Optimization of the Configuration of Askaryan Radio Array Observatory
碩士 === 國立臺灣大學 === 物理研究所 === 100 === Askaryan Radio Array (ARA) is an observatory designed to detect the radio frequency (RF) Cherenkov radiation generated by the shower induced by ultra high energy (UHE) cosmic neutrino whose energy lies between 10^17eV and 10^21eV. Tracing the UHE neutrinos is the...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | zh-TW |
| Published: |
2012
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| Online Access: | http://ndltd.ncl.edu.tw/handle/33531005093298186382 |