請用此 Handle URI 來引用此文件:
http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/32172
完整後設資料紀錄
DC 欄位 | 值 | 語言 |
---|---|---|
dc.contributor.advisor | 王名儒(Min-Zu Wang) | |
dc.contributor.author | Kuei-Ling Hung | en |
dc.contributor.author | 洪桂苓 | zh_TW |
dc.date.accessioned | 2021-06-13T03:35:02Z | - |
dc.date.available | 2006-08-03 | |
dc.date.copyright | 2006-08-03 | |
dc.date.issued | 2006 | |
dc.date.submitted | 2006-07-26 | |
dc.identifier.citation | [1] Kai Auber. Neutrino Physics. The Insitute of Physics, London, 2004.
[2] David Berge. Development of an Algorithm for the Shower Reconstruction with the H.E.S.S. Telescope System. PhD thesis, HumboldtUniversity in Berlin, 2002. [3] S. Eidelman et al. Particle data group. Phys. Lett., B(592), 2004. [4] Y.S. Velikzhanin et al. Design of a general purpose data collection module for the nutel telescope. Nuclear Instruments and Methods in Physics Research, A(552):477-488, 2005. [5] HAMAMATSU. PHOTOMULTIPLIER TUBES Basic and Applications [6] HAMAMATSU. MULTIANODE PHOTOMULTIPLIER TUBE ASSEMBLY H7546, Sept. 2000. [7] Eugene Hecht. OPTICS, chapter 6.3, pages 253-273. Addison Wesley, 2002. [8] D. Heck and T. Pierog. Extensive Air Shower Simiulation with CORSIKA: A user's Guide (Version 6.500 from March 6, 2006). [9] David Kincaid and Ward Cheney. Numerical Analysis: Methematics of Scientific Computing, chapter 4.4, pages 186-191. Wadsworth Group, 2001. | |
dc.identifier.uri | http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/32172 | - |
dc.description.abstract | Abstract
NuTel is an experiment to observe the ultra-high energy cosmic tau neutrinos with the earth skimming technique. Mountains are used as targets to convert tau neutrinos to tau leptons and also as a filter to block cosmic ray backgrounds. The signature of a high energy tau is an air shower that originates from the mountains or the ground. NuTel is designed to observed the Cherenkov in such air showers. The optical and electronic systems of NuTel have been designed and are being built and tested. A simulation program to describe both the optics and the electronics is developed. Based on the simulated photo-image, the energy and inicident angle of the shower can be determined by a reconstruction program, which also handles background filtering and desaturation. It is found that the simple and rough filter produces the largest error due to loss of accuracy in position and amplitudes. | en |
dc.description.provenance | Made available in DSpace on 2021-06-13T03:35:02Z (GMT). No. of bitstreams: 1 ntu-95-R93222003-1.pdf: 1123289 bytes, checksum: 98dfd384e30ee1a4468183299741af0d (MD5) Previous issue date: 2006 | en |
dc.description.tableofcontents | Contents
1 Introduction 5 1.1 Ultra-High Energy Cosmic Neutrino . . . . . . . . . . . . . . . . . . . . . . . 5 1.2 Earth-Skimming Technique . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 1.3 Organization of the Thesis . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7 2 The NuTel Telescope Apparatus 9 2.1 The Optical System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10 2.2 Multi-Anode Photomultiplier Tube (MAPMT) . . . . . . . . . . . . . . . . . 10 2.3 Charge Sharing Board (CSB) . . . . . . . . . . . . . . . . . . . . . . . . . . 11 2.4 Preamplifier . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12 2.5 Data Collection Module (DCM) . . . . . . . . . . . . . . . . . . . . . . . . . 13 2.6 Night Sky Background . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15 3 Simulation 17 3.1 CORSIKA . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19 3.2 The Optical System . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21 3.2.1 Focusing Device . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21 3.2.2 Light Guide . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23 3.3 Multi-Anode Photomultiplier Tubes (MAPMTs) . . . . . . . . . . . . . . . . 23 3.3.1 Transform Photon to Photoelectron . . . . . . . . . . . . . . . . . . . 24 3.3.2 Transform Photoelectrons to Charges . . . . . . . . . . . . . . . . . . 24 3.4 Charge Sharing Board (CSB) . . . . . . . . . . . . . . . . . . . . . . . . . . 24 3.5 Preamplifer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25 3.6 Data Collection Module (DCM) . . . . . . . . . . . . . . . . . . . . . . . . . 27 3.7 Trigger . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 27 3.8 Background Mixer . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 27 3 4 CONTENTS 3.9 Simulation Result . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28 4 Reconstruction 31 4.1 Detector Reconstruction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31 4.1.1 Desaturate . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 32 4.1.2 Filter Out Noise and Background . . . . . . . . . . . . . . . . . . . . 33 4.1.3 DCM Reconstruction . . . . . . . . . . . . . . . . . . . . . . . . . . . 33 4.1.4 Direction Reconstruction . . . . . . . . . . . . . . . . . . . . . . . . . 40 4.1.5 Result of Telescope Reconstruction . . . . . . . . . . . . . . . . . . . 41 4.2 Shower Reconstruction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47 4.2.1 Shower Maximum Position . . . . . . . . . . . . . . . . . . . . . . . . 50 4.2.2 Shower Energy . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51 4.3 Total Reconstruction Result . . . . . . . . . . . . . . . . . . . . . . . . . . . 58 4.4 Conclustion of Reconstruction . . . . . . . . . . . . . . . . . . . . . . . . . . 62 A Parameters in calib.db 63 B Classes 65 B.1 Devices . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 65 B.2 Data . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 67 | |
dc.language.iso | en | |
dc.title | 微中子望遠鏡之電子系統模擬與影像重建 | zh_TW |
dc.title | Simulation of the Electronic System and Shower Reconstruction for the NuTel Telescope | en |
dc.type | Thesis | |
dc.date.schoolyear | 94-2 | |
dc.description.degree | 碩士 | |
dc.contributor.coadvisor | 葉平(Ping Yeh),上野耕資(Koji Ueno) | |
dc.contributor.oralexamcommittee | 侯維恕(Wei-Shu Hou),張寶棣(Paoti Chang) | |
dc.subject.keyword | 微中子, | zh_TW |
dc.subject.keyword | NuTel,neutrino, | en |
dc.relation.page | 69 | |
dc.rights.note | 有償授權 | |
dc.date.accepted | 2006-07-27 | |
dc.contributor.author-college | 理學院 | zh_TW |
dc.contributor.author-dept | 物理研究所 | zh_TW |
顯示於系所單位: | 物理學系 |
文件中的檔案:
檔案 | 大小 | 格式 | |
---|---|---|---|
ntu-95-1.pdf 目前未授權公開取用 | 1.1 MB | Adobe PDF |
系統中的文件,除了特別指名其著作權條款之外,均受到著作權保護,並且保留所有的權利。