ANTARES 中微子望远镜的定位系统
天体物理仪器与方法
2015-06-04 v3 高能天体物理现象
摘要
ANTARES 中微子望远镜位于地中海土伦海岸外 40 公里处，锚定深度约 2475 米，由 12 条探测线组成，每条线通常配备 25 层。每层携带三个光学模块，用于探测由中微子相互作用产生的带电次级粒子（通常是 μ 子）所激发的切伦科夫光。由于这些线是柔性结构，固定在海底并由浮标拉紧，海流会导致线移动和层旋转。了解光学模块的位置精度优于 10 厘米对于粒子径迹的良好重建至关重要。本文描述了 ANTARES 定位系统。它包括一个用于距离三角测量的声学定位系统和一个用于测量层方向和倾斜度的罗盘-倾斜仪系统。讨论了必要的校正，并描述了探测器对准程序的结果。
引用
@article{arxiv.1202.3894,
title = {The Positioning System of the ANTARES Neutrino Telescope},
author = {S. Adrián-Martínez and M. Ageron and J. A. Aguilar and I. Al Samarai and A. Albert and M. André and M. Anghinolfi and G. Anton and S. Anvar and M. Ardid and A. C. Assis Jesus and T. Astraatmadja and J. -J. Aubert and B. Baret and S. Basa and V. Bertin and S. Biagi and A. Bigi and C. Bigongiari and C. Bogazzi and M. Bou-Cabo and B. Bouhou and M. C. Bouwhuis and J. Brunner and J. Busto and F. Camarena and A. Capone and C. Carloganu and G. Carminati and J. Carr and S. Cecchini and Z. Charif and Ph. Charvis and T. Chiarusi and M. Circella and R. Coniglione and H. Costantini and P. Coyle and C. Curtil and G. De Bonis and M. P. Decowski and I. Dekeyser and A. Deschamps and C. Distefano and C. Donzaud and D. Dornic and Q. Dorosti and D. Drouhin and T. Eberl and U. Emanuele and A. Enzenhöfer and J. -P. Ernenwein and S. Escoffier and P. Fermani and M. Ferri and V. Flaminio and F. Folger and U. Fritsch and J. -L. Fuda and S. Galatá and P. Gay and G. Giacomelli and V. Giordano and J. P. Gómez-González and K. Graf and G. Guillard and G. Halladjian and G. Hallewell and H. van Haren and J. Hartman and A. J. Heijboer and Y. Hello and J. J. Hernández-Rey and B. Herold and J. Hößl and C. C. Hsu and M. de Jong and M. Kadler and O. Kalekin and A. Kappes and U. Katz and O. Kavatsyuk and P. Keller and P. Kooijman and C. Kopper and A. Kouchner and I. Kreykenbohm and V. Kulikovskiy and R. Lahmann and P. Lamare and G. Larosa and D. Lattuada and D. Lefévre and A. Le Van Suu and G. Lim and D. Lo Presti and H. Loehner and S. Loucatos and S. Mangano and M. Marcelin and A. Margiotta and J. A. Martínez-Mora and A. Meli and T. Montaruli and L. Moscoso and H. Motz and M. Neff and E. Nezri and V. Niess and D. Palioselitis and G. E. Păvălaş and K. Payet and P. Payre and J. Petrovic and P. Piattelli and N. Picot-Clemente and V. Popa and T. Pradier and E. Presani and C. Racca and D. Real and C. Reed and G. Riccobene and C. Richardt and R. Richter and C. Rivière and A. Robert and K. Roensch and A. Rostovtsev and J. Ruiz-Rivas and M. Rujoiu and G. V. Russo and F. Salesa and D. F. E. Samtleben and F. Schöck and J. -P. Schuller and F. Schüssler and T. Seitz and R. Shanidze and F. Simeone and A. Spies and M. Spurio and J. J. M. Steijger and Th. Stolarczyk and A. Sánchez-Losa and M. Taiuti and C. Tamburini and S. Toscano and B. Vallage and V. Van Elewyck and G. Vannoni and M. Vecchi and P. Vernin and S. Wagner and G. Wijnker and J. Wilms and E. de Wolf and H. Yepes and D. Zaborov and J. D. Zornoza and J. Zúñiga},
journal= {arXiv preprint arXiv:1202.3894},
year = {2015}
}