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Multisource Assessments of the FengYun-3D Microwave Humidity Sounder (MWHS) On-Orbit Performance

机译:Fengyun-3D微波湿度发声器(MWHS)轨道性能的多源评估

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The microwave humidity sounder (MWHS) onboard the Fengyun-3D satellite is providing the data for profiling atmospheric temperature and moisture and has become an important data source for improving the weather forecasts. In this article, three data sources are utilized for assessing the MWHS on-orbit performance, including Global Navigation Satellite System Occultation Sounder (GNOS), ECMWF (European Centre for Medium-Range Weather Forecasts) Re-Analysis (ERA)-Interim reanalysis, and Advanced Technology Microwave Sounder (ATMS) data. GNOS-retrieved atmospheric profiles and the reanalysis data are used as inputs to the community radiative transfer model (CRTM) for simulating the MWHS brightness temperatures at the top of the atmosphere in July 2018 for characterizing the instrument performance. Since ATMS is a well-calibrated microwave sounding instrument onboard both Suomi NPP and NOAA-20 satellites, its measurements are also collocated with MWHS data for a consensus analysis using the simultaneous nadir overpasses (SNOs) method. In comparing GNOS simulations, MWHS upper air temperature sounding channels (36) have relatively larger biases (less than 2.5 K) than the water vapor sounding channels. However, the standard deviation of the difference between observations and simulations (O-B) is larger for water vapor sounding channels. For ERA simulations, MWHS sounding channels exhibit negative biases similar to GNOS results but the standard deviation of O-B at the water vapor channels is much smaller. When compared with ATMS water vapor channels, MWHS biases are mostly negative and agree with those from ERA simulation. Thus, the large uncertainty in simulating MWHS water vapor sounding channels from GNOS could result from the poor input water vapor profiles and high water vapor variability in the lower troposphere.
机译:凤云-3D卫星船上的微波湿度发声器(MWH)正在为分析大气温度和湿度提供数据,并已成为改善天气预报的重要数据源。在本文中,三个数据源用于评估MWH上的轨道性能,包括全球导航卫星系统覆盖探测器(GNOS),ECMWF(欧洲中等范围天气预报中心)重新分析(ERA) - Interim Reanysis,和先进的技术微波调音器(ATM)数据。 GNOS检索到的大气配置文件和再分析数据被用作社区辐射转移模型(CRTM)的输入,用于在2018年7月在大气顶部模拟MWHS亮度温度,以表征仪器性能。由于ATMS是诸如Suomi NPP和NOAA-20卫星的旋流均匀的微波探测仪器,因此其测量也与MWHS数据一起使用,用于使用同时Nadir立网(SnOS)方法进行共识分析。在比较GNOS模拟时,MWHS上部空气温度探测通道(36)的偏置相对较大(小于2.5k),而不是水蒸气探测通道。然而,观察和模拟之间的差异(O-B)之间的标准偏差对于水蒸气探测通道较大。对于ERA模拟,MWHS探测通道表现出类似于GNOS结果的负偏差,但是在水蒸气通道处的O-B的标准偏差要小得多。与ATMS水蒸气通道相比,MWHS偏差大多数是负的,与来自时代模拟的偏差相同。因此,模拟来自GNOS的MWHS水蒸气探测通道的大不确定性可能是由较差的对流层中的差的输入水蒸气分布和高水蒸气变异性导致。

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