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完整後設資料紀錄
DC 欄位 | 值 | 語言 |
---|---|---|
dc.contributor.advisor | 陳丕燊(Pisin Chen) | |
dc.contributor.author | Chih-Ching Chen | en |
dc.contributor.author | 陳志清 | zh_TW |
dc.date.accessioned | 2021-06-15T14:02:15Z | - |
dc.date.available | 2015-08-25 | |
dc.date.copyright | 2015-08-25 | |
dc.date.issued | 2015 | |
dc.date.submitted | 2015-08-20 | |
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dc.identifier.uri | http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/52000 | - |
dc.description.abstract | 本論文探討應用電波技術在超高能文中子的量測。第一部分研究超高能粒子所產生出的切輪可夫輻射行為,並使用有限元素法研究之。第二部分介紹ANITA實驗所利用的偵測方法、儀器設計及物理結果。第三部份介紹ARA天壇陣列實驗的偵測方法、儀器設計及物理結果。最後探討一種分辨超高能微中子味道的方法。 | zh_TW |
dc.description.abstract | In this thesis we study the Cherenkov radiation pulse from ultra-high energy particle shower by a numerical finite-difference time-domain (FDTD) method. Expounding the work on ANITA experiment include detection method, instrument and operation method. The design concept of Askaryan Radio Array (ARA) experiment and the hardware, deploy and operation. We propose our strategy to identify the neutrino flavor in observing cosmogenic neutrinos by radio neutrino telescopes, such as ARA, ARIANNA. | en |
dc.description.provenance | Made available in DSpace on 2021-06-15T14:02:15Z (GMT). No. of bitstreams: 1 ntu-104-D97244002-1.pdf: 18639883 bytes, checksum: 7b11c4b22560023df60a774d09c934d4 (MD5) Previous issue date: 2015 | en |
dc.description.tableofcontents | Contents i
List of Figures iv List of Tables xiv 1 Introduction 1 2 Radiation 3 2.1 CoherentCherenkovradiationpulses . . . . . . . . . . . . . . 3 2.2 Theoreticalconsiderations .................... 7 2.2.1 The one-dimensional approximation . . . . . . . . . . . 7 2.2.2 Thesqueezingeffect ................... 12 2.3 Numericalmethod ........................ 14 2.3.1 Algorithm......................... 15 2.3.2 Simulationsetup ..................... 17 2.4 Simulations ............................ 20 2.4.1 Towardsmorerealisticcases............... 20 2.5 Summary ............................. 29 3 ANITA 32 3.1 ANITAconcept.......................... 32 3.2 ANITA-IIInstrument....................... 36 3.2.1 RFantenna ........................ 37 3.2.2 Front-endsystem ..................... 37 3.2.3 SURF High Occupancy RF Trigger (SHORT) . . . . . 37 3.2.4 Trigger........................... 38 3.2.5 Digitization ........................ 38 3.2.6 Powersystemanddatatransmission . . . . . . . . . . 39 3.2.7 datatransmission..................... 39 3.3 Dataanalysis ........................... 39 3.3.1 SummaryofANITAmissionstodate . . . . . . . . . . 44 3.4 ANITA-IIresult.......................... 45 3.5 ANITA-IIasacosmicraydetector ............... 45 3.6 ANITA-IIasamonopoledetector................ 51 Askaryan Radio Array 55 4.1 TheARAStation......................... 55 4.2 Generaldesign .......................... 56 4.3 PerformanceoftheARAstationsA2andA3. . . . . . . . . . 62 4.4 The calibration of station geometry and timing . . . . . . . . 64 4.5 Signalchaincalibration...................... 68 4.6 Results............................... 72 5 Discrimination between Flavors for Detection of Cosmogenic Neutrinos 77 5.1 Thestrategyofflavoridentification ............... 77 5.2 Simulationforneutrinoevents.................. 79 5.3 Summary ............................. 84 | |
dc.language.iso | en | |
dc.title | 利用電波技術量測超高能微中子及宇宙射線 | zh_TW |
dc.title | The Radio Detection of Ultra High Energy Neutrinos and Cosmic Rays | en |
dc.type | Thesis | |
dc.date.schoolyear | 103-2 | |
dc.description.degree | 博士 | |
dc.contributor.oralexamcommittee | 黃明輝(Ming-Huey Huang),南智佑(Jiwoo Nam),王明儒(Min-Zu Wang),蕭宇劭(Jerry Shiao),陳勁豪(John Chin-Hao Chen) | |
dc.subject.keyword | 微中子,無線電,切倫可夫輻射,計算,超高能粒子, | zh_TW |
dc.subject.keyword | neutrino,radio frequency,Cherenkov radiation,calculation,ultra high energy particle, | en |
dc.relation.page | 93 | |
dc.rights.note | 有償授權 | |
dc.date.accepted | 2015-08-20 | |
dc.contributor.author-college | 理學院 | zh_TW |
dc.contributor.author-dept | 天文物理研究所 | zh_TW |
顯示於系所單位: | 天文物理研究所 |
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