300, 310 and 320 nm during and around the solar eclipse day of 24th October 1995. The Diurnal variation of the UV flux has shown the recovery phase, the flux has shown a sharp increase compared to the normal control day values, for about one to two hours depending on the wavelength. The direct solar flux recorded in the visible and near IR wavelengths did not show any such increase, indicating that there could be some atmospheric ozone decrease either at the surface level or in the columnar level leading to an increase in the measured global UV Flux.	en
dc.format.extent	87826 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar UV flux	en
dc.subject	Solar eclipse	en
dc.subject	Radiometer	en
dc.subject	Ozone	en
dc.title	Solar Ultraviolet Flux Variation in the Biological Band during the Total Solar Eclipse of October 24, 1995	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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