首页> 外文会议>Conference on sensors, systems, and next-generation satellites XXI >Sentinel-5/UVNS: Instrument The principle ability of a slit homogenizer to reduce scene contrast for earth observation spectrometer
【24h】

Sentinel-5/UVNS: Instrument The principle ability of a slit homogenizer to reduce scene contrast for earth observation spectrometer

机译:Sentinel-5 / UVN:仪器缝隙均质器的原理能力,以减少地球观测光谱仪的场景对比度

获取原文

摘要

Sentinel-5/UVNS is an Earth observation spectrometer system that is operating in nadir looking push broom mode from a low Earth orbit. While having a wide across-track field of view (≈2700 km) it covers approximately 7 km at nadir in flight direction during one dwell. However a high contrast in the scene in along track may lead to disturbance of the Instrument Spectral Response Function (ISRF) and with this a variation of measured spectrum. In order to reduce the effect of scene contrast along track, instead of a spectrometer slit two mirrors are introduced, in between which the light path is extended such as a one dimensional wave guide. The entrance length across track however is wide enough to let light pass unchanged. This new concept is called Slit Homogenizer (SH) within theSentinel-5 project. The entrance of the SH is placed on the image plane of the preceding optics. The exit of the SH represents the object plane of the subsequent spectrometer in the along track (spectral) direction. This article proposes a simulation model of a SH together with a preceding generic optics based on scalar diffraction theory. The model is used to evaluate quantitatively the homogenizing ability of the device. Some parameters in the discussed examples are taken from Sentinel-5/UVNS instrument but the model and its application is not limited to that mission.;Airbus Defence and Space GmbH, Willy-Messerschmitt-Str. 1, 82024 Taufkirchen, Germany; Sentinel-5/UVNS is an Earth observation spectrometer system that is operating in nadir looking push broom mode from a low Earth orbit. While having a wide across-track field of view (≈2700 km) it covers approximately 7 km at nadir in flight direction during one dwell. However a high contrast in the scene in along track may lead to disturbance of the Instrument Spectral Response Function (ISRF) and with this a variation of measured spectrum. In order to reduce the effect of scene contrast along track, instead of a spectrometer slit two mirrors are introduced, in between which the light path is extended such as a one dimensional wave guide. The entrance length across track however is wide enough to let light pass unchanged. This new concept is called Slit Homogenizer (SH) within theSentinel-5 project. The entrance of the SH is placed on the image plane of the preceding optics. The exit of the SH represents the object plane of the subsequent spectrometer in the along track (spectral) direction. This article proposes a simulation model of a SH together with a preceding generic optics based on scalar diffraction theory. The model is used to evaluate quantitatively the homogenizing ability of the device. Some parameters in the discussed examples are taken from Sentinel-5/UVNS instrument but the model and its application is not limited to that mission.;Airbus Defence and Space GmbH, Willy-Messerschmitt-Str. 1, 82024 Taufkirchen, Germany; Sentinel-5/UVNS is an Earth observation spectrometer system that is operating in nadir looking push broom mode from a low Earth orbit. While having a wide across-track field of view (≈2700 km) it covers approximately 7 km at nadir in flight direction during one dwell. However a high contrast in the scene in along track may lead to disturbance of the Instrument Spectral Response Function (ISRF) and with this a variation of measured spectrum. In order to reduce the effect of scene contrast along track, instead of a spectrometer slit two mirrors are introduced, in between which the light path is extended such as a one dimensional wave guide. The entrance length across track however is wide enough to let light pass unchanged. This new concept is called Slit Homogenizer (SH) within theSentinel-5 project. The entrance of the SH is placed on the image plane of the preceding optics. The exit of the SH represents the object plane of the subsequent spectrometer in the along track (spectral) direction. This article proposes a simulation model of a SH together with a preceding generic
机译:Sentinel-5 / UVN是一种地球观测光谱仪系统,该系统在Nadir上操作,从低地球轨道看推扫帚模式。虽然具有宽阔的轨道视野(≈2700km),但它在一个居住期间在飞行方向上覆盖Nadir约7公里。然而,沿着轨道的场景中的高对比度可能导致仪器光谱响应函数(ISRF)的干扰,并且具有测量光谱的变化。为了减少沿轨道的场景对比度的影响,而不是引入光谱仪狭缝,在诸如一维波导的诸如一维波导的光路之间。然而,轨道的入射长度足够宽,以使光通过不变。这种新的概念称为Thesentinel-5项目中的Slit均化器(SH)。 SH的入口处放置在前面光学的图像平面上。 Sh的出口表示随后的光谱仪的沿轨道(光谱)方向的物体平面。本文提出了一种基于标量衍射理论的先前通用光学器的SC的模拟模型。该模型用于定量评估装置的均化能力。讨论的示例中的一些参数来自Sentinel-5 / UVNS仪器,但模型及其应用不限于该任务。;空中客车防御和太空GmbH,Willy-Messerschmitt-str。 1,82024 Taufkirchen,德国; Sentinel-5 / UVN是一种地球观测光谱仪系统,该系统在Nadir上操作,从低地球轨道看推扫帚模式。虽然具有宽阔的轨道视野(≈2700km),但它在一个居住期间在飞行方向上覆盖Nadir约7公里。然而,沿着轨道的场景中的高对比度可能导致仪器光谱响应函数(ISRF)的干扰,并且具有测量光谱的变化。为了减少沿轨道的场景对比度的影响,而不是引入光谱仪狭缝,在诸如一维波导的诸如一维波导的光路之间。然而,轨道的入射长度足够宽,以使光通过不变。这种新的概念称为Thesentinel-5项目中的Slit均化器(SH)。 SH的入口处放置在前面光学的图像平面上。 Sh的出口表示随后的光谱仪的沿轨道(光谱)方向的物体平面。本文提出了一种基于标量衍射理论的先前通用光学器的SC的模拟模型。该模型用于定量评估装置的均化能力。讨论的示例中的一些参数来自Sentinel-5 / UVNS仪器,但模型及其应用不限于该任务。;空中客车防御和太空GmbH,Willy-Messerschmitt-str。 1,82024 Taufkirchen,德国; Sentinel-5 / UVN是一种地球观测光谱仪系统,该系统在Nadir上操作,从低地球轨道看推扫帚模式。虽然具有宽阔的轨道视野(≈2700km),但它在一个居住期间在飞行方向上覆盖Nadir约7公里。然而,沿着轨道的场景中的高对比度可能导致仪器光谱响应函数(ISRF)的干扰,并且具有测量光谱的变化。为了减少沿轨道的场景对比度的影响,而不是引入光谱仪狭缝,在诸如一维波导的诸如一维波导的光路之间。然而,轨道的入射长度足够宽,以使光通过不变。这种新的概念称为Thesentinel-5项目中的Slit均化器(SH)。 SH的入口处放置在前面光学的图像平面上。 Sh的出口表示随后的光谱仪的沿轨道(光谱)方向的物体平面。本文提出了一种与前一般通用的SH的模拟模型

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号