Add to ORKGRICE is designed to detect ultrahigh energy (>100 TeV) neutrinos from astrophysical sources. It will consist of an array of compact radio (100 to 1000 MHz) receivers buried in ice at the South Pole. During the 1995-96 and 1996-97 austral summers, several receivers transmitters were deployed in bore holes drilled for the AMANDA project, at depths of 141 to 260 m. This was the first in situ test of radio receivers in deep ice for neutrino astronomy
Since the early 1990s, the South Pole has been the site of the construction of the world's first und...
We report on studies of the viability and sensitivity of the Askaryan Radio Array (ARA), a new initi...
The flux and cross section of high energy neutrinos is an active area of research. Due to the expect...
The RICE experiment seeks observation of ultra-high energy (UHE; Ev \u3e 1017 eV) neutrinos interact...
Thesis (M.S.)--University of Hawaii at Manoa, 2007.Includes bibliographical references (leaves 47-49...
Ph.D. University of Hawaii at Manoa 2010.Includes bibliographical references.This work describes a s...
The Askaryan Radio Array (ARA) is an ultra-high energy (>1017>1017 eV) cosmic neutrino detector in p...
High energy astrophysical neutrinos are useful for understanding the origins of high energy cosmic r...
IceCube is currently being built deep in the glacial ice beneath the South Pole. In its second year ...
We present a compilation of recent results, submitted to the 2003 International Cosmic Ray Conferenc...
Radio Cherenkov radiation is arguably the most efficient mechanism for detecting showers from ultra-...
The AMANDA neutrino detector has been in operation at the South Pole for several years. A number of ...
The Radio Ice Cherenkov Experiment(RICE) located at the South Pole, is designed to detect the cohere...
Ultra-high energy (UHE) neutrinos are a promising messenger particle, and their discovery would be a...
The sensitivity of an ice radiowave detector to the anticipated high energy neutrino fluxes is calcu...
Since the early 1990s, the South Pole has been the site of the construction of the world's first und...
We report on studies of the viability and sensitivity of the Askaryan Radio Array (ARA), a new initi...
The flux and cross section of high energy neutrinos is an active area of research. Due to the expect...
The RICE experiment seeks observation of ultra-high energy (UHE; Ev \u3e 1017 eV) neutrinos interact...
Thesis (M.S.)--University of Hawaii at Manoa, 2007.Includes bibliographical references (leaves 47-49...
Ph.D. University of Hawaii at Manoa 2010.Includes bibliographical references.This work describes a s...
The Askaryan Radio Array (ARA) is an ultra-high energy (>1017>1017 eV) cosmic neutrino detector in p...
High energy astrophysical neutrinos are useful for understanding the origins of high energy cosmic r...
IceCube is currently being built deep in the glacial ice beneath the South Pole. In its second year ...
We present a compilation of recent results, submitted to the 2003 International Cosmic Ray Conferenc...
Radio Cherenkov radiation is arguably the most efficient mechanism for detecting showers from ultra-...
The AMANDA neutrino detector has been in operation at the South Pole for several years. A number of ...
The Radio Ice Cherenkov Experiment(RICE) located at the South Pole, is designed to detect the cohere...
Ultra-high energy (UHE) neutrinos are a promising messenger particle, and their discovery would be a...
The sensitivity of an ice radiowave detector to the anticipated high energy neutrino fluxes is calcu...
Since the early 1990s, the South Pole has been the site of the construction of the world's first und...
We report on studies of the viability and sensitivity of the Askaryan Radio Array (ARA), a new initi...
The flux and cross section of high energy neutrinos is an active area of research. Due to the expect...