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Winter 2018 major sudden stratospheric warming impact on midlatitude mesosphere from microwave radiometer measurements

机译:微波辐射计测量的2018年冬季2018年主要突然平流层温度影响Meslate Messphere

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The impact of a major sudden stratospheric warming (SSW) in the Arctic in February?2018 on the midlatitude mesosphere is investigated by performing the microwave radiometer measurements of carbon monoxide (CO) and zonal wind above Kharkiv, Ukraine (50.0°N, 36.3°E). The mesospheric peculiarities of this SSW event were observed using a recently designed and installed microwave radiometer in eastern Europe for the first time. Data from the ERA-Interim and MERRA-2 reanalyses, as well as the Aura microwave limb sounder measurements, are also used. Microwave observations of the daily CO profiles in January–March 2018 allowed for the retrieval of mesospheric zonal wind at 70–85km (below the winter mesopause) over the Kharkiv site. Reversal of the mesospheric westerly from about 10ms?1 to an easterly wind of about ?10ms?1 around 10 February was observed. The local microwave observations at our Northern Hemisphere (NH) midlatitude site combined with reanalysis data show wide-ranging daily variability in CO, zonal wind, and temperature in the mesosphere and stratosphere during the SSW of 2018. The observed local CO variability can be explained mainly by horizontal air mass redistribution due to planetary wave activity. Replacement of the CO-rich polar vortex air by CO-poor air of the surrounding area led to a significant mesospheric CO decrease over the station during the SSW and fragmentation of the vortex over the station at the SSW start caused enhanced stratospheric CO at about 30km. The results of microwave measurements of CO and zonal wind in the midlatitude mesosphere at 70–85km altitudes, which still are not adequately covered by ground-based observations, are useful for improving our understanding of the SSW impacts in this region.
机译:通过在乌克兰的一氧化碳(CO)和乌克兰高于kharkiv上方的一氧化碳(CO)和Zonal Wind(50.0°N,36.3°,通过执行微波辐射计测量的微波辐射计测量e)。使用最近设计和安装的微波辐射计是第一次使用最近设计和安装的微波辐射计观察到这一SSW事件的伴奏特性。还使用来自ERA-INSIM和MERRA-2 Reanalyses的数据以及光环微波肢体测量仪测量。 2018年1月至2018年1月至3月的每日CO档案的微波观察允许在哈尔科夫网站上以70-85km(低于冬季冬季冬季冬季冬季)的伴奏区域风的检索。从大约10ms的伴游逆转到了大约10ms?1到了一个关于10ms的东风?1月10日左右被观察到。我们北半球(NH)中际位点的局部微波观察与再分析数据相结合,在2018年SSW期间,在Messhery和Stratophere中的CO,Zonal风和温度中显示出广泛的日常变异性。观察到的本地CO变异主要是由于行星波活动引起的水平空气质量再分配。在SSW期间,通过周边地区的共差的空气通过共同差的差距较好地替换了共同的极性涡流空气,并在SSW上的涡流上的碎片在SSW开始时旋转,从而引起了大约30km的增强的平衡器CO 。在70-85公里海拔高度的中间态影圈中的CO和Zonal风的微波测量结果仍然没有被地面观测结果充分涵盖,可用于改善我们对该地区SSW的理解。
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