Performance and simulation of the RICE detector

被引：88

作者：

Kravchenko, I

Frichter, GM

Seckel, D

Spiczak, GM

Adams, J

Seunarine, S

Allen, C

Bean, A

Besson, D

Box, DJ

Buniy, R

Drees, J

McKay, D

Meyers, J

Perry, L

Ralston, J

Razzaque, S

Schmitz, DW

机构：

[1] MIT, Nucl Sci Lab, Cambridge, MA 02139 USA

[2] Florida State Univ, High Energy Phys, Tallahassee, FL 32306 USA

[3] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA

[4] Univ Canterbury, Dept Phys & Astron, Christchurch, New Zealand

[5] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA

来源：

ASTROPARTICLE PHYSICS | 2003年 / 19卷 / 01期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1016/S0927-6505(02)00194-9

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Radio Ice Cherenkov Experiment at the South Pole, co-deployed with the AMANDA experiment, seeks to detect ultra-high energy electron neutrinos interacting in cold polar ice. Such interactions produce electromagnetic showers, which emit radio-frequency Cherenkov radiation. We describe the experimental apparatus and the procedures used to measure the neutrino flux. (C) 2002 Elsevier Science B.V. All rights reserved.

引用

页码：15 / 36

页数：22

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