A radio air shower detector as an extension for IceCube and IceTop
نویسندگان
چکیده
منابع مشابه
30TH INTERNATIONAL COSMIC RAY CONFERENCE A radio air shower surface detector as an extension for IceCube and IceTop
The IceCube neutrino detector is built into the Antarctic ice sheet at the South Pole to measure high energy neutrinos. For this, 4800 photomultiplier tubes (PMTs) are being deployed at depths between 1450 and 2450 meters into the ice to measure neutrino induced charged particles like muons. IceTop is a surface air shower detector consisting of 160 Cherenkov ice tanks located on top of IceCube....
متن کاملCosmic Ray Results from the IceTop Air Shower Array
IceTop, the surface component of the IceCube neutrino telescope at the South Pole, is an air-shower array which will finally consist of 160 ice Cherenkov tanks at 80 stations spread over an area of 1 km. Currently 40 stations are deployed and taking data. The detector is designed to cover the energy range above the knee up to about 10 eV and study the mass composition of primary cosmic rays. In...
متن کاملAURA - A radio frequency extension to IceCube
The excellent radio frequency transparency of cold polar ice, combined with the coherent Cherenkov emission produced by neutrinoinduced showers when viewed at wavelengths longer than a few centimeters, has spurred considerable interest in a large-scale radiowave neutrino detector array. The AURA (Askaryan Under-ice Radio Array) experimental effort, within the IceCube collaboration, seeks to tak...
متن کاملIceRay: An IceCube-centered Radio-Čerenkov GZK Neutrino Detector
We discuss design considerations and simulation results for IceRay, a proposed large-scale ultra-high energy (UHE) neutrino detector at the South Pole. The array is designed to detect the coherent Askaryan radio emission from UHE neutrino interactions in the ice, with the goal of detecting the cosmogenic neutrino flux with reasonable event rates. Operating in coincidence with the IceCube neutri...
متن کاملIceTop - Cosmic Ray Physics with IceCube
The IceCube experiment at South Pole consists of two detector components the IceTop air shower array on the surface and the neutrino telescope at depths from 1450 to 2450 meters below. Currently, 26 IceTop stations and 22 InIce strings are deployed. With the present size of the IceTop array, it is possible to measure cosmic rays with energies ranging from 0.5 PeV to 100 PeV. Coincident events b...
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ژورنال
عنوان ژورنال: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
سال: 2009
ISSN: 0168-9002
DOI: 10.1016/j.nima.2009.03.179