Zobrazeno 1 - 10
of 91
pro vyhledávání: '"B.P Pant"'
Publikováno v:
SciPost Physics Proceedings, Iss 13, p 021 (2023)
The GRAPES-3 experiment is a unique, extensive air shower experiment consisting of 400 scintillator detectors spread over 25000 m$^2$ and a 560 m$^2$ muon telescope. The experiment located at Ooty, India, has been collecting data for the past two dec
Externí odkaz:
https://doaj.org/article/532e4cd096db456a8b552eca69c797b4
Akademický článek
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Autor:
F. Varsi, 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, S. Mishra, P.K. Mohanty, R. Moharana, Y. Muraki, P.K. Nayak, T. Nonaka, A. Oshima, B.P. Pant, D. Pattanaik, A.K. Pradhan, G.S. Pradhan, M. Rameez, K. Ramesh, L.V. Reddy, S. Saha, R. Sahoo, R. Scaria, S. Shibata, M. Zuberi
Publikováno v:
Journal of Instrumentation. 18:P03046
The GRAPES-3 experiment located in Ooty, India, samples the electron and muon components in extensive air showers using an array of plastic scintillator detectors and a muon telescope (G3MT) consisting of proportional counters to study the compositio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::92f5622394b50e1ebfe5483504b341ce
https://doi.org/10.1088/1748-0221/18/03/p03046
https://doi.org/10.1088/1748-0221/18/03/p03046
Autor:
Pravata Mohanty, S. Ahmad, M. Chakraborty, A. Chandra, S.R Dugad, U.D Goswami, S.K Gupta, B. Hariharan, Y. Hayashi, P. Jagadeesan, A. Jain, 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. Varsid, M. Zuberia
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The GRAPES-3 is a near-equatorial extensive air shower experiment, located in Ooty, India at an altitude of 2200 m above mean sea level. It consists of a dense array of 400 scintillator detectors of 1 m$^{2}$ area each with 8 m inter separation. The
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a7ea46e35d6b866b1c42b6913ae021a3
https://doi.org/10.22323/1.395.0003
https://doi.org/10.22323/1.395.0003
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
L.V. Reddy, F. Varsi, G.S. Pradhan, Yasushi Muraki, S. R. Dugad, M. Rameez, M. Chakraborty, B.P. Pant, Toshiyuki Nonaka, Pankaj Jain, K. Tanaka, K. Ramesh, R. Scaria, S. Mahapatra, Anuj Chandra, Shafiq Ahmad, Y. Hayashi, Akitoshi Oshima, P.S. Rakshe, S.K. Gupta, S. Kawakami, Balakrishnan Hariharan, R. Sahoo, P. Jagadeesan, D. Pattanaik, Hiroshi Kojima, Umananda Dev Goswami, Prakash Kumar Nayak, R. Moharana, P. K. Mohanty, M. Zuberi, A. Jain, Shoichi Shibata
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The GRAPES-3 extensive air shower (EAS) array located at Ooty is equipped with 400 plastic scintillator detectors spread over an area of 25000 m$^2$ and a muon telescope of area 560 m$^2$ built with 3,712 proportional counters. One of its principal o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8460352447f692765b8c89c2c4f03560
https://doi.org/10.22323/1.395.0396
https://doi.org/10.22323/1.395.0396
Autor:
S. Mahapatra, S.K. Gupta, K. Ramesh, J. Soni, M. Rameez, Umananda Dev Goswami, B.P. Pant, P.S. Rakshe, M. Zuberi, Shoichi Shibata, R. Scaria, P. K. Mohanty, K. Tanaka, Toshiyuki Nonaka, G.S. Pradhan, R. Moharana, Hiroshi Kojima, A. Jain, F. Varsi, Prakash Kumar Nayak, R. Sahoo, S. R. Dugad, M. Chakraborty, D. Pattanaik, Shafiq Ahmad, S. Kawakami, L.V. Reddy, Akitoshi Oshima, Balakrishnan Hariharan, Yasushi Muraki, Pankaj Jain, Y. Hayashi, P. Jagadeesan, Anuj Chandra
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The GRAPES-3 experiment located in Ooty consists of an array of 400 plastic scintillator detectors spread over an area of 25000𝑚 2 and a large area (560 𝑚 2 ) muon telescope. Every day, the array records about 3 million showers induced by the i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1cc460edcb02dd904c05f87a05c2b05c
https://doi.org/10.22323/1.395.0394
https://doi.org/10.22323/1.395.0394
Cosmic ray energy spectrum and composition measurements from the GRAPES-3 experiment: Latest results
Autor:
K. Ramesh, P. Jagadeesan, P.S. Rakshe, S. Mahapatra, Yasushi Muraki, M. Zuberi, J. Soni, Y. Hayashi, Pankaj Jain, D. Pattanaik, Umananda Dev Goswami, F. Varsi, S. Kawakami, R. Sahoo, M. Rameez, A. Jain, Toshiyuki Nonaka, Anuj Chandra, Shoichi Shibata, Balakrishnan Hariharan, Shafiq Ahmad, B.P. Pant, P. K. Mohanty, R. Moharana, L.V. Reddy, R. Scaria, S. R. Dugad, M. Chakraborty, Akitoshi Oshima, K. Tanaka, S.K. Gupta, G.S. Pradhan, Hiroshi Kojima, Prakash Kumar Nayak
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The Gamma Ray Astronomy at PeV EnergieS phase-3 (GRAPES-3) experiment is located at Ooty in India (11.4$^{\circ}$ N, 76.7$^{\circ}$ E and 2200 m above m.s.l.). It consists of a densely packed array of 400 plastic scintillator detectors and a large ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::300965479f0f78c10f82ce60395e9bab
https://doi.org/10.22323/1.395.0388
https://doi.org/10.22323/1.395.0388
Autor:
S. Mahapatra, Toshiyuki Nonaka, A. Jain, L.V. Reddy, P. K. Mohanty, S. K. Gupta, M. Zuberi, Yasushi Muraki, Y. Hayashi, Hiroshi Kojima, K. Ramesh, F. Varsi, R. Scaria, K. Tanaka, S. R. Dugad, Umananda Dev Goswami, Akitoshi Oshima, Prakash Kumar Nayak, S. Kawakami, M. Rameez, Anuj Chandra, M. Chakraborty, P. K. Jain, Balakrishnan Hariharan, P.S. Rakshe, G.S. Pradhan, Shafiq Ahmad, P. Jagadeesan, J. Soni, D. Pattanaik, B.P. Pant, R. Sahoo, Shoichi Shibata, R. Moharana
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The deflection of cosmic rays (CRs) in the interstellar magnetic field results in an almost isotropic flux as observed on Earth. However, an anisotropy has been observed at the level of ∼ 10^{-4} − 10^{-3}. The GRAPES-3 experiment located at Ooty
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a6f00ee3d209a50f47407b8b044daf54
https://doi.org/10.22323/1.395.0393
https://doi.org/10.22323/1.395.0393
Autor:
Y. Hayashi, R. Moharana, L.V. Reddy, M. Rameez, Shoichi Shibata, P. K. Mohanty, F. Varsi, J. Soni, R. Scaria, R. Sahoo, Yasushi Muraki, S.K. Gupta, Umananda Dev Goswami, Pankaj Jain, Akitoshi Oshima, M. Zuberi, S. Kawakami, S. Mahapatra, A. Jain, Hiroshi Kojima, Shafiq Ahmad, Prakash Kumar Nayak, D. Pattanaik, K. Tanaka, Toshiyuki Nonaka, Anuj Chandra, S. R. Dugad, M. Chakraborty, G.S. Pradhan, P.S. Rakshe, P. Jagadeesan, Balakrishnan Hariharan, K. Ramesh, B.P. Pant
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The Moon acts as a shield against the cosmic rays, preventing them from reaching the earth, which gives rise to a deficit in the flux along the direction of the Moon. The observed deficit can be used for obtaining the absolute calibration of the angu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d125cd67749ac8031ef427f5f6881565
https://doi.org/10.22323/1.395.0391
https://doi.org/10.22323/1.395.0391