Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2357
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dc.contributor.authorOsborne, J. L-
dc.contributor.authorAye, M-
dc.contributor.authorChadwick, P. M-
dc.contributor.authorDaniel, M. K-
dc.contributor.authorMcComb, T. J. L-
dc.contributor.authorMcKenny, J. M-
dc.contributor.authorNolan, S. J-
dc.contributor.authorOrford, K. J-
dc.contributor.authorRayner, S. M-
dc.date.accessioned2008-05-27T10:13:32Z-
dc.date.available2008-05-27T10:13:32Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 1, pp. 51 - 59en
dc.identifier.urihttp://hdl.handle.net/2248/2357-
dc.description.abstractA 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.extent728590 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30...51Oen
dc.subjectAtmospheric Cherenkov Telescopeen
dc.subjectAtmospheric Absorptionen
dc.subjectAtmospheric Monitoringen
dc.titleThe importance of atmospheric monitoring in Cherenkov experimentsen
dc.typeArticleen
Appears in Collections:BASI Publications

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