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研究生:姚德劭
研究生(外文):De-Shao Yao
論文名稱:高頻電波斜向傳播模擬
指導教授:朱延祥
指導教授(外文):Yen-Hsyang Chu
學位類別:碩士
校院名稱:國立中央大學
系所名稱:太空科學研究所
學門:自然科學學門
學類:天文及太空科學學類
論文種類:學術論文
論文出版年:2019
畢業學年度:107
語文別:中文
論文頁數:143
中文關鍵詞:電波覓跡高頻電波模擬
外文關鍵詞:Ray traceHF band wave propagation simulation
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越地平天波通訊是將電波斜向入射電離層並透過電離層反射實現,所以為了建立越地平天波通訊技術,須先了解電波傳播之情形。電波的傳播方向會受折射指數梯度影響;其中,主要影響高頻電波傳播方向的因素為電離層內折射指數的梯度。本篇論文將在不同背景假設下進行電波軌跡模擬(電波覓跡),包含:(1)直角坐標僅考慮電子濃度;(2)球坐標僅考慮電子濃度;(3)球坐標考慮電子濃度、磁場,其中以考慮磁場、電子濃度與梯度的球坐標模擬為主要探討對象。模擬中,不考慮磁場部分可透過理論方程式與解析解進行驗證,論文的模擬結果與理論值比對後十分接近,可認定模擬結果有極高的準確性;而考慮磁場模擬部分,電離層中的磁場資訊將參考國際地磁參考場模式(International Geomagnetic Reference Field model,IGRF model);而電子濃度則是參考國際電離層參考模式(International Reference Ionosphere model ,IRI model),電波模擬之時間為太陽活動週期極大期(2015)與太陽活動周期極小期(2008)的正午與凌晨。因考慮磁場作用,電波將分為正常波與異常波,因傳播性質與特性差異甚大,所以對於模擬結果將分開做討論。模擬結果包含對影響正異常波傳播特性因素比較、太陽活動周期與日夜變化對傳播路徑與頻率的影響,最後模擬在三維球坐標下,正異常波傳播軌跡、落點與極化面旋轉估算。
本篇論文藉由在不同假設下的電波模擬比較電波傳播性質的差異進而驗證電波傳播特性,以建立越地平系統發射電波軌跡模擬模型,提供使用者快速、準確的發射參數選擇依據。
Over the horizon (OTH) communications is obliquely transmitting the electromagnetic wave (EM wave) through the atmosphere and reflecting by ionosphere. To establish OTH sky wave communications system, understanding the EM wave properties is the most important. The propagation directions are influenced by the gradient of refractive indexes. Because transmission frequency of OTH communications is HF band (3~ 30MHz), the major affected factor is ionospheric refractive index gradient. In the thesis, the simulations apart into two kinds: including magnetic field and not including magnetic field.
When the simulations don’t include the magnetic field, the result can verify by theoretical formula. By comparing results and theoretical value, the simulation results are much precise.
When the simulations include the magnetic field, the background information of ionosphere refer to IRI and IGRF and the dates are minimal solar activity period (2008) and maximal solar activity period (2015). Under the influence of magnetic field, the EM wave divides into ordinary wave (O-wave) and extraordinary wave (X-wave) when the wave propagates in ionosphere. The results include the major influence of the difference between O-wave and X-wave propagation property and the impact of solar activity and daily varying on transmission frequency. In the end, the thesis shows the results about EM wave propagation paths, footprints and polarized plane variations in three-dimensional spherical coordinates.
The thesis concludes the propagation properties in different situations and coordinates by numerical simulations. By results, establishing the ray trace model to provide much fast and accurate basis about OTH communication system.
摘要 i
Abstract ii
目錄 v
圖目錄 viii
表目錄 xi
第一章、序論 - 1 -
1.1研究動機與目的 - 1 -
1.2內容組織大綱 - 3 -
第二章、模擬理論與基礎 - 4 -
2.1 磁離理論 - 4 -
2.1.1電漿頻率(Plasma frequency) - 4 -
2.1.2 電子旋繞頻率(Electron gyro-frequency) - 5 -
2.2 電離層折射指數與極化面旋轉 - 7 -
2.2.1 電離層折射指數 - 7 -
2.2.2 極化面旋轉 - 10 -
2.3電離層介紹 - 12 -
2.3.1 D層 - 12 -
2.3.2 E層 - 13 -
2.3.3 F層 - 14 -
2.4 國際電離層參考模式(IRI model) - 16 -
2.5 國際地磁參考場模式(IGRF model) - 19 -
2.6數值方法 - 20 -
2.6.1 Euler方法 - 20 -
2.6.2 ABM方法 - 21 -
第三章、模擬方法與流程 - 25 -
3.1運用司乃耳定律僅考慮電子濃度之電波模擬 - 25 -
3.1.1 正割定理(Secant law) - 26 -
3.1.2 Breit and Tuve 定理 - 27 -
3.1.3 模擬流程 - 29 -
3.2運用球面司乃耳定律僅考慮電子濃度之電波模擬 - 33 -
3.2.1 正割定理 - 33 -
3.2.2 電波路徑解析解計算 - 35 -
3.2.3 模擬流程 - 39 -
3.3 考慮電子濃度與磁場之二維球坐標模擬 - 44 -
3.3.1 折射指數 - 44 -
3.3.2 模擬方程組 - 44 -
3.3.3 模擬流程 - 46 -
3.4考慮電子濃度與磁場之三維球坐標模擬 - 49 -
第四章、模擬結果與討論 - 53 -
4.1運用司乃耳定律僅考慮電子濃度之電波模擬 - 53 -
4.1.1 傳輸曲線 - 53 -
4.1.2 電波模擬 - 54 -
4.2運用球面司乃耳定律僅考慮電子濃度之電波模擬 - 70 -
4.2.1 電波模擬與驗證 - 71 -
4.2.2 坐標系統差異 - 86 -
4.3 考慮電子濃度與磁場之二維球坐標模擬 - 91 -
4.3.1 電離層電子濃度與磁場對電波路徑影響分析 - 92 -
4.3.2 電波往返路徑探討 - 93 -
4.3.3 高頻電波電波覓跡模擬 - 96 -
4.4 考慮電子濃度與磁場之三維球坐標模擬 - 105 -
4.4.1 三維電波傳播軌跡與落點模擬 - 106 -
4.4.2 電波極化面旋轉估算 - 113 -
第五章、結論與未來展望 - 117 -
5.1結論 - 117 -
5.2 未來展望 - 120 -
參考文獻 - 122 -
附錄一、模擬方程組推導 - 124 -
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2. Budden, K.G. The Propagation of the Radio Wave. Cambridge University Press, Cambridge, 1985.
3. Cesidio Bianchi, Alessandro Settimi, Carlo Scotto, Adriano Azzarone, Angelo Lozito.A method to test HF ray tracing algorithm in the ionosphere by means of the virtual time delay. Advances in Space Research Volume 48, Issue 10, Pages 1600-1605, 2011.
4. Davies, K, Ionospheric Radio Propagation, London,1968.
5. D. Bilitza and B.W. Reinisch , International Reference Ionosphere 2007: Improvements and new parameters, Advances in Space Research 42 599–609,2008.
6. Erwin Kreyszig , Advanced Engineering Mathematics,陳常侃,江大成譯,全華圖書,2012.
7. John M. Kelso, Ray Tracing in the Ionosphere, RADIO SCIENCE, Vol. 3 (New Series), No. 1, January 1968.
8. Jones, R.M., Stephenson, J.J. A versatile three-dimensional ray tracing computer program for radio waves in the ionosphere. OT Report, 75–76, US Department of Commerce, Office of Telecommunication, US Government Printing Office, Washington, US, 1974.
9. Lighthill M. J, Group Velocity, J.Inst.Maths Applies 1,1964.
10. Newbern Smith, The Relation of Radio Sky-Wave Transmission to Ionosphere Measurements.
11. R. J. Norman and P.S. Cannon, A two- dimensionalanalytic ray tracing technique accommodatinghorizontal gradients, RadioScience, Volume32, Number2, Pages387-396,March-April 1997.
12. Thomas A. Croft and Harry Hoogasian, Exact Ray Calculations in a Quasi-Parabolic Ionosphere With No Magnetic Field , RadioScience, Vol. 3 (New Series), No. l,p63-74,1968.
13. Tsai, L.‐C., C. H. Liu, and J. Y. Huang, Three‐dimensional numerical ray tracing on a phenomenological ionospheric model, Radio Sci., 45, RS5017,2010.
14. Witvliet Ben A., Erik van Maanen, George J. Petersen, Albert J. Westenberg,Mark J. Bentum, Cornelis H. Slump, and Roel Schiphorst, Measuring the Isolation of the Circularly Polarized Characteristic Waves in NVIS Propagation, IEEE Antennas Propagat . Mag.,vol.57 ,pp.120 - 145,June 2015.
15. Xueqin Huang and Bodo W. Reinisch, Real-time HF ray tracing through a tilted ionosphere, RadioScience, VOL. 41, RS5S47,2006
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