A Study of the Diurnal Tide in the MLT Region During the 2020 Sudden Stratospheric Warming Over Yinchuan, China (38.8°N, 106.8°E)

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2025-01-17 DOI:10.1029/2024JA033427
Yun Gong, Jiaxin Bao, Shaodong Zhang, Zheng Ma, Qihou Zhou, Jiahui Luo
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Abstract

We present a study of diurnal tidal variations in the mesosphere and lower thermosphere (MLT) region over Yinchuan (38.8°N, 106.8°E) during the 2020 Northern Hemisphere winter sudden stratospheric warming (SSW) event. This research utilizes data from a newly established meteor radar at Yinchuan, in conjunction with the Specified Dynamics Whole Atmosphere Community Climate Model with Thermosphere and Ionosphere Extension (SD-WACCM-X), the Modern-Era Retrospective analysis for Research and Applications, Version 2 (MERRA-2) reanalysis data, and a meteor radar in Beijing, China (40.3°N, 116.2°E). Our analysis reveals a significant enhancement in the amplitude of the diurnal tide during the 2020 SSW in both meridional and zonal wind components, exceeding the climatological mean by two standard deviations. The variation in the ratio of absolute vorticity to planetary vorticity in the MLT region is known to correlate with diurnal tide amplitude. Our findings indicate that the zonal-mean zonal wind in the MLT underwent a dramatic change during the SSW, with the ratio beginning to decrease 2 days prior to the event. This suggests that changes in the zonal-mean zonal wind during the SSW may play a crucial role in the observed amplification of the diurnal tidal amplitudes. Nevertheless, further investigations are needed to better understand the amplification of diurnal tides in the MLT region during SSWs.

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2020年银川平流层突然变暖(38.8°N, 106.8°E)期间MLT地区日潮特征研究
本文研究了2020年北半球冬季平流层突然变暖(SSW)事件期间银川(38.8°N, 106.8°E)上空中层和低层热层(MLT)区的日潮汐变化。本研究利用银川新建立的流星雷达数据,结合具有热层和电离层扩展的特定动力学全大气群落气候模式(SD-WACCM-X)、现代研究与应用回顾分析第2版(MERRA-2)再分析数据,以及中国北京(40.3°N, 116.2°E)的流星雷达。分析表明,在2020年西南纬向风分量中,经向风分量和纬向风分量的日潮幅值均显著增强,超过气候平均值两个标准差。在MLT区域,绝对涡度与行星涡度之比的变化与日潮汐幅值有关。研究结果表明,南海纬向风的纬向-平均纬向风的比值在南海纬向前2天开始减小。这表明纬向风的变化可能对观测到的日潮振幅的放大起关键作用。然而,需要进一步的研究来更好地了解在ssw期间MLT区域的日潮放大。
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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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