Simulating atmospheric turbulence: Code development and educational applications

Ferran Salazar, Antonio Marzoa Domínguez, M. Crusellas, O. Casamor, Jordi Mazón Bueso, J. Arines
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Abstract

Earth atmosphere turbulence affects many areas of interest related with Space studies, such as optical communications or Astronomy. In fact, it is a key topic for such applications and, thus, it is important for students in aerospace and aeronavigation studies to get some knowledge of the basis of such phenomena, and how to compensate for it. The phenomenon of turbulence is tangent to many areas such as Optics, Meteorology, Fluid Dynamics, Astronomy, Space Science and Telecommunications, among others. To properly understand the effect of such phenomena on the propagation of an optical signal is imprescindible to properly evaluate and implement the corrections introduced with Adaptive Optics [1] and for understanding the limitations of optical free-space communications channels. The simulation of optical propagation through turbulence constitutes an intuitive and powerful tool for visualizing and understanding such phenomena. Within those ideas, a Final Degree Project, based on the development of simulation tools of atmospheric turbulence is carried out in the Escola d’Enginyeria de Telecomunicacions i Aeroespacial de Castelldefels (EETAC) of the Universitat Politècnica de Catalunya (UPC). In this communication the development of an application, written in MATLAB®, for the simulation of optical propagation through turbulent mediums is presented. The project consists of the development of a software based on scalar diffraction theory [2] and Kolmogorov’s turbulence theory for the generation of turbulent phases under specific meteorological conditions and the simulation of the propagation of an electromagnetic signal through them. With this tool, different applications are going to be analysed. As an example of application, at the moment this communication is presented, the code is capable of performing the reconstruction of the generated phase in terms of Zernike coefficients [3], providing key information for the understanding of the aberrations introduced by the turbulence and also for correcting them with a proper design. The communication first describes the main basis of the problem, in terms of scalar diffraction theory, and the structure of the application. Later, some results are presented and discussed. Finally, the application of the tool for adaptive optics, optical free-space communications and as an educational application for aeronavigation and aerospace students is discussed, with emphasis in the context of the different degrees, courses and subjects taught in the EETAC.
模拟大气湍流:代码开发和教育应用
地球大气湍流影响许多与空间研究相关的领域,如光通信或天文学。事实上,这是此类应用的一个关键主题,因此,对于航空航天和航空研究的学生来说,了解这种现象的基础以及如何补偿它是很重要的。湍流现象与光学、气象学、流体动力学、天文学、空间科学和电信等许多领域都有切线关系。正确理解这种现象对光信号传播的影响,对于正确评估和实施自适应光学[1]引入的校正以及理解光自由空间通信信道的局限性是至关重要的。光在湍流中的传播模拟为可视化和理解这类现象提供了一个直观而有力的工具。在这些想法的基础上,在加泰罗尼亚政治大学(UPC)的Castelldefels航空航天电信工程学院(EETAC)开展了一个基于大气湍流模拟工具开发的最终学位项目。本文介绍了用MATLAB®编写的用于模拟光在湍流介质中的传播的应用程序的开发。该项目包括开发基于标量衍射理论[2]和Kolmogorov湍流理论的软件,用于特定气象条件下湍流相的产生和电磁信号在其中传播的模拟。有了这个工具,我们将分析不同的应用程序。作为一个应用示例,在提供此通信的时刻,该代码能够根据泽尼克系数[3]对生成的相位进行重建,为理解湍流引入的像差并通过适当的设计纠正它们提供关键信息。通信首先描述了问题的主要基础,在标量衍射理论方面,以及结构的应用。最后给出了一些结果并进行了讨论。最后,讨论了该工具在自适应光学、光学自由空间通信以及航空航天学生教育中的应用,重点是在EETAC教授的不同学位、课程和科目的背景下。
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