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Development of a Mars lidar (MARLI) for measuring wind and aerosol profiles from orbit

机译:火星激光雷达(MARLI)的开发,用于测量轨道上的风和气溶胶剖面

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Our understanding of the Mars atmosphere and the coupled atmospheric processes that drive its seasonal cycles is limited by a lack of observation data, particularly measurements that capture diurnal and seasonal variations on a global scale. As outlined in the 2011 Planetary Science Decadal Survey and the recent Mars Exploration Program Analysis Group (MEPAG) Goals Document, near-polar-orbital measurements of height-resolved aerosol backscatter and wind profiles are a high-priority for the scientific community and would be valuable science products as part of a next-generation orbital science package. To address these needs, we have designed and tested a breadboard version of a direct detection atmospheric wind lidar for Mars orbit. It uses a single-frequency, seeded Nd:YAG laser ring oscillator operating at 1064 nm (4 kHz repetition rate), with a 30-ns pulse duration amplified to 4 mJ pulse energy. The receiver uses a Fabry-Perot etalon as part of a dual-edge optical discrimination technique to isolate the Doppler-induced frequency shift of the backscattered photons. To detect weak aerosol backscatter profiles, the instrument uses a 4x4 photon-counting HgCdTe APD detector with a 7 MHz bandwidth and < 0.4 fW/Hz~(1/2) noise equivalent power. With the MARLI lidar breadboard instrument, we were able to measure Doppler shifts continuously between 1 and 30 m/s by using a rotating chopper wheel to impart a Doppler shift to incident laser pulses. We then coupled the transmitter and receiver systems to a laser ranging telescope at the Goddard Geophysical and Astronomical Observatory (GGAO) to measure backscatter and Doppler wind profiles in the atmosphere from the ground. We measured a 5.3 ± 0.8 m/s wind speed from clouds in the planetary boundary layer at a range of 4 to 6 km. This measurement was confirmed with a range-over-time measurement to the same clouds as well as compared to EMC meteorological models. Here we describe the lidar approach and the breadboard instrument, and report some early results from ongoing field experiments.
机译:由于缺乏观测数据,尤其是在全球范围内捕获昼夜和季节变化的测量数据,我们对火星大气层及其驱动季节循环的耦合大气过程的理解受到限制。正如《 2011年行星科学十年调查》和最近的《火星探索计划分析小组(MEPAG)目标文件》所概述的那样,高度分辨的气溶胶反向散射和风廓线的近极轨道测量对科学界来说是当务之急,有价值的科学产品,是下一代轨道科学软件包的一部分。为了满足这些需求,我们为火星轨道设计并测试了直接检测大气风激光雷达的实验板版本。它使用工作在1064 nm(4 kHz重复频率)的单频种子Nd:YAG激光环形振荡器,将30 ns的脉冲持续时间放大到4 mJ脉冲能量。接收器使用Fabry-Perot标准具作为双边缘光学判别技术的一部分,以隔离多普勒引起的背向散射光子的频移。为了检测微弱的气溶胶反向散射曲线,该仪器使用具有7 MHz带宽和<0.4 fW / Hz〜(1/2)噪声等效功率的4x4光子计数HgCdTe APD检测器。使用MARLI激光雷达面包板仪器,我们能够通过使用旋转的斩波轮对入射激光脉冲进行多普勒频移来连续测量1到30 m / s之间的多普勒频移。然后,我们将发射器和接收器系统连接到戈达德地球物理和天文台(GGAO)的激光测距望远镜,以测量地面大气中的反向散射和多普勒风廓线。我们在4至6 km的范围内测得了行星边界层中云的风速为5.3±0.8 m / s。通过对相同云的时间范围测量以及与EMC气象模型的比较,证实了该测量。在这里,我们描述了激光雷达方法和面包板仪器,并报告了正在进行的现场实验的一些早期结果。

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