| 研究生: |
曾子弋 Tzu-i Tseng |
|---|---|
| 論文名稱: |
閃電之定位與誤差模擬:雷達干涉法與時間差法之分析與研究 A comparative study of lightning detection and error analysis between interferometry method and time-of-arrival technique |
| 指導教授: |
朱延祥
Yen-Hsyang Chu |
| 口試委員: | |
| 學位類別: |
碩士 Master |
| 系所名稱: |
地球科學學院 - 太空科學研究所 Graduate Institute of Space Science |
| 論文出版年: | 2014 |
| 畢業學年度: | 102 |
| 語文別: | 中文 |
| 論文頁數: | 126 |
| 中文關鍵詞: | 閃電 、雷達干涉法 、時間差法 、誤差模擬 |
| 外文關鍵詞: | lightning, interferometry, time-of-arrival, error distribution |
| 相關次數: | 點閱:7 下載:0 |
| 分享至: |
| 查詢本校圖書館目錄 查詢臺灣博碩士論文知識加值系統 勘誤回報 |
民國 101 年,中壢 52MHz 特高頻雷達站增設了一套干涉天線陣列,
由 5 座八木天線排列成非等間距之十字型,提供干涉定位所需 5 路接收
信號;干涉定位時必須利用不同天線間接收目標時,因傳播路徑差而產生
之相位差值,推估出目標物的空間位置;本研究的主要目的是建立此干涉
天線接收閃電訊號並篩選、定位之方法,並以定位結果與整合型閃電落雷
偵測系統的資料進行比較。
利用誤差模擬的模型,對台灣的整合型閃電落雷偵測系統,進行誤差
分布的模擬,再依模擬結果,對閃電偵測系統的誤差進行分析,發現中
壢、新屋附近定位誤差可能很大,閃電偵測系統本身的系統誤差也有4-5
公里。也利用誤差模擬之模型,對氣象局計劃設站的站址,進行布站位置
誤差分布的模擬,並與台電的測站誤差分布進行比較
利用雷達資料對閃電訊號做統計,電壓崩潰後約0.0262 秒會產生回
擊;一次閃電事件,閃電通道能反射、散射雷達脈波的閃電訊號總發生時
間長度為0.4624 秒;多次電壓崩潰幅射出的電磁波,總發生時間約為
0.5285 秒;雷達系統定位閃電的極限距離約為20 公里。利用雷達定位出
閃電的三維結構,推測台電閃電偵測系統,在CG(cloud-ground)的判斷上
有低估的現象。
The new interferometry antenna array composed with the five YAGIs is built at Chung-Li 52MHz VHF radar station in 2012. The antenna array is arranged in the form of an asymmetric cross providing that 5 channels interference received signal. The purpose of this study is to create the method of lightning positioning by interferometry antenna array. And compare the positioning result with Total Lightning Detection System. Interference positioning requires individual path differences between the receiving antennas and targets. We can estimate the spatial position of the target through phase differences due to propagation path difference.
Using the simulation results of error distribution. To analyze the error of Total Lightning Detection System. By simulation result, we can find out there is a high error area near Chung-Li and Xin-Wu. It can also explain why the statistic number of data difference is large at about 11-12 KM. Also use models to simulation the error distribution for the location where central weather bureau will set lightning detection stations. And compare with Total Lightning Detection System.
The stroke will happen about 0.0262 second after leader tip breakdown; The lightning signal will exist about 0.4624 second in a flash. The EM pulse radiate by electrical breakdown will exist 0.5285 second in a flash. Radar detection limit is about 20KM.Use radar data to find out Total Lightning Detection System is underestimate on CG.
(1) N. Marchand, “Error Distributions of Best Estimate of Position from Multiple Time Difference Hyperbolic Networks”, IEEE Trans. on ANE, Vol.11, pp.96-100, Jun, 1964.
(2)Koshak J William , Solakiewicz J Richard.” On the retrieval of lightning radio sources from time-of-arrival data”. J Geophys Res, 101(D21):26631-26639,1996.
(3) Xiu Jian-juan, Xiu Jian-hua, He You, “Location Error Analysis of Direction Finding Location System”,IEEE International Symposium on Microwave, Antenna, Propagation and EMC Technologies for Wireless Communications Proceedings, 2005.
(4) Ronald J. Thomas,Paul R. Krehbiel, William Rison,Steven J. Hunyady,William P. Winn, Timothy Hamlin, and Jeremiah Harlin,” Accuracy of the Lightning Mapping Array”, JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 109, D14207, doi:10.1029/2004JD004549, 2004.
(5) Petersen, W. A., and S. A. Rutledge, “On the relationship between cloud-to-ground lightning and convective rainfall”, J. Geophys. Res.,103(D12), 14,025– 14,040, 1998.
(6) Zipser, E. J., and K. R. Lutz, “The vertical profile of radar reflectivity of convective cells: A strong indicator of storm intensity and lightning probability?” Mon, Wea. Rev., 122, 1751–1759, 1994.
(7) Uman, M. A.,” Lightning,” McGraw-Hill, pp. 264, 1968.
(8) MacGorman, D. R. W. David Rust, “The electrical nature of storms”, Oxford University Press, New York, 1998.
(9) DavidM ackerras, M at Darveniza, Richard E . Orville, Earle R . Williams and Steven J . Goodman, “Global lightning: Total, cloud and ground flash estimates”, JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 103, NO. D16, PAGES 19,791-19,809, AUGUST 27, 1998.
(10)Kenneth L Cummins, Philip Krider E, Malone D., ”The US National Lightning Detection Network and application of cloud-to-ground lightning data by electric power utilities ”, IEEE Transactions on Electromagnetic Compatibility, 40(4):465-479 ,1998.
(11)Lewis E. A., Harvey R. B., Rasmussen J.E., “Hyperbolic Direction finding with sferics of transatlantic origin”, J Geophys Res, 65:1879-1905, 1960.
(12) Elizabeth A. Jacobson and E. Philip Krider,” Electrostatic Field Changes Produced by Florida Lightning”, J. Atmos. Sci., 33, 103–117, 1976.
(13) Kenneth L. Cummins, Martin J. Murphy, Jeffrey V. Tuel,” Lightning Detection Methods And Meteorological Applications”, Presented at the IV International Symposium on Military MeteorologyHydro-Meteorological Support of Allied Forces and PfP Members Tasks Realization, September 26 – 28, 2000.
(14)張文娟,孟青,呂偉濤,姚雯,張義軍,”時間差閃電監測網的誤差分析和布局優化”,應用氣象學報,vol.20,No.4,August,2009.
(15)林熹閔,雲對地閃電與降水關係之研究。大氣科學,27,1,75-98,1999。
(16)吳璧如,細說閃電。物理雙月刊,21,543-549,1999。
(17)朱延祥,MST 雷達回波機制的研究,博士論文,國立中央大學大氣物
理研究所,1988。
(18)楊波,邱實,寧軍,高太長,”閃電定位誤差及探測效率評估”,解放軍理工大學學報,Vol.7,No.5,Oct,2006.
(19)林熹閔與郭鴻基,”1994年南台灣夏季午後對流之研究”。大氣科學,24,4,249-280,1996。
(20)廖建興、曾孝忠,“無線電測向及交叉定位技術研析(下)”,中華民國電子零件認證委員會,IECQ報導第五十三期,2009年9月。
(21)程昭團,利用雷達干涉法進行流星尾定位與背景風場估計,國立中央大學太空科學研究所,碩士論文,2005。
(22)林廷翰,利用中壢特高頻雷達研究中緯度電離層散塊 E層公尺級不規則體之動力行為,國立中央大學太空科學研究所,碩士論文,2009。
(23)陳祥章,中壢雷達三維輻射場型模擬與分析及系統建立,國立中央大學太空科學研究所,碩士論文,2005。
(24)龔瑞鳴,利用中壢VHF雷達進行流星尾觀測系統及方法之建立,國立中央大學大氣物理研究所,博士論文,1998。
(25)鍾明哲,利用中壢特高頻雷達新干涉天線陣列觀測中氣層之風場,國立中央大學太空科學研究所,碩士論文,2013。
(26)毛永毅,無線通信系統定位技術的研究,中國科學院研究生院,博士論文,2008。