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 language | English |
|---|---|
| Title of host publication | Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007 |
| Publisher | Universidad Nacional Autonoma de Mexico |
| Pages | 1005-1008 |
| Number of pages | 4 |
| Volume | 5 |
| Edition | HE PART 2 |
| Publication status | Published - 2007 |
| Externally published | Yes |
| Event | 30th International Cosmic Ray Conference, ICRC 2007 - Merida, Yucatan, Mexico Duration: 2007 Jul 3 → 2007 Jul 11 |
Other
| Other | 30th International Cosmic Ray Conference, ICRC 2007 |
|---|---|
| Country | Mexico |
| City | Merida, Yucatan |
| Period | 07/7/3 → 07/7/11 |
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ASJC Scopus subject areas
- Nuclear and High Energy Physics
Cite this
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 proceeding › Conference contribution
}
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
AN - SCOPUS:84862789668
VL - 5
SP - 1005
EP - 1008
BT - Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007
PB - Universidad Nacional Autonoma de Mexico
ER -