SiPM-based azimuthal position sensor in ANITA-IV Hi-Cal Antarctic balloon experiment
dc.contributor.author | Novikov, A. | |
dc.contributor.author | Besson, David Zeke | |
dc.contributor.author | Chernysheva, I. | |
dc.contributor.author | Dmitrenko, V. V. | |
dc.contributor.author | Grachev, V. M. | |
dc.contributor.author | Petrenko, D. | |
dc.contributor.author | Prohira, Steven | |
dc.contributor.author | Shustov, A. | |
dc.contributor.author | Ulin, S. E. | |
dc.contributor.author | Uteshev, Z. M. | |
dc.contributor.author | Vlasik, K. F. | |
dc.date.accessioned | 2018-10-26T16:14:55Z | |
dc.date.available | 2018-10-26T16:14:55Z | |
dc.date.issued | 2017 | |
dc.identifier.citation | A. Novikov et al 2017 J. Phys.: Conf. Ser. 789 012217 | en_US |
dc.identifier.uri | http://hdl.handle.net/1808/27054 | |
dc.description.abstract | Hi-Cal (High-Altitude Calibration) is a balloon-borne experiment that will be launched in December, 2016 in Antarctica following ANITA-IV (Antarctic Impulsive Transient Antenna) and will generate a broad-band pulse over the frequency range expected from radiation induced by a cosmic ray shower. Here, we describe a device based on an array of silicon photomultipliers (SiPMs) for determination of the azimuthal position of Hi-Cal. The angular resolution of the device is about 3 degrees. Since at the float altitude of ~38 km the pressure will be ~0.5 mbar and temperature ~ − 20 °C, the equipment has been tested in a chamber over a range of corresponding pressures (0.5 ÷ 1000) mbar and temperatures (−40 ÷ +50) °C. | en_US |
dc.publisher | IOP Publishing | en_US |
dc.rights | Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. | en_US |
dc.rights.uri | https://creativecommons.org/licenses/by/3.0/ | en_US |
dc.title | SiPM-based azimuthal position sensor in ANITA-IV Hi-Cal Antarctic balloon experiment | en_US |
dc.type | Article | en_US |
kusw.kuauthor | Novikov, A. | |
kusw.kuauthor | Besson, David Zeke | |
kusw.kudepartment | Physics and Astronomy | en_US |
dc.identifier.doi | 10.1088/1742-6596/798/1/012217 | en_US |
kusw.oaversion | Scholarly/refereed, publisher version | en_US |
kusw.oapolicy | This item meets KU Open Access policy criteria. | en_US |
dc.rights.accessrights | openAccess | en_US |
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Except where otherwise noted, this item's license is described as: Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.