首页> 外文会议>55th International Astronautical Congress 2004 vol.2 >The ALADIN Transmit-Receive Optics (TRO) for the Space-borne ADM Aeolus Wind Lidar Mission
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The ALADIN Transmit-Receive Optics (TRO) for the Space-borne ADM Aeolus Wind Lidar Mission

机译:ALADIN发射-接收光学系统(TRO),用于星载ADM风神激光雷达任务

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This paper describes the design of the so-called Transmit-Receive Optics (TRO) for the Aladin lidar instrument on the future ADM Aeolus weather satellite. The TRO as the central optical unit of the Aladin instrument feeds the optical signals from the laser source to the emitting/receiving telescope, and vice versa, the received back scattered signals from the telescope to the spectrometers for Doppler shift evaluation. Additionally, a calibration branch is supported, which bypasses the telescope (from the laser to the spectrometers) and aims at levelling out the received signals in terms of wavelength and signal height changes due to wavelength and intensity variations of the laser. The TRO makes use of refractive optics (lenses) to a high extend taking advantage of the fact, that the spectral range of the Aladin instrument is narrow (centred at 354.8 nm). The opto-mechanical concept of the TRO features afocal optical groups, which are connected by parallel beams. Extreme requirements have been defined for the TRO on the end-to-end transmission (>= 73 %) with an associated effective bandwidth of less than 1 nm over the 200 - 1100 nm spectral range. A solution to these stringent requirements is addressed in this paper. A further feature of the TRO are two so-called aberration generators on the emitting and calibration branch, with which an artificial astigmatism can be realised for eye safety reasons. A three lens configuration has been designed for the aberration genertor. Its effect on astigmatism is presented. This article also addresses the effort on stray light suppression, which is of high importance for the TRO. The qualification of optical coatings, the integration and test philosophy for the TRO concludes this paper.
机译:本文介绍了在未来的ADM Aeolus天气卫星上为Aladin激光雷达仪器设计的所谓的收发光学(TRO)。 TRO作为阿拉丁仪器的中心光学单元,将来自激光源的光信号馈送到发射/接收望远镜,反之亦然,从望远镜接收到的回散射信号到光谱仪以进行多普勒频移评估。此外,还支持一个校准分支,该分支绕过望远镜(从激光器到光谱仪),并旨在根据波长和由于激光器的波长和强度变化而引起的信号高度变化来均衡接收到的信号。 TRO充分利用了Aladin仪器的光谱范围狭窄(集中在354.8 nm)这一事实,充分利用了折射光学器件(透镜)。 TRO的光机械概念具有无焦点光学组,它们由平行光束连接。 TRO对端到端传输(> = 73%)的极端要求已定义,在200-1100 nm光谱范围内,相关有效带宽小于1 nm。本文解决了这些严格要求的解决方案。 TRO的另一个特点是在发射和校准分支上有两个所谓的像差发生器,出于眼睛安全的原因,可以使用它们来实现人工像散。已经为像差产生器设计了三透镜配置。介绍了其对散光的影响。本文还讨论了抑制杂散光的工作,这对于TRO非常重要。总结了光学涂层的鉴定,TRO的集成和测试原理。

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