The importance of atmospheric monitoring in Cherenkov experiments

dc.contributor.author	Osborne, J. L
dc.contributor.author	Aye, M
dc.contributor.author	Chadwick, P. M
dc.contributor.author	Daniel, M. K
dc.contributor.author	McComb, T. J. L
dc.contributor.author	McKenny, J. M
dc.contributor.author	Nolan, S. J
dc.contributor.author	Orford, K. J
dc.contributor.author	Rayner, S. M
dc.date.accessioned	2008-05-27T10:13:32Z
dc.date.available	2008-05-27T10:13:32Z
dc.date.issued	2002
dc.identifier.citation	BASI, Vol. 30, No. 1, pp. 51 - 59	en
dc.identifier.uri	http://hdl.handle.net/2248/2357
dc.description.abstract	A review is presented of Monte Carlo simulations of the effects of differing atmospheric structure and absorption models on the Imaging Atmospheric Cherenkov Telescope signal. Methods of monitoring the atmosphere are discussed.	en
dc.format.extent	728590 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2002BASI...30...51O	en
dc.subject	Atmospheric Cherenkov Telescope	en
dc.subject	Atmospheric Absorption	en
dc.subject	Atmospheric Monitoring	en
dc.title	The importance of atmospheric monitoring in Cherenkov experiments	en
dc.type	Article	en