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dc.contributor.advisorBeatty, James
dc.creatorWilliams, Christopher
dc.date.accessioned2008-05-27T20:17:43Z
dc.date.available2008-05-27T20:17:43Z
dc.date.issued2008-06
dc.identifier.urihttp://hdl.handle.net/1811/32110
dc.description.abstractThe Antarctic Impulsive Transient Antenna (ANITA) is a balloon-borne experiment that flew for 35 days in the 2006/07 austral summer looking for ultra-high energy neutrinos (10^18-10^20eV) interacting within the Antarctic ice. These ultra-high energy neutrinos are believed to be produced primarily through cosmic ray attenuation by the Cosmic Microwave Background (CMB) via the Greisen-Zatsepin-Kuzmin (GZK) mechanism. This research serves as a study of the observed radio background over the 1GHz (200MHz-1.2GHz) band that ANITA was sensitive to. We look for significant anthropogenic noise anomalies as well as confirmation of a thermal noise background. Radio noise from the sun and galactic center is also observed and confirmed to match predicted values. Analysis of the sun/galactic center radio noise was done using pointing software based on the payload's spatial location given by onboard GPS. We also study the synchronization of the on-board calibration pulsing antennas with the instrument's triggering system. This is necessary to confirm that events observed by hardware triggering have correctly matching information provided by software.en_US
dc.language.isoen_USen_US
dc.publisherThe Ohio State Universityen_US
dc.relation.ispartofseriesThe Ohio State University. Department of Physics Honors Theses; 2008en_US
dc.subjectNeutrino Astrophysicsen_US
dc.subjectCosmic Raysen_US
dc.titleA Calibration Study of the ANITA Instrumenten_US
dc.typeThesisen_US
dc.description.embargoNo embargoen_US
dc.rights.ccAttribution-NoDerivs 3.0 Unporteden_US
dc.rights.ccurihttp://creativecommons.org/licenses/by-nd/3.0/en_US


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