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VESPA-22: a ground-based microwave spectrometer for long-term measurements of polar stratospheric water vapor

机译:Vespa-22:一种基于地基微波光谱仪,用于极性平流层水蒸气的长期测量

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摘要

The new ground-based22 GHz spectrometer, VESPA-22 (water Vapor Emission Spectrometer forPolar Atmosphere at 22 GHz) measures the 22.23 GHz watervapor emission line with a bandwidth of 500 MHz and a frequencyresolution of 31 kHz. The integration time for a measurement rangesfrom 6 to 24 h, depending on season and weather conditions. Water vaporspectra are collected using the beam-switching technique. VESPA-22 isdesigned to operate automatically with little maintenance; it employs anuncooled front-end characterized by a receiver temperature of about180 K and its quasi-optical system presents a full width at halfmaximum of 3.5°. Every 30 min VESPA-22 measures also the sky opacityusing the tipping curve technique. The instrument calibration is performedautomatically by a noise diode; the emission temperature of this element isestimated twice an hour by observing alternatively a black body at ambienttemperature and the sky at an elevation of 60°. The retrievedprofiles obtained inverting 24 h integration spectra present a sensitivitylarger than 0.8 from about 25 to 75 km of altitude during winter andfrom about 30 to 65 km during summer, a vertical resolution fromabout 12 to 23 km (depending on altitude), and an overall 1σuncertainty lower than 7 % up to 60 km altitude and rapidlyincreasing to 20 % at 75 km.In July 2016, VESPA-22 was installed at the Thule High Arctic AtmosphericObservatory located at Thule Air Base (76.5° N, 68.8° W),Greenland, and it has been operating almost continuously since then. TheVESPA-22 water vapor mixing ratio vertical profiles discussed in this workare obtained from 24 h averaged spectra and are compared with version 4.2 ofconcurrent Aura/Microwave Limb Sounder (MLS) water vapor vertical profiles.In the sensitivity range of VESPA-22 retrievals, the intercomparison fromJuly 2016 to July 2017 between VESPA-22 dataset and Aura/MLS datasetconvolved with VESPA-22 averaging kernels shows an average difference within1.4 % up to 60 km altitude and increasing to about 6 %(0.2 ppmv) at 72 km.
机译:新地基22GHz光谱仪,Vespa-22(水蒸气发射光谱仪22GHz的极地气氛)测量22.23GHz水具有500MHz的带宽和频率的蒸汽发射线分辨率为31kHz。测量范围的集成时间从6到24小时,取决于季节和天气条件。水蒸气使用光束切换技术收集光谱。 Vespa-22是旨在自动运行,只需很少维护;它雇用了通过接收器温度的未冷却前端特征180K及其准光学系统呈现半宽最大为3.5°。每30分钟Vespa-22也衡量天空不透明使用TIPPE曲线技术。执行仪器校准由噪声二极管自动;该元素的排放温度是每小时估计两次,通过在环境中观察黑色的身体温度和天空升高为60°。检索到获得24h积分光谱的概率呈现灵敏度在冬季和海拔大约25至75公里大于0.8在夏季约30至65公里,垂直分辨率大约12到23公里(取决于高度),以及整体1σ不确定性低于7%,高度高度高度和快速75公里增加到20%。2016年7月,Vespa-22安装在Thule高北极大气中观测台位于Thule Air Base(76.5°N,68.8°W),格陵兰岛,从那时起几乎不断运作。这Vespa-22水蒸气混合比在这项工作中讨论的垂直型材从24h平均光谱获得,与版本4.2进行比较并发Aura /微波肢体发声器(MLS)水蒸气垂直型材。在Vespa-22检索的敏感范围内,来自的互通2016年7月至2017年7月Vespa-22数据集和Aura / MLS数据集之间用Vespa-22卷绕平均内核显示平均差异1.4%高达60公里的高度,增加至约6%(0.2ppmv)72km。

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