Zenith angle dependence of pressure effect in GRAPES-3 muon telescope

M. Zuberi,S. Ahmad,M. Chakraborty, A. Chandra,S. R. Dugad,U. D. Goswami, S. K. Gupta,B. Hariharan, Y. Hayashi, P. Jagadeesan, A. Jain, P. Jain, S. Kawakami, H. Kojima,S. Mahapatra,P. K. Mohanty,R. Moharana, Y. Muraki,P. K. Nayak,T. Nonaka, A. Oshima, B. P. Pant,D. Pattanaik, G. S. Pradhan, P. S. Rakshe, M. Rameez,K. Ramesh,L. V. Reddy, R. Sahoo, R. Scaria, S. Shibata, J. Soni, K. Tanaka,F. Varsi

37TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2021(2022)

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摘要
A large area (560 m(2)) muon telescope in the GRAPES-3 experiment at Ooty, India records muon intensity at high cutoff rigidities (R-C) varies from 14-32 GV along 169 independent directions spanning a field of view of 2.3 sr. The threshold energy of the recorded muons is sec(theta) GeV along a direction with a zenith angle (theta) and with the average angular accuracy of similar to 4 degrees. The directional capabilities of the muon telescope are exploited for studying the effect of atmospheric pressure on the muon flux as a function of R-C. It is observed that the barometric coefficients relationship with logarithmic R-C can be well described by second-order polynomial function with a high Spearman Rank correlation coefficient of 0.99.
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