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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 | Shih-Ying Hsu | en |
dc.contributor.author | 許世穎 | zh_TW |
dc.date.accessioned | 2021-06-15T11:14:05Z | - |
dc.date.available | 2017-10-05 | |
dc.date.copyright | 2016-10-05 | |
dc.date.issued | 2016 | |
dc.date.submitted | 2016-08-21 | |
dc.identifier.citation | [1] http://www.physics.utah.edu/~whanlon/spectrum.html.
[2] http://swift.gsfc.nasa.gov/. [3] https://lecospa.ntu.edu.tw/. [4] Corsika is a popular air shower simulation program. https://www.ikp.kit.edu/corsika/index.php. [5] Gc electronics type 44 heat sink compound. http://www.alliedelec.com/gc-electronics-10-8118/70159782/. [6] Root is a program developed by the cern for the data analysis. https://root.cern.ch/. [7] B. Bodhaine et al. Atmos. Ocean. Technol., 16:1854, 1999. [8] M. Corporation. Tristar mppt modbus specification. http://www.soligent.net/uploads/products/24886_7.pdf. [9] C. W. James, H. Falcke, T. Huege, and M. Ludwig. Phys Rev. E, 84. [10] F. D. Kahn and I. Lerche. Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences, 289(1417):206–213, 1996. [11] Haslam, C. G. T., et al,. Astronomy and Astrophysics, 100:209–219, 1981. [12] heodor Wulf. Observations on the radiation of high penetration power on the eiffel towel. Physikalische Zeitschrschift, 11:811, 1910. [13] T. Instruments. Lm2678 simple switcher high efficiency 5a step-down voltage regulator. http://www.ti.com.cn/cn/lit/ds/symlink/lm2678.pdf. [14] James Ralston, James Heagy, Roger Sullivan. IDA Paper, (P-3385), 1998. [15] J. Linsley. Proc. 15th International Cosmic Ray Conference (ICRC), Plovdiv, Bulgaria, 12:89, 1977. [16] J. Linsley and A. A. Watson. Phys. Rev. Lett, 46:459, 1981. [17] J. Matthews. Astropart. Phys., 22:387–397, 2005. [18] LAMBDA. Haslam 408 mhz data products. http://lambda.gsfc.nasa.gov/product/foreground/2014_haslam_408_get.cfm. [19] J. Linsley. private communication by m. hillas (1988). [20] Morningstar Corporation. Heat dissipation of the tristar & tristar mppt controllers insideenclosures. http://www.morningstarcorp.com/wp-content/uploads/2014/02/TechTip-EnclosureHeatDissipation.pdf. [21] N. Kalmykov and S. Ostapchenko. Phys. Atom. Nucl., 56:346, 1993. [22] Ralf Ulrich and the Pierre Auger Collaboration. Measurement of the proton-air crosssectionwith the pierre auger observatory. EPJ Web of Conference, 53(07005), 2013. [23] D. Mぴuller et al. Ap J, 374:356, 1991. [24] A. Aab et al., (Auger Collab.). Phys. Rev., D91(092008), 2015. [25] A.D. Panov et al. Bull Russian Acad of Science, Physics, 71:494, 2007. [26] Afanasiev, et al. 1996 Proc. Int. Symp. on Extremely High Energy Cosmic Rays, 1996. [27] AMS Collab. Phys. Lett. B, 490:27, 2000. [28] B. Pontecorvo. Zh. Eksp. Teor. Fiz., 33:549–551, 1957. [29] Benjamin Fuchs, for the Pierre Auger Collaboration. Nucl. Instr. Meth. A, 692:93–97, 2012. [30] D.J. Bird et al. (HiRes Collaboration). Astrophys. J., 424:491–502, 1994. [31] E. Fermi. Phys. Rev., 75(8):1169, 1949. [32] E. Waxman and J. Bahcall. Phys. Rev. D, 3359(023002), 1999. [33] F. Aharonian et al. (HESS Collab.). Phys. Rev. D, 75(042004):75, 2007. [34] G. Askaryan. Sov. J. Atom. Energy, 3:921, 1957. [35] Greisen, Kenneth. Phys. Rev. Lett., 16:748–750, 1966. [36] Grigorov, et al. Proceedings of the 12th ICRC, Tasmania, Australia, 5:1760, 1971. [37] H. Falcke, et al. Nature, 435:313–136, 2005. [38] H. Falcke, P. W. Gorhan. Astropart. Phys., 19:477–494, 2003. [39] HiRes Collaboration. Phys.Rev.Lett., 100(101101), 2008. [40] HiRes Collaboration. Astropart. Phys., 32(101101):53–60, 2009. [41] H.S. Ahn et al. Astrophys. J., 707:593, 2000. [42] I. Allekotte et al., for the Pierre Auger Collaboration. Nucl. Instr. Meth. A, 586:409–420, 2008. [43] I. Kravchenko et al., (RICE Collab.). Phys. Rev., D73(082002), 2006. [44] J. Abraham et al. Nuclear Instruments and Methods in Physics Research Section A:Accelerators, Spectrometers, Detectors and Associated Equipment, 620:227–251,2010. [45] J. Abraham et al. (Pierre Auger Collab.). Phys. Rev. Lett., 100(211101), 2008. [46] J. Abraham et al. (The Pierre Auger Collaboration). Phys.Rev.Lett., 101(061101),2008. [47] J. Beringer et al. (Particle Data Group). Phys. Rev. D, 86(010001), 2012. [48] K. Asakimori et al. (JACEE Collab.). Astrophys. J., 502:278, 1998. [49] K. Kotera and A. V. Olinto. Ann. Rev. Astron. Astrophys., 49:119, 2011. [50] M A Lawrence, R J O Reid and A A Watson. J. Phys. G: Nucl. Part. Phys., 17:733, 1991. [51] M. Ackermann et al. (IceCube Collaboration). Astrophys. J., 675(1014), 2008. [52] M. Ave et al. Astrophys. J., 678:262, 2008. [53] M. Boezio et al. Astropart. Phys., 19:583, 2003. [54] M. Nagano, et al. J. Phys. G: Nucl. Part. Phys., 18:423, 1992. [55] M.G. Aartsen et al., (IceCube Collab.). Phys. Rev., D88(112008), 2013. [56] O. Scholten et al. Astropart. Phys., 29:94–103, 2008. [57] P. Chen, et al. (arXiv:1106.3929 [astro-ph.HE]), 2011. [58] P. Gorham et al., (ANITA Collab.). Phys. Rev., D82(022004), 2010. [59] P. Sokolsky, for the HiRes Collaboration. Phys. Rev. Lett., 100(101101), 2008. [60] P. Sokolsky (High Resolution Fly’s Eye Collaboration). Nuclear Physics B (Proc.Suppl.), 212-213:74–78, 2011. [61] P. W. Gorham, et al. Astroparticle Phys., 32:10–41, 2009. [62] P. W. Gorham, et al. Phys. Rev. Lett., 103(051103), 2009. [63] P. W. Gorham, et al. (arXiv:1011.5004 [astro-ph.HE]), 2010. [64] P. W. Gorham, et al. (arXiv:1603.05218 [astro-ph.HE]), 2016. [65] Pierre Auger Collaboration. Phys. Lett. B, B685(061101):239–246, 2010. [66] Pierre Auger Collaboration. Nucl. Instr. Meth. A, 798:172–213, 2015. [67] Pisin Chen, Toshiki Tajima, and Yoshiyuki Takahashi. Phys. Rev. Lett., 89(161101), 2002. [68] R. Engel, D. Seckel, and T. Stanev. Phys. Rev. D, 64(093010), 2001. [69] S. Haino et al. Phys. Lett. B, 594:35, 2004. [70] S. Hoover, J. Nam, et al. Phys. Rev. Lett., 105(151101), 2010. [71] S.C. Corbató, H.Y. Dai, J.W. Elbert, D.B. Kieda, E.C. Loh, P.V. Sokolsky, P. Sommers, J.K.K. Tang. Nuclear Physics B, 28(1417):36–39, 1992. [72] Seo, E. S., et al. Astrophysical Journal, Part 1, 378:763–772, 1991. [73] T. Sanuki et al. Astrophys. J., 545:1135, 2000. [74] Tim Huege. (arXiv:1601.07426 [astro-ph.IM]), 2016. [75] Tim Huege, Clancy W. James. (arXiv:1307.7566 [astro-ph.HE]). [76] V.A. Derbina et al. Astrophys. J., 628:L41, 2005. [77] W. I. Axford, E. Leer and G. Skadron. International Cosmic Ray Conference, 11:132–137, 1977. [78] Zatsepin, G. T.; Kuz’min, V. A. Experimental and Theoretical Physics Letters, 4:78, 1966. [79] T. Abu-Zayyad, et al,. Astroparticle Physics, 48:16–24, 2013. [80] The Pierre Auger Collaboration. arXiv, (1301.6637). [81] Thomas Meures and ARA Collaboration. AIP Conf. Proc., 1535, 2013. [82] T. Huege, et al. (arXiv:1301.2132), 2013. [83] T. K. Gaisser et al. Proc. 16th International Cosmic Ray Conference (ICRC), Kyoto, Japan, 9:275, 1979. [84] Tod E. Kurt. Arduino-serial: C code to talk to arduino. https://todbot.com/blog/2006/12/06/arduino-serial-c-code-to-talk-to-arduino/. [85] W. Heitler. The quantum theory of radiation. [86] Yuanming Ding, Jingjing Sun, Xue Wang. TELKOMNIKA Indonesian Journal of Electrical Engineering, 12(4):3168–3176, 2014. | |
dc.identifier.uri | http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/49029 | - |
dc.description.abstract | 極高能宇宙射線及宇宙微中子的研究已行之有年,而近年來關於無線電波波段的探測方法逐漸地被開發、討論。
南極脈衝瞬態天線 (ANtarctic Impulse Transient Antenna,簡稱 ANITA) 是南極的熱氣球實驗,ANITA 能偵測到宇宙微中子在冰層中因阿斯卡瑞安效應所放出來的訊號,此外,在冰層的反射之下,ANITA 也能觀測宇宙射線大氣簇射所發出的電磁波。從過去兩次飛行中獲得豐碩的成果之後,2014 至 2015 年間進行了第三次的飛行。本論文針對行 ANITA - III 所搭載的資料儲存系統進行研究,設計出一導熱、電磁屏蔽皆良好的資料儲存系統,是當時 NASA 熱氣球計畫中容量最高的設備。 臺灣天文粒子地磁同步輻射觀測站 (Taiwan Astroparticle Radio Observatory of Geosynchrotron Emission,簡稱 TAROGE) 同樣探測無線電波。TAROGE 位於臺灣花蓮的山上,以 12 支水平指向太平洋的天線來探索大天頂角的宇宙射線及宇宙微中子。以宇宙射線大氣簇射與地磁作用所引發出來的電磁波而言,由於臺灣東部山脈緊貼著海岸,除了直接接收到的訊號以外,也可能偵測到海面反射後的訊號,TAROGE 也有能力觀測掠過地球的微中子 (Earth-Skimming Neutrino) 訊號。本論文就 TAROGE 的條件進行模擬,探討坦討此系統探測宇宙射線的的可行性。 本論文也包含了 TAROGE-2 的電源系統研究。一般而言,在背景雜訊微弱的地方不容易有現存的電力來源,本論文就天線站的需求設計出太陽能電力系統,除了電磁屏蔽之外,如何分配電力、電源控制等也是設計的方向。 | zh_TW |
dc.description.abstract | The detection of the ultra high energy cosmic rays (UHECRs) and the cosmic neutrinos has been studied for ages. In the past decades, the use of radio frequency waves (RF) to detect UHE cosmic rays an neutrinos has advanced significantly.
ANtarctic Impulse Transient Antenna (ANITA) is a balloon-borne observatory. It searches for the RF emissions induced by the Askaryan effect when cosmic neutrinos interact with the ice and the ice-reflected signals emitted from the air showers induced by UHECRs. With the enormous harvest from its two flights, ANITA took the third flight in 2014-2015. This thesis presents the study of the ANITA-III storage system. The design principle was the heat dissipation and the RF shielding. The ANITA-III storage system was the largest-storage device in NASA balloon-borne telescope. Taiwan Astroparticle Radio Observatory of Geosynchrotron Emissiom (TAROGE) is also an RF-based detector. TAROGE is located on a coastal mountain-top in Hua-Lian and its 12 antennas are horizontally pointing toward the Pacific Ocean. It can detect not only the direct signals but also the reflected signals emitted from the air showers induced by the CRs. In addition, the Earth-skimming neutrinos are also detectable for TAROGE.This thesis presents the simulation result of the cosmic rays events. This thesis also includes the studies of the TAROGE-2 power system. There is usually no existing power supply system in a RF-quiet location. We built the solar power supply system and the power control system for TAROGE-2. | en |
dc.description.provenance | Made available in DSpace on 2021-06-15T11:14:05Z (GMT). No. of bitstreams: 1 ntu-105-R02222043-1.pdf: 22173727 bytes, checksum: ef5d28a1cf7485cb6f348495c708536b (MD5) Previous issue date: 2016 | en |
dc.description.tableofcontents | 誌謝 v
Acknowledgements vii 摘要 ix Abstract xi 1 Introduction 1 1.1 Cosmic Rays 1 1.1.1 History 1 1.1.2 Composition 1 1.1.3 Energy Spectrum 2 1.1.4 Greisen–Zatsepin–Kuzmin Limit 4 1.1.5 Accelerations 4 1.1.6 Ultra-High-Energy Cosmic Rays (UHECRs) 5 1.2 Ultra-High Energy Cosmic Neutrinos 8 1.2.1 Motivation 8 1.2.2 Cosmogenic Neutrinos 8 1.2.3 Energy Spectrum 9 1.2.4 Earth-Skimming Neutrino 9 1.3 Detections of Cosmic Rays and Cosmic Neutrinos 10 1.3.1 Air Showers 10 1.3.2 Type of Air Showers 11 1.3.3 Air Fluorescence 12 1.3.4 Particle Detector 13 1.4 Radio Frequency Detections 13 1.4.1 Radio Emission Mechanisms 14 1.4.2 Incoherence and Askaryan Effect 15 1.4.3 Radio Frequency Astroparticle Telescopes 17 2 ANtarctic Impulse Transient Antenna (ANITA) 19 2.1 Concepts 19 2.2 ANITA-I and ANITA-II 20 2.3 ANITA-III and Further 21 3 Taiwan Astroparticle Radiowave Observatory for Geo-synchrotron Emissions (TAROGE) 23 3.1 Concepts 23 3.2 TAROGE-1 25 3.3 TAROGE-2 25 4 TAROGE Simulation 27 4.1 Simulation Tools 27 4.1.1 CORSIKA (COsmic Ray SImulations for KAscade) 27 4.1.2 CoREAS 28 4.1.3 Event Template 28 4.2 Shower Production 31 4.2.1 Event Direction and Position 31 4.2.2 Isotropy 32 4.2.3 Cross Section (σ) and Interaction Length (λ) 32 4.2.4 The First Interaction Point )(X 0 ) 34 4.2.5 Shower Maximum (X max ) 34 4.2.6 Maximum Particle Number(N max ) 36 4.2.7 Curvature 37 4.3 Direct Radiation Simulation 39 4.3.1 Cherenkov Angle θ C 39 4.3.2 Event Rescaling: Cherenkov Radius 41 4.3.3 Event Rescaling: Magnetic Field 41 4.3.4 Event Rescaling: Primary Energy 42 4.3.5 Electric Spectral Density Selection and Calibration 43 4.4 Reflected Radiation Simulation 44 4.4.1 Geometry 44 4.4.2 Reflection Coefficient 44 4.5 Signal Processing 46 4.5.1 Polarization of the Signal 46 4.5.2 Power Spectral Density 47 4.5.3 LPDA (Log-Periodic Dipole Array Calculator) 47 4.5.4 Filter, LNA (Low-Pass Amplifier), and Band Filters 48 4.6 Noise 49 4.6.1 Thermal Noise and Noise Temperature 49 4.6.2 Input Noise 50 4.6.3 Receiver Noise 52 4.6.4 System Noise 54 4.7 Trigger Judgement 55 4.8 Simulation Result 56 4.8.1 Effective Area 56 4.8.2 Event Rate 57 4.8.3 Angular Distribution of Triggered Events 61 4.9 Summary 61 5 TAROGE Power System 63 5.1 TAROGE-2 Power Requirement 63 5.2 PV (PhotoVoltaic) Panel Array 64 5.2.1 PV Panels 64 5.2.2 Wiring 65 5.2.3 Waterproofing 65 5.3 Power Box 66 5.3.1 MPPT (Maximum Power Point Tracking) Controller 66 5.3.2 Feedthrough Connectors 67 5.3.3 Adapter Plate and Acrylic Cover 67 5.4 Battery Bank 68 5.4.1 Wiring 68 5.4.2 Characteristic Curve 69 5.5 DAQ Box: Power Board 70 5.5.1 Power Controller 70 5.5.2 Regulator Board 73 5.5.3 Relay Boards 76 5.5.4 Rail-Mount Terminal Blocks and Distribution Blocks 77 5.6 DAQ Box: Computer 77 5.6.1 Serial Communication 77 5.6.2 Program: PowerMonitor 78 5.6.3 Program: PowerOff 78 5.7 Summary 79 6 ANITA Storage System 81 6.1 Box 81 6.1.1 Feedthrough Connectors 82 6.2 SBC (Single Board Computer) 83 6.2.1 Heat Spreader and Thermal Pad 84 6.2.2 Heat Sink 85 6.2.3 SSD (Solid State Disk) 86 6.3 System Internal Battery 86 6.4 RF Noise Measurement 87 6.4.1 Measurement Setting 87 6.4.2 Result 88 6.5 System Test 89 6.5.1 Stress Test 89 6.5.2 Low Pressure Test 90 6.6 Summary 91 7 Conclusion 95 Appendix A Regulator Board 97 Appendix B The Permittivity of the Sea Water 99 Bibliography 101 | |
dc.language.iso | en | |
dc.title | 宇宙射線及宇宙微中子之無線電波探測研究:臺灣天文粒子地磁同步輻射觀測站及南極脈衝瞬態天線 | zh_TW |
dc.title | Studies of the Radio Wave Detection of Cosmic Rays and Cosmic Neutrinos for TAROGE and ANITA | en |
dc.type | Thesis | |
dc.date.schoolyear | 104-2 | |
dc.description.degree | 碩士 | |
dc.contributor.oralexamcommittee | 南智祐(Jiwoo Nam),王名儒(Min-Zu Wang) | |
dc.subject.keyword | 宇宙射線,收音機波, | zh_TW |
dc.subject.keyword | Cosmic ray,radio wave, | en |
dc.relation.page | 106 | |
dc.identifier.doi | 10.6342/NTU201603044 | |
dc.rights.note | 有償授權 | |
dc.date.accepted | 2016-08-21 | |
dc.contributor.author-college | 理學院 | zh_TW |
dc.contributor.author-dept | 物理學研究所 | zh_TW |
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