Observation of the Askaryan effect in ice with the ANITA experiment

Thesis (M.S.)--University of Hawaii at Manoa, 2007. Includes bibliographical references (leaves 47-49). xvi, 49 leaves, bound ill. (some col.) 29 cm First hypothesized by Gurgen Askaryan in the 1960's and later confirmed in 2001 at SLAC (Stanford Linear Accelerator Center), radio Cherenkov dete...

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Main Author: Kowalski, Richard Jeffrey
Format: Thesis
Language:English
Published: 2007
Subjects:
Online Access:http://hdl.handle.net/10125/20831
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record_format openpolar
spelling ftunivhawaiimano:oai:scholarspace.manoa.hawaii.edu:10125/20831 2023-07-30T03:59:19+02:00 Observation of the Askaryan effect in ice with the ANITA experiment Kowalski, Richard Jeffrey 2007 application/pdf http://hdl.handle.net/10125/20831 en-US eng Theses for the degree of Master of Science (University of Hawaii at Manoa). Physics; no. 4211 http://hdl.handle.net/10125/20831 All UHM dissertations and theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission from the copyright owner. Ice -- Effect of radiation on Cherenkov counters Neutrino interactions Thesis Text 2007 ftunivhawaiimano 2023-07-15T22:27:47Z Thesis (M.S.)--University of Hawaii at Manoa, 2007. Includes bibliographical references (leaves 47-49). xvi, 49 leaves, bound ill. (some col.) 29 cm First hypothesized by Gurgen Askaryan in the 1960's and later confirmed in 2001 at SLAC (Stanford Linear Accelerator Center), radio Cherenkov detection techniques are possible in the ultra-high energy regime (1018 -> 1022 eV) while observing electromagnetic cascades in dielectric media. This method of detection has now moved into the field of neutrino astrophysics. Recently, the interest in using ice as a dielectric medium to observe coherent microwave Cherenkov pulses from ultra-high energy neutrino induced particle showers has grown considerably with advances from experiments such as RICE, FORTE, and ANITA-lite. ANITA (ANtarctic Impulsive Transient Antenna), is a radio telescope designed to exploit this effect while looking for UHE neutrino interactions in Antarctic ice. In June 2006, ANITA observed these highly coherent radio impulses in SLAC's ESA (End Station A) with 28.5 GeV electrons interacting with a 7.5 tonne ice target to produce the EM shower. These first measurements of the Askaryan effect in ice were consistent with shower and electrodynamics simulations for ice and provided a clear indication that the radiation is coherent over the 200-1200 MHz frequency window. In addition to the ANITA payload in SLAC's ESA, four log-period dipole array antennas, two monocone antennas, and one high frequency gain horn (nominally 2.6-3.95 GHz) recorded impulsive events emanating from the ice target. I report on further analysis of coherent radio Cherenkov impulses using the standard gain horn and demonstrate that the results are fully consistent with theoretical expectations. Thesis Antarc* Antarctic ScholarSpace at University of Hawaii at Manoa Antarctic
institution Open Polar
collection ScholarSpace at University of Hawaii at Manoa
op_collection_id ftunivhawaiimano
language English
topic Ice -- Effect of radiation on
Cherenkov counters
Neutrino interactions
spellingShingle Ice -- Effect of radiation on
Cherenkov counters
Neutrino interactions
Kowalski, Richard Jeffrey
Observation of the Askaryan effect in ice with the ANITA experiment
topic_facet Ice -- Effect of radiation on
Cherenkov counters
Neutrino interactions
description Thesis (M.S.)--University of Hawaii at Manoa, 2007. Includes bibliographical references (leaves 47-49). xvi, 49 leaves, bound ill. (some col.) 29 cm First hypothesized by Gurgen Askaryan in the 1960's and later confirmed in 2001 at SLAC (Stanford Linear Accelerator Center), radio Cherenkov detection techniques are possible in the ultra-high energy regime (1018 -> 1022 eV) while observing electromagnetic cascades in dielectric media. This method of detection has now moved into the field of neutrino astrophysics. Recently, the interest in using ice as a dielectric medium to observe coherent microwave Cherenkov pulses from ultra-high energy neutrino induced particle showers has grown considerably with advances from experiments such as RICE, FORTE, and ANITA-lite. ANITA (ANtarctic Impulsive Transient Antenna), is a radio telescope designed to exploit this effect while looking for UHE neutrino interactions in Antarctic ice. In June 2006, ANITA observed these highly coherent radio impulses in SLAC's ESA (End Station A) with 28.5 GeV electrons interacting with a 7.5 tonne ice target to produce the EM shower. These first measurements of the Askaryan effect in ice were consistent with shower and electrodynamics simulations for ice and provided a clear indication that the radiation is coherent over the 200-1200 MHz frequency window. In addition to the ANITA payload in SLAC's ESA, four log-period dipole array antennas, two monocone antennas, and one high frequency gain horn (nominally 2.6-3.95 GHz) recorded impulsive events emanating from the ice target. I report on further analysis of coherent radio Cherenkov impulses using the standard gain horn and demonstrate that the results are fully consistent with theoretical expectations.
format Thesis
author Kowalski, Richard Jeffrey
author_facet Kowalski, Richard Jeffrey
author_sort Kowalski, Richard Jeffrey
title Observation of the Askaryan effect in ice with the ANITA experiment
title_short Observation of the Askaryan effect in ice with the ANITA experiment
title_full Observation of the Askaryan effect in ice with the ANITA experiment
title_fullStr Observation of the Askaryan effect in ice with the ANITA experiment
title_full_unstemmed Observation of the Askaryan effect in ice with the ANITA experiment
title_sort observation of the askaryan effect in ice with the anita experiment
publishDate 2007
url http://hdl.handle.net/10125/20831
geographic Antarctic
geographic_facet Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_relation Theses for the degree of Master of Science (University of Hawaii at Manoa). Physics; no. 4211
http://hdl.handle.net/10125/20831
op_rights All UHM dissertations and theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission from the copyright owner.
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