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研究生: 林勝亞
Ling, Sheng-Ya
論文名稱: 適用於大氣瞬變現象偵測的快速光度儀之研製
Development of a Fast Speed Photometer for Atmospheric Transient Phenomena
指導教授: 陳炳志
Chen, Bing-Chih
學位類別: 碩士
Master
系所名稱: 理學院 - 太空與電漿科學研究所
Institute of Space and Plasma Sciences
論文出版年: 2022
畢業學年度: 110
語文別: 中文
論文頁數: 66
中文關鍵詞: 快速光度儀大氣瞬變現象閃電高空短暫發光現象
外文關鍵詞: Fast speed photometer(FSP), Atmospheric Transient Phenomena, Lightning, Transient Luminous Events(TLEs)
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  • 大氣瞬變現象(Atmospheric Transient Phenomena)為大氣層內所發生各種光度的變化,包含閃電(Lightning)、高空短暫發光現象(Transient Luminous Events, TLEs)、大氣輝光(Airglows)與極光(Aurora)等,是太空與大氣物理研究中主要的領域之一。為取得大氣瞬變現象的光變曲線與光譜特性,高靈敏度的快速光度儀是量測大氣瞬變現象不可或缺的工具。由於地面觀測會受限於大氣消光的影響,觀測大氣瞬變現象的首選為衛星遙測。然而過往的光電量測酬載(如ISUAL)大多體積龐大且使用到高壓電,因此本論文欲發展一體積小且低耗能的快速光度儀。
    本論文所發展的科學酬載-快速光度儀雛型體(prototype),已在實驗中驗證能夠精確的量測到微小的亮度變化,快速的響應時間與採樣率可有效的紀錄光度變化的細節,資料擷取儲存系統亦能夠準確的識別事件的發生,並準確擷取事件發生瞬間的資料進行儲存。快速光度儀具有低重量體積小等優點,容易滿足中小型載具的任務需求,且擴充性佳,更換光電倍增管和鏡頭即可滿足其他波段的觀測,提供不同科學目的的使用。

    Atmospheric transient phenomena can be defined as all kinds of dynamic luminous events that happen in atmosphere, such as lightning, Transient Luminous Events (TLEs), airglows and aurora, are one of the major topics in space physics and atmospheric physics. To measure the optical characteristic of atmospherics transient phenomena, a sensitive fast speed photometer is necessary. Observations from the ground, airplanes were limited in scope, duration, and especially coverage, therefor a long-term global observation from satellite is the first choice. However, former satellite payloads for photoelectric measurement are mostly huge and heavy, also requiring high voltage. That was a reason for the development of the fast speed photometer that features low energy consumption and simple structure.
    The prototype of fast speed photometer has been testified through experiments that is capable to measure details from rapidly varying of brightness. With data identify and saving algorithm, fast speed photometer can identify atmospheric transient phenomena precisely and recording data automatically. Fast speed photometer is light and compact enough to satisfy satellite missions, and with wide response spectrum can easily fulfil different scientific missions.

    摘要 I 誌謝 IX 表目錄 XII 圖目錄 XIII 第壹章 緒論 1 第1.1節 引言 1 第1.2節 大氣瞬變現象 1 第1.2.1節 閃電 1 第1.2.2節 高空短暫發光現象 4 第1.2.3節 大氣輝光 11 第1.2.4節 大氣瞬變現象的量測 12 第1.3節 研究動機與目的 12 第貳章 快速光度儀設計 14 第2.1節 光電倍增管與基本原理 14 第2.2節 光學與機械結構設計 20 第2.2.1節 光學鏡頭 20 第2.2.2節 光學視野 22 第2.2.3節 機械結構設計 22 第2.3節 快速光度儀與系統架構 25 第2.4節 類比訊號處理電路設計 26 第2.4.1節 電流-電壓轉換器 28 第2.4.2節 緩衝器 29 第2.4.3節 差動放大器 30 第2.4.4節 反相放大器 30 第2.4.5節 低通濾波器 31 第2.4.6節 類比訊號處理電路總體增益 31 第2.5節 類比轉數位訊號與資料擷取演算法 32 第2.6節 總結 36 第參章 快速光度儀校正與性能量測 37 第3.1節 實驗儀器與環境設定 37 第3.2節 增益倍率之校正實驗 39 第3.2.1節 增益倍率之計算 40 第3.2.2節 實驗設置 41 第3.2.3節 數據分析與討論 42 第3.3節 光陰極靈敏度校正 44 第3.4節 FOV量測實驗 47 第3.4.1節 實驗設置 47 第3.4.2節 實驗結果 49 第3.5節 模擬大氣瞬變現象的量測 51 第3.5.1節 實驗配置 52 第3.5.2節 實驗結果 53 第3.6節 實驗總結 56 第肆章 結論與未來展望 57 第4.1節 結論 57 第4.2節 未來展望 58 參考文獻 60 附錄 63

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