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从MABEL光子计数激光雷达的原始数据中检测海洋表面。

Detecting the ocean surface from the raw data of the MABEL photon-counting lidar.

作者信息

Ma Yue, Liu Rui, Li Song, Zhang Wenhao, Yang Fanlin, Su Dianpeng

出版信息

Opt Express. 2018 Sep 17;26(19):24752-24762. doi: 10.1364/OE.26.024752.

DOI:10.1364/OE.26.024752
PMID:30469587
Abstract

With much smaller footprints (approximately a few tens of meters), the data of a laser altimeter are promising for obtaining the sea level near offshore areas, where radar altimeters with larger footprints cannot operate. However, the current ocean surface detection methods for a photon-counting lidar cannot effectively eliminate the noise photons when measuring the sea surface, thereby introducing a ranging bias. In this paper, a new ocean surface detection method is derived based on the JONSWAP (Joint North Sea Wave Project) wave spectrum and LM (Levenberg-Marquardt) nonlinear least-squares fitting. Using the data photons that are captured by the NASA MABEL (Multiple Altimeter Beam Experimental Lidar) photon-counting lidar, the new method is tested and compared to the MABEL standard result. The new method achieved better profile detection of sea surfaces and successfully discarded the noise photons in a sub-layer below the sea surface from the MABEL standard result. By reconstructing the "accumulated waveform", we found that the noise photons in the sub-layer produce small tails after the main waveform, which introduces an overestimated ranging bias of 9 cm. This difference of 9 cm is similar to the sea level bias of 10 cm that was obtained from the ICESat/GLAS laser altimeter data and the TOPEX/Poseidon radar altimeter data in an earlier study, which limited the use of laser altimeter data. According to the analysis in this paper, we can partially interpret what occurred for the ICESat/GLAS waveform tails when ICESat was measuring sea surfaces. The newly derived method can protect the MABEL and incoming ICESat-2 data photons from noise photon interference and ranging bias when measuring the sea surface.

摘要

激光高度计的数据足迹要小得多(约几十米),有望用于获取近海区域的海平面,而足迹较大的雷达高度计在这些区域无法运行。然而,目前光子计数激光雷达的海面探测方法在测量海面时无法有效消除噪声光子,从而引入测距偏差。本文基于JONSWAP(联合北海海浪项目)波谱和LM(Levenberg-Marquardt)非线性最小二乘拟合推导了一种新的海面探测方法。利用美国国家航空航天局MABEL(多高度计光束实验激光雷达)光子计数激光雷达捕获的数据光子,对新方法进行了测试,并与MABEL标准结果进行了比较。新方法实现了更好的海面剖面探测,并成功地从MABEL标准结果中剔除了海面以下子层中的噪声光子。通过重建“累积波形”,我们发现子层中的噪声光子在主波形之后产生小尾巴,这引入了9厘米的高估测距偏差。这9厘米的差异与早期研究中ICESat/GLAS激光高度计数据和TOPEX/Poseidon雷达高度计数据获得的10厘米海平面偏差相似,这限制了激光高度计数据的使用。根据本文的分析,我们可以部分解释ICESat测量海面时ICESat/GLAS波形尾部出现的情况。新推导的方法可以保护MABEL和即将到来的ICESat-2数据光子在测量海面时免受噪声光子干扰和测距偏差的影响。

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