IceCube's in-ice radio extension: Status and results

被引:1
|
作者
Landsman, H. [1 ]
Cheng, E. [1 ]
Kulcyk, E. [1 ]
Laundrie, A. W. [1 ]
Rotter, B. [2 ]
Ruckman, L. [2 ]
Sandstrom, P. W. [1 ]
Varner, G. S. [2 ]
机构
[1] Univ Wisconsin, Dept Phys, Madison, WI 53703 USA
[2] Univ Hawaii, Dept Phys & Astron, Manoa, HI 96822 USA
来源
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2012年 / 662卷
关键词
Neutrino astronomy; Radio frequency; South Pole; GZK neutrinos; Neutrinos detection; Ice properties;
D O I
10.1016/j.nima.2010.11.144
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
In 2006-2010, several radio frequency (RF) detectors and calibration equipment were deployed as part of the IceCube array at depths between 5 and 1400 m in preparation for a future large scale GZK neutrino detector. IceCube's deep holes and well-established data handling system provide a unique opportunity for deep-ice RF detection studies at the South Pole. We will present verification and calibration results as well as a status-review of ongoing analyses such as ice-properties, RF noise and reconstruction algorithms. Published by Elsevier B.V.
引用
收藏
页码:S54 / S58
页数:5
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