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Longitudinal shower development and its signature at observation level

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dc.contributor.author Chitnis, V. R
dc.contributor.author Bhat, P. N
dc.date.accessioned 2008-06-19T06:04:00Z
dc.date.available 2008-06-19T06:04:00Z
dc.date.issued 2002
dc.identifier.citation BASI, Vol. 30, No. 1, pp. 351 - 355 en
dc.identifier.uri http://hdl.handle.net/2248/2450
dc.description.abstract From a study of Cverenkov photon arrival times at various core distances at the observation level it has already been established that the photon front is well fitted with a spherical surface traveling at the speed of light and originating from a fixed point on the shower axis. The radius of curvature as measured at the observation level has been found to be roughly equal to the height of shower maximum from the observation level. In the present work we study the relationship between the radius of curvature of the shower fromt (R), the height of electron maximum (he), the Cverenkov photon maximum (hCv) and the average production height of Cverenkov photons (h-). Cverenkov pulse width (w) has always ben used as a parameter to study cascade development especially at tens of PeV energies. We discuss the relation between the w and he at TeV energies for gamma-ray and proton primaries. en
dc.format.extent 449869 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..351C en
dc.subject VHE Gamma-Ray Astronomy en
dc.subject Air Shower Simulations en
dc.title Longitudinal shower development and its signature at observation level en
dc.type Article en


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