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Optimizing cirrus optical depth retrievals over the ocean from collocated CALIPSO and AMSR-E observations

机译:优化卷曲光学深度检索在海洋中,从搭配Calipso和AMSR-E观察

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摘要

Retrievals of particulate optical depths and extinction coefficients from the cloud-aerosol lidar with orthogonal polarization (CALIOP) instrument deployed on the CALIPSO satellite mainly rely on a single global mean extinction-to-backscatter ratio, also known as the lidar ratio. However, the lidar ratio depends on the microphysical properties of particulates. An alternative approach is adopted to infer single-layer semi-transparent cirrus optical depths (CODs) over the open ocean that does not rely on an assumed lidar ratio. Instead, the COD is inferred directly from backscatter measurements obtained from the CALIOP lidar in conjunction with collocated sea surface wind speed data obtained from AMSR-E. This method is based on a Gram-Charlier ocean surface reflectance model relating wind-driven wave slope variances to sea surface wind speeds. To properly apply this method, the impact of multiple scattering between the sea surface and ice clouds should be taken into account. We take advantage of the 532 nm cross-polarization feature of CALIOP and introduce an empirical method based on the depolarization change at the sea surface to correct for potential bias in sea surface backscatter caused by whitecaps, bubbles, foam, and multiple scattering. After the correction, the COD can be derived for individual CALIOP retrievals in a single cloud layer over the ocean with this method. The global mean COD was found to be roughly 14% higher than the current values determined by the Version 4 CALIOP extinction retrieval algorithm. This study is relevant to future improvements of CALIOP operational products and is expected to lead to more accurate COD retrievals. (C) 2018 Optical Society of America
机译:从Calipso卫星上部署的云 - 气溶胶激光器的云 - 气溶胶激光雷达的颗粒光学深度和消光系数主要依赖于单一的全局平均灭绝反向散射率,也称为激光雷达比。然而,激光雷达比取决于颗粒的微神科性质。采用一种替代方法来推断出在不依赖于假设的激光比的开阔海洋上的单层半透明螺杆光学深度(CODS)。相反,COD被直接推断出从卡利波激光雷达获得的反向散射测量结合从AMSR-e获得的并置海表面风速数据。该方法基于革兰西郡海面反射率模型,将风力驱动波坡差异与海表面风速相关。为了正确应用这种方法,应考虑海面和冰云之间多次散射的影响。我们利用卡利波的532nm十字极化特征,并引入了基于海面的去极化变化的经验方法,以校正由白斑,气泡,泡沫和多个散射引起的海表面后散射的潜在偏差。在校正之后,可以通过这种方法在海洋上的单个云层中的单个卡径检索来导出COD。发现全局平均鳕鱼比由版本4 Caliop灭绝检索检索算法确定的电流值高出14%。本研究与Caliop运营产品的未来改进相关,预计将导致更准确的COD检索。 (c)2018年光学学会

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  • 来源
    《Applied optics》 |2018年第26期|共10页
  • 作者单位

    Stevens Inst Technol Dept Phys Hoboken NJ 07030 USA;

    NASA Langley Res Ctr Hampton VA 23681 USA;

    Stevens Inst Technol Dept Phys Hoboken NJ 07030 USA;

    Lanzhou Univ Coll Atmospher Sci Lanzhou 730000 Gansu Peoples R China;

    Stevens Inst Technol Dept Phys Hoboken NJ 07030 USA;

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  • 正文语种 eng
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