請用此 Handle URI 來引用此文件：
http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/28159完整後設資料紀錄
| DC 欄位 | 值 | 語言 |
|---|---|---|
| dc.contributor.advisor | 王名儒 | |
| dc.contributor.author | Kun-Xian Huang | en |
| dc.contributor.author | 黃坤賢 | zh_TW |
| dc.date.accessioned | 2021-06-13T00:01:53Z | - |
| dc.date.available | 2007-09-01 | |
| dc.date.copyright | 2007-07-31 | |
| dc.date.issued | 2007 | |
| dc.date.submitted | 2007-07-30 | |
| dc.identifier.citation | [1] Current Aspects of Neutrino Physics, Chapter 3, David O. Caldwell,
2001. [2] Neutrino Physics, Chapter12, Kai Zuber, 2004. [3] P. Bhattacharjee & G. Sigl. [arXiv:astro-ph/9811011] [4] Revised by T.K. Gaisser and T. Stanev, Physics Letters B, Vol. 592, 233, (2004) [5] Enrich Fermi, Physical Review, Vol. 75, Number 8, 1169, (1949) [6] Gamma-ray Burst Real-time Sky map. http://grb.sonoma.edu/index.php [7] E. Waxman, 33rd annual European Physical Society Conference, Rome, 2006. [arXiv:astro-ph/0607353] [8] P. Meszaros, [arXiv:astro-ph/0605208] [9] A.V.Olinto, [arXiv:astro-ph/0002006] [10] Y. Fukuka et al. (The SuperKamioka Collaboration). [arXiv:hepex/ 9807003] [11] Sandip Pakvasa, [arXiv:hep-ph/0305317] [12] F. Vannucci, [arXiv:hep-ph/0106061] [13] Estimation of the Sensitivity of the Neutrino telescope (NuTel), Tsai Shiang-Rung, Master thesis, National Taiwan University. [14] George W.S. Hou and M.A. Huang, World Scientific, April 9, 2002. [arXiv:astro-ph/0204145] [15] Optics, fourth edition, Chapter 5, Eugene Hecht. [16] Hamamatsu homepage, URL (http://jp.hamamatsu.com/en/index. html ) [17] Calibration of Light Measurement of the Neutrino Telescope, Ping-Jung Su, Master thesis, National Taiwan University. [18] Building Scientific Apparatus, second edition, Chapter6, John H. Moore, Christopher C. Davis, Michael A. Coplan, [19] ANALOG DEVICES homepage, URL (http://www.analog.com/en/ prod/0,,759 842 AD8131,00.html) [20] Yuri Velikzhanin, URL (http://hep1.phys.ntu.edu.tw/nutel/DCM/) [21] PLX Technology homepage, URL(http://www.plxtech.com/ products/io/pci9054.asp) [22] Linux Device Driver, second edition, O’RELLY, Alessandro Rubini & Jonathan Corbet. [23] Yuri Velikzhanin, et al. Nuclear Instruments and Methods in Physics Reach A 552, 2005. [24] TINA URL (http://www.tina.com/) [25] Keithley Instruments, Inc. Section 2-21, Low Level Measurements Handbook, 6th Edition. [26] ANALOG DEVICES homepage, URL (http://www.analog.com/en/ prod/0,,AD9203,00.html) [27] Radiation Detection And Measurement, Ch17, Glenn F Knoll. | |
| dc.identifier.uri | http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/28159 | - |
| dc.description.abstract | 摘要
台大高能實驗室的微中子望遠鏡是用作偵測從宇宙射線中的陶子微中子（ντ）,因陶子 微中子比較容易和相對於宇宙密度較大的地球地表起作用產生陶子（τ）,陶子其次級粒子 在能量大的情況下會產生契倫諧夫光（Cherenkov light).我們可以在山之背面偵測到此光 之訊號來作為偵測到陶子微中子之證據. 微中子望遠鏡之系統包括了光學部份和前端的電子式讀出系統,我們的電子式讀出系統 包括了光電倍增管（MAPMT）,前端放大器(Pre-amp.),資料擷取板(DCM). 資料擷取系統(DAQ) 則是負責將資料擷取板上所紀錄之已觸發之事件資料經由CPCI的匯流排,擷取後儲存在儲 存裝置中（如硬碟）. 我負責的部份是前端電子是讀出系統的校正測試及資料擷取系統,在本論文中我將會介 紹資料擷取系統的流程以及一些前端讀出系統的測試. | zh_TW |
| dc.description.abstract | Abstract
NuTel is the detector for detecting Tau Neutrino. By watching light from air shower behind the mountain, we may detect high energy ¿ particle that is coming from º¿ . The whole system consists of optics and electronic readout. Electronic readout include MAPMT, Pre-amp and DCM. Finally, DCMs record triggered events and DAQ read and save these data into hard disc through CPCI bus. My study are related to the front-end readout system tests and DAQ (data acquisition system). In this thesis I will introduce how user can use this DAQ system to take data from DCM and how can driver transfer data to user.The electronics test results of Pre-amps and DCMs are also discussed in this thesis. | en |
| dc.description.provenance | Made available in DSpace on 2021-06-13T00:01:53Z (GMT). No. of bitstreams: 1 ntu-96-R93222015-1.pdf: 14951434 bytes, checksum: 3bcc7dce486da176ff84975daa989327 (MD5) Previous issue date: 2007 | en |
| dc.description.tableofcontents | 1 Physics Motivation 1
1.1 Neutrinos from Cosmic Ray . . . . . . . . . . . . . . . . . . . 1 1.1.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . 1 1.1.2 Sources of Ultra High Energy Cosmic Neutrinos . . . . 2 1.2 NuTel–Cerenkov detector . . . . . . . . . . . . . . . . . . . . . 4 1.2.1 Earth-Skimming method . . . . . . . . . . . . . . . . . 4 1.2.2 Sensitivity . . . . . . . . . . . . . . . . . . . . . . . . . 6 2 NuTel apparatus 9 2.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9 2.2 Optics System . . . . . . . . . . . . . . . . . . . . . . . . . . . 11 2.3 Multi-Anode Photo Multiplier Tubes (MAPMT) . . . . . . . . 13 2.4 Pre-amplifier (Pre-amp) . . . . . . . . . . . . . . . . . . . . . 15 2.5 Data Collection Module (DCM) . . . . . . . . . . . . . . . . . 19 3 NuTelDAQ characteristics 25 3.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25 3.2 Hardware . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25 3.3 PCI driver and application . . . . . . . . . . . . . . . . . . . . 27 3.4 Events from PCI bus . . . . . . . . . . . . . . . . . . . . . . . 29 3.5 Event lost rate measurement . . . . . . . . . . . . . . . . . . . 31 4 Readout tests 35 4.1 Pre-amps’ response with single pulse . . . . . . . . . . . . . . 35 4.1.1 setting and result . . . . . . . . . . . . . . . . . . . . . 35 4.1.2 conclusion . . . . . . . . . . . . . . . . . . . . . . . . . 48 4.2 Pre-amps’ response with double pulses . . . . . . . . . . . . . 49 4.2.1 method and result . . . . . . . . . . . . . . . . . . . . 49 4.2.2 conclusion . . . . . . . . . . . . . . . . . . . . . . . . . 54 4.3 Linearity of ADC . . . . . . . . . . . . . . . . . . . . . . . . . 55 4.3.1 method and result . . . . . . . . . . . . . . . . . . . . 55 4.3.2 conclusion . . . . . . . . . . . . . . . . . . . . . . . . . 59 4.4 Finding pedestal . . . . . . . . . . . . . . . . . . . . . . . . . 59 4.4.1 method and result . . . . . . . . . . . . . . . . . . . . 59 4.4.2 conclusion . . . . . . . . . . . . . . . . . . . . . . . . . 65 4.5 Linearity of Pre-amps . . . . . . . . . . . . . . . . . . . . . . . 66 4.5.1 method and result . . . . . . . . . . . . . . . . . . . . 66 5 Conclusion 69 | |
| dc.language.iso | en | |
| dc.title | 微中子望遠鏡的前端讀出系統 | zh_TW |
| dc.title | Front-End Readout System of Neutrino Telescope | en |
| dc.type | Thesis | |
| dc.date.schoolyear | 95-2 | |
| dc.description.degree | 碩士 | |
| dc.contributor.oralexamcommittee | 上野耕資,葉平,侯維恕,熊怡 | |
| dc.subject.keyword | 微中子,望遠鏡,高能實驗, | zh_TW |
| dc.subject.keyword | neutrino,telescope,high energy experiment, | en |
| dc.relation.page | 72 | |
| dc.rights.note | 有償授權 | |
| dc.date.accepted | 2007-07-31 | |
| 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 | |
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