Calibration of TA surface detectors

T. Nonaka, D. Ikeda, E. Kido, K. Miyata, H. Ohoka, T. Okuda, Shunsuke Ozawa, H. Sagawa, N. Sakurai, M. Takeda, T. Tomida, Y. Yamakawa

Research output: Chapter in Book/Report/Conference proceedingConference contribution

7 Citations (Scopus)

Abstract

The surface detector of Telescope Array(TA) experiment are deployed in desert of western utah,USA. The detector consists of two layers of plastic scintillators of 3m2 area with wave length shifter fiber(WLSfiber). There are 2 PMTs and each PMT is connected with fibers from corresponding layer. To check PMT linearity, 2 LEDs are equipped for each layer. To estimate no of shower particles with good accuracy,it is needed to know the response for 1 minimum ionization particle and monitoring the environmental effect on it. And PMT linearity are also needed to be monitored and calibrated. Here we report observed variation on detector response and its calibration. And the result of linearity check with LEDs also will be reported.

Original languageEnglish
Title of host publicationProceedings of the 30th International Cosmic Ray Conference, ICRC 2007
PublisherUniversidad Nacional Autonoma de Mexico
Pages1005-1008
Number of pages4
Volume5
EditionHE PART 2
Publication statusPublished - 2007
Externally publishedYes
Event30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico
Duration: 2007 Jul 32007 Jul 11

Other

Other30th International Cosmic Ray Conference, ICRC 2007
CountryMexico
CityMerida, Yucatan
Period07/7/307/7/11

Fingerprint

linearity
telescopes
detectors
light emitting diodes
fibers
deserts
showers
scintillation counters
plastics
ionization
estimates

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Cite this

Nonaka, T., Ikeda, D., Kido, E., Miyata, K., Ohoka, H., Okuda, T., ... Yamakawa, Y. (2007). Calibration of TA surface detectors. In Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007 (HE PART 2 ed., Vol. 5, pp. 1005-1008). Universidad Nacional Autonoma de Mexico.

Calibration of TA surface detectors. / Nonaka, T.; Ikeda, D.; Kido, E.; Miyata, K.; Ohoka, H.; Okuda, T.; Ozawa, Shunsuke; Sagawa, H.; Sakurai, N.; Takeda, M.; Tomida, T.; Yamakawa, Y.

Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007. Vol. 5 HE PART 2. ed. Universidad Nacional Autonoma de Mexico, 2007. p. 1005-1008.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Nonaka, T, Ikeda, D, Kido, E, Miyata, K, Ohoka, H, Okuda, T, Ozawa, S, Sagawa, H, Sakurai, N, Takeda, M, Tomida, T & Yamakawa, Y 2007, Calibration of TA surface detectors. in Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007. HE PART 2 edn, vol. 5, Universidad Nacional Autonoma de Mexico, pp. 1005-1008, 30th International Cosmic Ray Conference, ICRC 2007, Merida, Yucatan, Mexico, 07/7/3.
Nonaka T, Ikeda D, Kido E, Miyata K, Ohoka H, Okuda T et al. Calibration of TA surface detectors. In Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007. HE PART 2 ed. Vol. 5. Universidad Nacional Autonoma de Mexico. 2007. p. 1005-1008
Nonaka, T. ; Ikeda, D. ; Kido, E. ; Miyata, K. ; Ohoka, H. ; Okuda, T. ; Ozawa, Shunsuke ; Sagawa, H. ; Sakurai, N. ; Takeda, M. ; Tomida, T. ; Yamakawa, Y. / Calibration of TA surface detectors. Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007. Vol. 5 HE PART 2. ed. Universidad Nacional Autonoma de Mexico, 2007. pp. 1005-1008
@inproceedings{32c3b1351a654270a55400e373b7d497,
title = "Calibration of TA surface detectors",
abstract = "The surface detector of Telescope Array(TA) experiment are deployed in desert of western utah,USA. The detector consists of two layers of plastic scintillators of 3m2 area with wave length shifter fiber(WLSfiber). There are 2 PMTs and each PMT is connected with fibers from corresponding layer. To check PMT linearity, 2 LEDs are equipped for each layer. To estimate no of shower particles with good accuracy,it is needed to know the response for 1 minimum ionization particle and monitoring the environmental effect on it. And PMT linearity are also needed to be monitored and calibrated. Here we report observed variation on detector response and its calibration. And the result of linearity check with LEDs also will be reported.",
author = "T. Nonaka and D. Ikeda and E. Kido and K. Miyata and H. Ohoka and T. Okuda and Shunsuke Ozawa and H. Sagawa and N. Sakurai and M. Takeda and T. Tomida and Y. Yamakawa",
year = "2007",
language = "English",
volume = "5",
pages = "1005--1008",
booktitle = "Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007",
publisher = "Universidad Nacional Autonoma de Mexico",
edition = "HE PART 2",

}

TY - GEN

T1 - Calibration of TA surface detectors

AU - Nonaka, T.

AU - Ikeda, D.

AU - Kido, E.

AU - Miyata, K.

AU - Ohoka, H.

AU - Okuda, T.

AU - Ozawa, Shunsuke

AU - Sagawa, H.

AU - Sakurai, N.

AU - Takeda, M.

AU - Tomida, T.

AU - Yamakawa, Y.

PY - 2007

Y1 - 2007

N2 - The surface detector of Telescope Array(TA) experiment are deployed in desert of western utah,USA. The detector consists of two layers of plastic scintillators of 3m2 area with wave length shifter fiber(WLSfiber). There are 2 PMTs and each PMT is connected with fibers from corresponding layer. To check PMT linearity, 2 LEDs are equipped for each layer. To estimate no of shower particles with good accuracy,it is needed to know the response for 1 minimum ionization particle and monitoring the environmental effect on it. And PMT linearity are also needed to be monitored and calibrated. Here we report observed variation on detector response and its calibration. And the result of linearity check with LEDs also will be reported.

AB - The surface detector of Telescope Array(TA) experiment are deployed in desert of western utah,USA. The detector consists of two layers of plastic scintillators of 3m2 area with wave length shifter fiber(WLSfiber). There are 2 PMTs and each PMT is connected with fibers from corresponding layer. To check PMT linearity, 2 LEDs are equipped for each layer. To estimate no of shower particles with good accuracy,it is needed to know the response for 1 minimum ionization particle and monitoring the environmental effect on it. And PMT linearity are also needed to be monitored and calibrated. Here we report observed variation on detector response and its calibration. And the result of linearity check with LEDs also will be reported.

UR - http://www.scopus.com/inward/record.url?scp=84862789668&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84862789668&partnerID=8YFLogxK

M3 - Conference contribution

VL - 5

SP - 1005

EP - 1008

BT - Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007

PB - Universidad Nacional Autonoma de Mexico

ER -