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Photon-Counting Multikilohertz Microlaser Altimeters for Airborne and Spaceborne Topographic Measurements

机译:光子计数多千赫兹微激光高度计,用于机载和星载地形测量

摘要

We consider the optimum design of photon-counting microlaser altimeters operating from airborne and spaceborne platforms under both day and night conditions. Extremely compact Q-switched microlaser transmitters produce trains of low energy pulses at multi-kHz rates and can easily generate subnanosecond pulse-widths for precise ranging. To guide the design, we have modeled the solar noise background and developed simple algorithms, based on Post-Detection Poisson Filtering (PDPF), to optimally extract the weak altimeter signal from a high noise background during daytime operations. Practical technology issues, such as detector and/or receiver dead times, have also been considered in the analysis. We describe an airborne prototype, being developed under NASA's instrument Incubator Program, which is designed to operate at a 10 kHz rate from aircraft cruise altitudes up to 12 km with laser pulse energies on the order of a few microjoules. We also analyze a compact and power efficient system designed to operate from Mars orbit at an altitude of 300 km and sample the Martian surface at rates up to 4.3 kHz using a 1 watt laser transmitter and an 18 cm telescope. This yields a Power-Aperture Product of 0.24 W-square meter, corresponding to a value almost 4 times smaller than the Mars Orbiting Laser Altimeter (0. 88W-square meter), yet the sampling rate is roughly 400 times greater (4 kHz vs 10 Hz) Relative to conventional high power laser altimeters, advantages of photon-counting laser altimeters include: (1) a more efficient use of available laser photons providing up to two orders of magnitude greater surface sampling rates for a given laser power-telescope aperture product; (2) a simultaneous two order of magnitude reduction in the volume, cost and weight of the telescope system; (3) the unique ability to spatially resolve the source of the surface return in a photon counting mode through the use of pixellated or imaging detectors; and (4) improved vertical and transverse spatial resolution resulting from both (1) and (3). Furthermore, because of significantly lower laser pulse energies, the microaltimeter is inherently more eyesafe to observers on the ground and less prone to internal optical damage, which can terminate a space mission prematurely.
机译:我们考虑在白天和黑夜条件下从机载和星载平台运行的光子计数微激光高度计的最佳设计。极为紧凑的调Q开关微激光发射器可产生多kHz速率的低能量脉冲序列,并可轻松产生亚纳秒脉冲宽度,以实现精确的测距。为了指导设计,我们对太阳噪声背景进行了建模,并基于后泊松泊松滤波(PDPF)开发了简单的算法,以在白天运行时从高噪声背景中最佳地提取弱测高仪信号。分析中还考虑了实际技术问题,例如检测器和/或接收器停滞时间。我们描述了一种航空原型,它是根据NASA的仪器孵化器计划开发的,旨在以10 kHz的速率从高达12 km的飞机巡航高度以几微焦耳的激光脉冲能量运行。我们还分析了一个紧凑而高效的系统,该系统旨在在300 km的火星轨道上运行,并使用1瓦激光发射器和18 cm望远镜以高达4.3 kHz的速率对火星表面进行采样。这样产生的Power-Aperture乘积为0.24 W平方米,对应的值几乎比Mars Orbiting Laser Altimeter(0。88W平方米)小4倍,但采样率大约是400倍(4 kHz vs 10 Hz)相对于传统的高功率激光高度计,光子计数激光高度计的优势包括:(1)更有效地利用可用的激光光子,对于给定的激光功率望远镜孔径,可提供高达两个数量级的更大表面采样率产品; (2)同时缩小望远镜系统的体积,成本和重量两个数量级; (3)通过使用像素化或成像检测器以光子计数模式在空间上解析表面回波源的独特能力; (4)改善了(1)和(3)的垂直和横向空间分辨率。此外,由于大大降低了激光脉冲能量,因此微高度计本来就对地面上的观察者来说对眼睛更安全,并且不易受到内部光学损害,因为内部光学损害会提前终止太空任务。

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