運用ITS系統對於低緯度電離層斷層掃瞄的; 模擬與研究 The simulation of low latitude ionospheric tomography by using ITS system

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題名:	運用ITS系統對於低緯度電離層斷層掃瞄的;模擬與研究 The simulation of low latitude ionospheric tomography by using ITS system
作者:	陳鶴元;Her-Yuan Chen
貢獻者:	太空科學研究所
關鍵詞:	電離層斷層掃描;Tomography
日期:	2006-06-30
上傳時間:	2009-09-22 09:47:10 (UTC+8)
出版者:	國立中央大學圖書館
摘要:	電離層斷層掃描網是一個非常適合用來作為研究大尺度大範圍的系統，特別是台灣地區正恰好可觀察到赤道異常區的大尺度電子濃度的變化。過去於西元1992春季，中央央大學成立低緯度電離層掃描網 (, Low Latitude Ionospheric Tomographic Network , LITN) 此掃描網由北向南共有六個觀測站中國大陸的上海、溫州、臺灣的中壢、高雄、菲律賓的碧瑤和馬尼拉是利用美國海軍導航衛系統 (, Naval Navigation Satellite System , NNSS) 和接收機JMR –1 藉由斷層掃描技術來做為電離層的電子濃度二維的分布圖(Tsai et al . , 2000 ; Huang et al . , 1997 ; 黃啟瑞 , 1997 ) ，但現今NNSS衛星系統中有些衛星已經失效為了能繼續能研究臺灣區上空附近的電離層所以必須重建電離層斷層掃描網。現在於2003年7月中央大學開始向美國NWRA(NorthWest Research Associates , Inc . ) 購置ITS 接收機預計先後在台灣中壢中央大學、草屯南開技術學院和屏東海生館成立接收站，成立低緯度電離層觀測掃描網( LITN )而後希望推展至國外其它地方如菲律賓和印尼等使觀測範更加廣大。而本文中會使用STK衛星軌道模擬軟體與IRI-model來找出衛星的軌道位置與初始值，去找出GPS/MET與真實LITN之電子濃度分佈。結果將與動態電離層觀測儀做比較。福爾摩沙衛星三號升空待其飛到各自的軌道上，將可收集到到更多的資料 (六顆低軌道衛星和多一個頻率1066.66MHZ)，來作為電離層觀測掃描的反演。 The Low Latitude Ionospheric Tomographic Network (LITN) suitable for the study of lare scale ionosphere structure , especially in the Taiwan area , we can study the large scale electron density variation in the equatorial anomaly region . In the past, NCU had begun to set up LITN . It consisted of six ground-based receivers spanning 20∘along Taiwan meridian (121∘E) to receiver beacon signals from the US Naval Navigation Satellite System (NNSS) with receiver JMR-1 in order to carry out the large scale experiments on two-dimensional ionospheric imaging by computerized tomography until the decommission of NNSS satellites in late 1997.Since July 2003, NCU has purchased 4 ITS30 receivers from North West Research Associates, Inc. (NWRA) and set them in Pingtung , Nantou and Taoyuan in Taiwan for the reestablishment of the NEW LITN with the hope to promote the receiving stations to other countries such as Philippines , Indonesia and so on in the near future . In this thesis, We have applied STK ,IRI-model to determine the location of LEO satellite and initial electron number density . In addition, the simulation study of GPS/MET and real data inversion with the ITS receiver were accomplished. A comparison is made between our results and dynasonde data, some possible explanation were discussed. After Formosat-3, which consist of six LEO satellites and one more frequency band (1066.67MHz), entered into their orbits, we can get more data for the inversion of CIT study.
顯示於類別:	[太空科學研究所 ] 博碩士論文

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