中大機構典藏-NCU Institutional Repository-提供博碩士論文、考古題、期刊論文、研究計畫等下載:Item 987654321/92307
English  |  正體中文  |  简体中文  |  全文笔数/总笔数 : 80990/80990 (100%)
造访人次 : 42694641      在线人数 : 1452
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library IR team.
搜寻范围 查询小技巧:
  • 您可在西文检索词汇前后加上"双引号",以获取较精准的检索结果
  • 若欲以作者姓名搜寻,建议至进阶搜寻限定作者字段,可获得较完整数据
  • 进阶搜寻


    jsp.display-item.identifier=請使用永久網址來引用或連結此文件: http://ir.lib.ncu.edu.tw/handle/987654321/92307


    题名: 改善光學計算鏡光斑對太陽能發電效率之影響;Impact of Improving the Luminous Spot of Fresnel Lens on Solar Power Efficiency
    作者: 薛安翔;Hsueh, An-Hsiang
    贡献者: 光電科學與工程學系
    关键词: Fresnel透鏡;太陽能聚光器;光電發電;光斑;Fresnel lenses;Solar concentrator;PhotoVoltaic;the luminous spots
    日期: 2023-07-22
    上传时间: 2024-09-19 15:45:36 (UTC+8)
    出版者: 國立中央大學
    摘要: Fresnel透鏡作為一種聚光器,被廣泛應用於太陽能發電系統中,透過將太陽光折射的方式聚到太陽能電池片,但由於太陽會不斷移動,而太陽光線入射角度的改變會影響Fresnel透鏡所聚集的光斑位置和形狀,進而影響太陽能發電效率,本論文中光學計算鏡是以Fresnel透鏡原理所製作而成,以此來作為聚光器。
    本論文主要目的是探討光學計算鏡聚焦後光斑與太陽夾角之關係,並分析其對太陽能電池片的發電效率影響。使用Tracepro光線追蹤軟體進行模擬實驗,建立太陽光光源、太陽能電池片模型,以曲率50mm,焦距160mm的Fresnel透鏡,找出光學計算鏡與太陽能電池片放置的最佳距離為30mm,配合調整太陽光光源之角度,得到最合適的光斑寬度為50mm×500mm。
    實驗結果,使用Fresnel透鏡時,考慮全年光斑偏移變量並加以修正,可有效提高能量利用率大於1.5倍。
    ;As a concentrator, the Fresnel lenses are widely used in solar power systems to oncentrate sunlight onto solar cells by refracting the sun. However, due to the continuous movement of the sun, changes in the angle of incidence of sunlight can affect the position and shape of the focused luminous spot created by the Fresnel lens, thereby impacting the efficiency of solar power efficiency.In this paper, an optical calculation mirror, based on the principle of the Fresnel lens, is developed and employed as a concentrator.
    The main objective of this paper is to investigate the relationship between the angle of incidence of focused the luminous spots produced by Fresnel lenses and the efficiency of solar cells. Simulation experiments are conducted using Tracepro ray tracing software, with the setup of a solar light source and a solar cell model. A Fresnel lens with a curvature of 50mm and a focal length of 160mm is utilized, and the optimal distance between the optical calculation mirror and the solar cell is determined to be 30mm. By adjusting the angle of the solar light source, the most suitable Luminous Spot size is obtained, measuring 50mm×500mm.
    The experimental results show that when considering the full-year variation of the spot offset and making appropriate corrections while using the Fresnel lens, the energy utilization efficiency can be effectively increased by more than 1.5 times.
    显示于类别:[光電科學研究所] 博碩士論文

    文件中的档案:

    档案 描述 大小格式浏览次数
    index.html0KbHTML34检视/开启


    在NCUIR中所有的数据项都受到原著作权保护.

    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