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A mini ACT experiment at low and high altitudes

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dc.contributor.author Vishwanath, P. R
dc.contributor.author Acharya, B. S
dc.contributor.author Bhat, P. N
dc.contributor.author Chitnis, V. R
dc.date.accessioned 2009-09-08T14:12:48Z
dc.date.available 2009-09-08T14:12:48Z
dc.date.issued 2005
dc.identifier.citation Sripathi Acharya, B. eds., [et al.]... Proceedings of the 29th International Cosmic Ray Conference. August 3 - 10, 2005, Pune, India. pp. 271 - 274 en
dc.identifier.uri http://hdl.handle.net/2248/4796
dc.description.abstract A simple experimental apparatus was used to measure rate of cosmic ray events due to Atmospheric Cerenkov Radiation at two mountain altitude sites with the height difference of 3.5 km. The event rates at Hanle (altitude ~ 4.5 km AMSL) was found to be a factor ~ 2 higher than those at Pachmarhi (altitude ~1 km AMSL). Consideration of the ratio of mean distance of the Cerenkov photon from the axis of the shower for the two altitudes shows a decrease in energy threshold of cosmic rays by a factor of 3.5 ± 0.7 at the higher altitude. A semi Monte Carlo calculation using the lateral distribution curves and the detector response also shows a similar decrease in the energy threshold. However, for a bigger array like the one at Pachmarhi the energy threshold is expected to decrease by a larger factor (~ 6 ± 2) since cosmic rays become inefficient in production of Cerenkov light at lower energies. en
dc.language.iso en en
dc.publisher Tata Institute of Fundamental Research en
dc.relation.ispartofseries International Cosmic Ray Conference;Vol. 5
dc.relation.uri http://adsabs.harvard.edu/abs/2005ICRC....5..271V en
dc.subject ACT Experiment en
dc.subject Cosmic Ray en
dc.subject Atmospheric Cerenkov Radiation en
dc.subject Cerenkov Photon en
dc.subject Threshold of Cosmic Rays en
dc.subject Semi Monte Carlo Calculation en
dc.subject Energy Threshold en
dc.subject Cerenkov Light at Lower Energies en
dc.title A mini ACT experiment at low and high altitudes en
dc.type Article en


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