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Computer modeling of slit diffraction (spatial filtering)

机译:狭缝衍射的计算机建模(空间滤波)

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Abstract: Generally, there are two sources of diffraction to consider when modeling optical systems: diffraction due to apertures (edge diffraction) and slit diffraction (spatial filtering). Most optical design and analysis programs can handle aperture diffraction, but until recently, none could easily handle slit diffraction. This type of analysis is needed in many areas of optical instrumentation such as spectroscopy or laser systems that utilize spatial filtering. In order to compute slit diffraction, an incoming optical field must first be truncated by a very small aperture (slit, pinhole, etc.). A Fourier decomposition is then performed on this truncated field to produce new direction vectors that then become the diffracted field. At the request of Ball Aerospace Systems group (BASG), Breault Research Organization (BRO), Inc. has developed a new subroutine called DECOMPOSE for their Advanced Systems Analysis Package (ASAP) software. This paper will describe how BASG verified the performance of this subroutine and evaluated it against textbook theory to prove its viability. This work was performed in an effort to analyze a portion of the Infrared Spectrograph (IRS) for the Space Infrared Telescope Facility (SIRTF).!2
机译:摘要:通常,在对光学系统建模时要考虑两个衍射源:由于孔引起的衍射(边缘衍射)和狭缝衍射(空间滤波)。大多数光学设计和分析程序都可以处理孔径衍射,但是直到最近,没有一个程序可以轻松地处理狭缝衍射。光学仪器的许多领域都需要这种类型的分析,例如光谱学或利用空间滤波的激光系统。为了计算狭缝衍射,必须首先通过很小的孔径(狭缝,针孔等)截断入射光场。然后对该截断场进行傅立叶分解,以产生新的方向矢量,该矢量随后成为衍射场。应Ball Aerospace Systems Group(BASG)的要求,Breault研究组织(BRO),Inc.开发了一个名为DECOMPOSE的新子例程,用于其高级系统分析软件包(ASAP)软件。本文将描述BASG如何验证该子程序的性能,并根据教科书理论对其进行评估,以证明其可行性。进行这项工作是为了分析太空红外望远镜设施(SIRTF)的一部分红外光谱仪(IRS)。!2

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