来自地球观测系统(EOS)卫星的激光雷达压力和温度廓线测量模拟

C. Korb, C. Weng
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引用次数: 1

摘要

大气压和温度场是气象学、气候研究和所有尺度的天气预报中最重要的两个基本变量。压力场用于描述大气状态、锋面特征和确定质量运动。温度场是确定对流层顶高度、行星边界层深度和结构以及锋面和气团特征所必需的。本文分析了激光雷达差分吸收(DIAL)测量地球观测系统(EOS)卫星压力和温度所需的灵敏度和仪器参数。EOS平台上拟议的激光雷达大气探测仪和高度计(LASA)设施将允许从700公里的极地轨道上测量全球压力和温度分布。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Simulation of Lidar Pressure and Temperature Profile Measurements from the Earth Observing System (EOS) Satellite
The atmospheric pressure and temperature fields are two of the basic variables of fundamental importance in meteorology, climate studies, and for all scales of weather forecasting. The pressure field is used to describe the state of the atmosphere, frontal characteristics and to determine mass movement. The temperature field is needed for determining tropopause height, the depth and structure of the planetary boundary layer, and frontal and air mass characteristics. This paper presents an analysis of the sensitivity and instrumental parameters needed for lidar differential absorption (DIAL) measurements of pressure and temperature from the Earth Observing System (EOS) satellite. The proposed Lidar Atmospheric Sounder and Altimeter (LASA) facility on the EOS platform will allow global measurements of pressure and temperature profiles from a 700 km polar orbit.
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