Observation of cosmic ray sidereal time variation by Grapes III muon telescope at Ooty

Details Observation of cosmic ray sidereal time variation by Grapes III muon telescope at Ooty Observation of cosmic ray sidereal time variation by Grapes III muon telescope at Ooty

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc...10.3943k&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

We analyzed the sidereal time variation on the data of muons counting rate observed by the large muon telescope of GRAPES III ( total area 560 m2 , muon's energy > 1GeV) over 3 years at Ooty ( 11.4deg latitude, 76.7deg longitude). Their counting rate is around 53,000 counts /sec and this high counting rate is great advantage for modulation measurement. The analysis based on the data of such high-statistics enable us to compare the sidereal diurnal variation even with each single year's result. We observed the Tail-in and Loss corn anisotropies through detailed analysis. We newly started the measurement of direction of individual muons with accuracy of about 8 degrees from 1999. We present some results on the siderealdailyvariation obtained by this systemtoo.

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