Oceanic wind vector determination using a dual-frequency microwave airborne radiometer theory and experiment

M. Jacobson, W. Emery, E. Westwater
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引用次数: 2

Abstract

Passive ocean-viewing microwave radiometers produce promising results for measuring the near-surface wind vector by measuring the thermal emission from the combined rough surface and atmosphere. The brightness temperature variations of the rough ocean surface provide the necessary information for determining the near ocean surface wind speed and direction. Ocean wind direction measurements have only recently been obtained by microwave radiometers. These recent wind direction measurements showed that ocean brightness temperature variations with respect to azimuth angle (wind direction) varied by a few Kelvin. All these radiometers measured the azimuthal dependence of vertically- and horizontally-polarized ocean brightness temperatures. Brightness temperature measurements at other polarization states (four Stokes parameters) are also sensitive to near surface ocean wind direction. This paper focuses on a nonpolarimetric aircraft-based dual-frequency dual-polarized microwave radiometer that was developed at the Environmental Technology Laboratory (ETL) of the National Oceanic and Atmospheric administration (NOAA). The lower frequency at 23.87 GHz is horizontally-polarized with respect to the aircraft's flight direction and the 31.65 GHz frequency is vertically-polarized to that direction. This radiometer was one of several instruments deployed in ETL's first Advanced Sensor Applications Program (ASAP) experiment. This experiment was named the San Clements Ocean Probing Experiment (SCOPE). The main purpose of the airborne microwave radiometer was to determine if it could measure azimuthal-dependent brightness temperature variations from a rough ocean surface, and thus infer the near-surface wind vector. Furthermore, in order to gain a better understanding on the potential of the NOAA dual-frequency radiometer for near-surface wind vector determination, the SCOPE radiometer measurements are compared with a new combined atmospheric and two-scale ocean surface model.
双频微波机载辐射计测定海洋风矢量的理论与实验
被动海洋观测微波辐射计通过测量粗糙表面和大气的热发射来测量近地面风矢量,取得了令人满意的结果。粗糙海面的亮温变化为确定近海面风速和风向提供了必要的信息。直到最近才通过微波辐射计获得海洋风向的测量。这些最近的风向测量表明,海洋亮度温度随方位角(风向)的变化变化了几个开尔文。所有这些辐射计都测量了垂直和水平极化海洋亮度温度的方位依赖性。在其他偏振状态(四个Stokes参数)下的亮度温度测量对近地表海洋风向也很敏感。本文以美国国家海洋和大气管理局(NOAA)环境技术实验室(ETL)研制的基于飞机的非偏振双频双极化微波辐射计为研究对象。23.87 GHz的较低频率相对于飞机的飞行方向是水平极化的,31.65 GHz的频率相对于该方向是垂直极化的。该辐射计是ETL第一个先进传感器应用程序(ASAP)实验中部署的几种仪器之一。这个实验被命名为圣克莱门茨海洋探测实验(SCOPE)。机载微波辐射计的主要目的是确定它是否能够从粗糙的海洋表面测量出与方位相关的亮度温度变化,从而推断近地面风矢量。此外,为了更好地了解NOAA双频辐射计在近地面风矢量测定中的潜力,将SCOPE辐射计的测量结果与一个新的大气和海洋表面双尺度联合模式进行了比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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