English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 80990/80990 (100%)
造訪人次 : 41628645      線上人數 : 3236
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library IR team.
搜尋範圍 查詢小技巧:
  • 您可在西文檢索詞彙前後加上"雙引號",以獲取較精準的檢索結果
  • 若欲以作者姓名搜尋,建議至進階搜尋限定作者欄位,可獲得較完整資料
  • 進階搜尋


    請使用永久網址來引用或連結此文件: http://ir.lib.ncu.edu.tw/handle/987654321/48142


    題名: 使用白光干涉儀以基因演算法從反射光譜振幅計算光學常數;Calculation of optical constants from reflected spectral amplitude with Genetic Algorithm by white light interferometer
    作者: 蕭義勝;Yi-sheng Siao
    貢獻者: 光電科學研究所
    關鍵詞: 白光干涉儀;薄膜光學常數;基因演算法;Genetic Algorithm;optical costant;optical properties;white light interferometer
    日期: 2011-07-20
    上傳時間: 2012-01-05 14:35:13 (UTC+8)
    摘要: 基因演算法應用在數值分析上一直有傑出的表現,本論文將基因演算 法應用於反推薄膜光學常數,在單層膜且沒有吸收時,可以很精確的反推 出薄膜光學常數。 本論文用五種樣本測量光譜並使用基因演算法擬合光學常數,並將多 次擬合後的光學常數取平均值,將計算出的光譜與測量光譜比較,使用的 材料有Ta2O5、Nb2O5、以及SiO2,其中Ta2O5 與Nb2O5 折射率與厚度較大, 因此在基因演算法中所設定的上下限可以比較廣,薄膜折射率範圍可以在1 到3而薄膜厚度範圍可以在1到1000nm,而SiO2樣本折射率與厚度均較小, 造成光譜沒有轉折點較難擬合,因此將薄膜折射率範圍設定在1.4 到1.5 時 才能得出正確的薄膜厚度。 本論文中的Ta2O5 與Nb2O5 材料,折射率精確度可以優於2%,膜厚精 確度可優於1%,但總體而言擬合的折射率與厚度誤差均小於5%,而SiO2 材料經修正範圍後,擬合出的折射率誤差更可以小於1%,厚度誤差小於 3%。 同一片薄膜樣本,其表面厚度也不一定會各點完全相同,橢圓偏振儀 只能測量出薄膜上某一點的薄膜光學常數,本論文使用白光干涉儀的快速 測量光譜搭配基因演算法的精確擬合,可以將二維的薄膜各點厚度求出 , 將來可以應用在工業上的快速測量與大面積的測量,減少測量時間成本。 The genetic algorithm (GA) is excellent at solving global numerical optimization problems. We propose GA to acquire optical constant of thin films from spectral amplitude retrieved using Fourier transform of the Interferogram. The optical parameters such as refractive index and thickness of thin films are essential for comparison of samples which are produced using different methods. These optical parameters are usually determined by photometric methods or Ellipsometer. The optical thickness, the product of refractive index and thickness determine the spectrum of the thin films. As optical constant in multiple of quarter wave we can find spectrum peaks. Under the condition when the single layer sample has larger optical thickness, we can acquire the optical parameters accurately through GA. In this study, we select five samples which are different materials and thickness and use GA to fit the spectrum to acquire the optical parameters of each sample. We use GA to fit the spectrum 1000 times and use the average optical parameters to calculate the spectrum comparing with the measured spectrum. We use three material Ta2O5, Nb2O5 and SiO2 as the samples. The refractive index of Ta2O5 and Nb2O5 are higher than SiO2, so it is easy for GA to acquire the optical constants under a wide range of the optical parameters. For Ta2O5 and Nb2O5, we set the range of refractive index between one to three and the thickness between 1 nm to 1000 nm. For SiO2, we change the range of refractive index between 1.4 to 1.5. The minimum errors of the calculated refractive index of Ta2O5 and Nb2O5 are smaller than 2% and the thickness are smaller than 1%. The total errors of the optical parameters are smaller than 5%. The errors of the calculated refractive index of SiO2 are smaller than 1% and the thickness are smaller than 3%. The same thin film sample would have different optical parameters on its two-dimensional surface. The Ellipsometer only measure one point on the thin film at a time and it cost at least thirty minute in a process. In this study, we use white-light interferometer with GA to measure the two-dimensional optical parameters on the thin film surface in a short time.
    顯示於類別:[光電科學研究所] 博碩士論文

    文件中的檔案:

    檔案 描述 大小格式瀏覽次數
    index.html0KbHTML627檢視/開啟


    在NCUIR中所有的資料項目都受到原著作權保護.

    社群 sharing

    ::: Copyright National Central University. | 國立中央大學圖書館版權所有 | 收藏本站 | 設為首頁 | 最佳瀏覽畫面: 1024*768 | 建站日期:8-24-2009 :::
    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library IR team Copyright ©   - 隱私權政策聲明