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研究生: 許維哲
Hsu, Wei-Che
論文名稱: 行星齒輪系之動態特性分析
Analysis of Dynamic Characteristics of a Planetary Gear System
指導教授: 崔兆棠
Choi, Siu-Tong
共同指導教授: 林博正
Lin, Bor-Jeng
學位類別: 碩士
Master
系所名稱: 工學院 - 航空太空工程學系
Department of Aeronautics & Astronautics
論文出版年: 2013
畢業學年度: 101
語文別: 中文
論文頁數: 52
中文關鍵詞: 有限元素法Lagrangian法行星齒輪系統
外文關鍵詞: Finite element method, Lagrangian approach, Planetary gear system
相關次數: 點閱:120下載:12
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  • 本論文主要以有限元素法分析風力發電機中重負載之行星齒輪增速機的動態特性。假設各齒輪、行星架皆為剛體,轉軸為撓性的Timoshenko樑。以Lagrangian法求得行星齒輪系統的運動方程式,再以Runge-Kutta法求解系統動態響應。本文探討行星齒輪系統在不同行星齒輪個數下,各齒輪之側向位移、太陽與行星齒輪間之壓力角及接觸比及支座軸承反力的變化。數值結果顯示,隨著行星齒輪數目增加,各齒輪與輸出端軸承之側向位移因而減小,壓力角及接觸比的變化幅度也減小,但輸入端軸承之側向位移卻依行星齒輪個數增加而增大。

    Dynamic characteristics of a heavily-loaded planetary gear speed increaser of a wind turbine is analyzed by using the finite element method in this thesis. All gears and carrier are considered to be rigid and rotating shafts are modeled as Timoshenko beams. The Lagrangian approach is used to derive the equations of motion of planetary gear system, and dynamic response is obtained by using the Runge-Kutta method. The effects of number of planetary gears on the lateral displacement of gears, pressure angle and contact ratio between the sun gear and the planetary, reaction force of bearings of the system are investigated. Numerical results of this research show that when the number of planetary gears increases, lateral displacements of gears and of the bearing at the output terminal decrease, and so do the amplitude of pressure angle and contact ratio. However, lateral displacements of the bearing at the input terminal increase as the number of planetary gears increases.

    目錄 摘要 i ABSTRACT ii 誌謝 iii 表目錄 vii 圖目錄 viii 符號說明 x 第一章 緒論 1 1-1前言 1 1-2文獻回顧 2 1-3本文研究 4 第二章 行星齒輪系統 6 2-1行星齒輪系 6 2-2模型建立 7 2-2-1系統基本假設 7 2-3自轉角速度 8 第三章 行星齒輪系統運動方程式 10 3-1運動方程式 10 3-1-1轉軸 10 3-1-2輸入端 12 3-1-3輸出端 17 3-1-4軸承 19 3-1-5齒輪嚙合 20 3-1-6系統運動方程式 23 3-2動態特性分析 24 3-2-1自然頻率分析 24 第四章 數值模擬結果與討論 26 4-1程式驗證 26 4-2位移響應 26 4-3支座軸承反力 27 4-4自然頻率 28 4-4-1齒輪質量對自然頻率之影響 28 4-4-2軸承勁度對自然頻率之影響 29 4-4-3轉軸半徑對自然頻率之影響 29 第五章 結論 31 參考文獻 33

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