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Flash Camera Options for Coherent Imaging

机译:用于相干成像的闪光灯选项

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We are coming into a time when flash imaging is available for coherent lidar applications. Over the last 20 years we have developed various flash camera options. Each flash imaging camera option has benefits and drawbacks. Most of these detectors however were not developed for coherent imaging. Historically for coherent imaging scientists wanted a strong local oscillator. More recently the ability to measure Doppler shift, and the ability to measure the field, including phase, have been important aspects of coherent imaging. These recent applications will be significantly enabled by flash imaging. Measuring Doppler shift point by point on a bridge, or on an engine, or on the ground, could have some value, but if you measure it in a flash image then you can instantaneously see the vibration spatial modes across the object being imaged. Flash imaging will enable many important applications associated with area vibration measurements. Another important application will be multiple input, multiple output, MIMO, lidar imaging. An array of 32 ×32 format, or more, cameras behind multiple apertures could capture the field in high resolution. If for example we have a hex 19 set of receive apertures we would have 5 apertures across the largest dimension, and if we use multiple transmitters separated across approximately the width of the receive array, and use 32 × 32 format cameras, we can capture coherent images as large as about 300 × 300. Cameras we might consider include Geiger Mode APDs, GMAPDs, Linear Mode APDs, LMAPDs, pin diodes, and framing cameras. Spatial heterodyne coherent imaging can use low bandwidth framing cameras. GMAPDs, LMAPDs, and pin diodes can be used for temporal heterodyne. They have fast enough time response to measure range based upon the time it takes light to get to an object and return. Pin diodes may require a strong LO. GMAPDs will require a weak LO, and LMAPDs could require anywhere from a strong to a weak LO, depending on camera sensitivity.
机译:我们已经进入了闪光成像可用于相干激光雷达应用的时代。在过去的20年中,我们开发了各种闪光灯相机选件。每个闪光灯成像相机选件都有其优点和缺点。然而,大多数这些探测器不是为相干成像而开发的。从历史上看,对于相干成像,科学家想要一个强大的本地振荡器。最近,测量多普勒频移的能力以及测量包括相位的场的能力已经成为相干成像的重要方面。这些最近的应用将通过闪光成像得到显着的支持。在桥梁,发动机,地面上逐点测量多普勒频移可能会有一些价值,但是如果您在闪光灯图像中进行测量,则可以立即看到整个被成像对象的振动空间模式。闪光成像将使许多与区域振动测量相关的重要应用成为可能。另一个重要的应用将是多输入,多输出,MIMO,激光雷达成像。多个光圈后面的32×32格式或更多格式的相机可以高分辨率捕获场。例如,如果我们有一组19个十六进制的接收孔径,那么我们将在最大尺寸上有5个孔径,并且如果我们使用多个发射器,它们在接收阵列的整个宽度上分开,并且使用32×32格式的摄像头,则可以捕获相干的图像的大小约为300×300。我们可能考虑使用的相机包括Geiger模式APD,GMAPD,线性模式APD,LMAPD,pin二极管和取景相机。空间外差相干成像可以使用低带宽成帧相机。 GMAPD,LMAPD和Pin二极管可用于时间外差。它们具有足够快的时间响应,可以根据光到达物体并返回所需的时间来测量范围。引脚二极管可能需要很强的LO。 GMAPD将需要一个弱的LO,而LMAPD可能需要一个强LO到一个弱LO,具体取决于相机的灵敏度。

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