The Calibration of the Geometry and Antenna Delay in Askaryan Radio Array Station 4 and 5статья (материалы конференций)
Аннотация: The Askaryan Radio Array (ARA) experiment at the South Pole is designed to detect the radio signals produced by ultra high energy cosmic neutrino interactions in the ice. There are 5 independent ARA stations, one of which (A5) includes a low-threshold phased array trigger string. Each ARA station is designed to work as an autonomous detector. The Data Acquisition System in all ARA stations is equipped with the Ice Ray Sampler second-generation (IRS2) chip, a custom-made, application-specific integrated circuit (ASIC) for high-speed sampling and digitization. In this contribution, we describe the methodology used to calibrate the IRS2 digitizer chip and the station geometry, namely the relative timing between each pair of ARA antennas, deployed at 200 m below the Antarctic ice surface, and their geometrical positions in the ice, for ARA stations 4 and 5. Our calibration allows for proper timing correlations between incoming signals, which is crucial for radio vertex reconstruction and thus detection of ultra high energy neutrinos through the Askaryan effect. We achieve a signal timing precision on a sub-nanosecond level and an antenna position precision within 10 cm.
Год издания: 2021
Авторы: P. Dasgupta, K. Hughes, M. Beheler-Amass, P. Dasgupta, M.-H. A. Huang, P. Allison, S. Archambault, J. J. Beatty, Dominique Besson, M. Beydler, C.H. Chen, P. Chen, Yanbang Chen, B. A. J. Clark, W. Clay, A. Connolly, L. Cremonesi, J. Davies, Keesjan de Vries, C. Deaconu, J. Flaherty, E. Friedman, R. Gaïor, K. Hanson, N. Harty, B. Clifford Hendricks, K. D. Hoffman, Benjamin Hokanson-Fasig, E. Hong, S.Y. Hsu, Jinjer Huang, M.-H. A. Huang, K. Hughes, A. Ishihara, A. Karle, J. L. Kelley, Raghav Khandelwal, K.-C. Kim, M.-C. Kim, Ryan Krebs, I. Kravchenko, Y. Ku, Colin Kuo, K. Kurusu, Uzair Abdul Latif, A. Laundrie, H. Landsman, Mingyu Lu, T.-C. Liu, B. Madison, K. Mase, T. Meures, Ju-Yeol Nam, А. В. Новиков, R. Nichol, Guy Nir, A. Nozdrina, E. Oberla, A. O’Murchadha, John W. Osborn, Yunxiang Pan, C. Pfendner, N. Punsuebsay, J. D. Roth, P. Sandstrom, D. Seckel, Y.-S. Shiao, A. Shultz, D. J.B. Smith, João Paulo N. Torres, S. Toscano, J. Touart, N. van Eijndhoven, Gary Varner, A. G. Vieregg, Minghuan Wang, S.-H. Wang, Y.H. Wang, Stephanie Wissel, Chao Xie, R. D. Young, S. Yoshida, M Beheler Amass, Simon De Kockere, M. A. DuVernois, J. Hanson
Источник: Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)
Ключевые слова: Astrophysics and Cosmic Phenomena, Radio Astronomy Observations and Technology, Scientific Research and Discoveries
Другие ссылки: Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) (PDF)
Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) (HTML)
UCL Discovery (University College London) (PDF)
UCL Discovery (University College London) (HTML)
UCL Discovery (University College London) (HTML)
Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) (HTML)
UCL Discovery (University College London) (PDF)
UCL Discovery (University College London) (HTML)
UCL Discovery (University College London) (HTML)
Открытый доступ: hybrid
Страницы: 1086–1086