Long-term Variation Characteristics of the Onset of Polar Mesospheric Clouds Season and Its Influencing Factors
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摘要: 夜光云作为形成于中高层(高度约83 km)大气的冰晶云, 其季节起始时间是研究极地中间层热力学与动力学耦合过程的重要参数. 基于1979-2023年多源观测数据, 系统分析了南北半球夜光云季节起始时间的长期演变特征, 并分析其与平流层纬向风场反转事件及太阳活动的相关性. 结果表明, 南北半球夜光云起始时间存在显著差异, 南半球的年际变幅(标准差22 d)约为北半球(11 d)的2倍, 这可能与半球间大气环流模态、重力波活动强度等热力和动力过程差异有关. 在南半球, 夜光云季起始时间与平流层纬向平均风的反转时间表现出极强的正相关关系; 对于北半球, 虽然呈现反相关特性, 但约60 d的相隔时间并不能直接判定二者的影响关系. 太阳活动(Lyman-α 辐射)对夜光云季节起始的调控也呈现半球不对称性, 北半球在2011年前与太阳活动呈一定的负相关, 后期因平流层动力背景转变而衰减, 南半球则表现为微弱响应, 表明太阳辐射效应与动力过程可能共同发挥作用. 此外, 多源数据在结果上的差异也表明, 不同探测体制和数据类型会对夜光云长期变化特性研究带来一定的不确定性.
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关键词:
- 夜光云 /
- 季节开启 /
- 长期变化 /
- 平流层纬向平均风反转 /
- 太阳周期活动
Abstract: Polar Mesospheric Clouds (PMCs), as ice crystal clouds formed in the middle and upper atmosphere (approximately 83 km high), have a seasonal onset that serves as an important parameter for studying the coupling processes between thermodynamics and dynamics in the polar mesosphere. Based on multi-source observational data from 1979 to 2023, the long-term evolution characteristics of the onset of PMCs in both hemispheres are systematically analyzed, and their correlations with the reversal time of stratospheric zonal mean wind and solar activity are examined. Results show that there are significant differences in the onset of PMCs between the two hemispheres: the interannual variation (with a standard deviation of 22 d) in the southern hemisphere is about twice that in the northern hemisphere (11 d), which may be related to differences in thermal and dynamic processes such as inter-hemispheric circulation modes and the intensity of gravity wave activity. In the southern hemisphere, the onset of PMCs season exhibits a very strong positive correlation with the reversal time of the stratospheric zonal mean wind, while in the northern hemisphere, although a negative correlation is observed, the approximately 60-day difference does not directly indicate a causal relationship between the two. The regulation of the onset by solar activity (Lyman-α radiation) also shows hemispheric asymmetry. In the northern hemisphere, there was a certain negative correlation with solar activity before 2011 that later weakened due to changes in the stratospheric dynamic background, whereas the southern hemisphere exhibited only a weak response. This indicates that both solar radiation effects and dynamic processes may jointly contribute. In addition, the discrepancies among multi-source data suggest that differences in detection systems and data types can introduce uncertainties in studies of the long-term variation characteristics of PMCs. -
图 2 1979-2023年南半球夜光云季起始时间与纬向平均风的相关性. (a)季节起始时间与纬向平均风反转时间的年际变化, (b)季节起始时间与纬向平均风反转时间的相关性
Figure 2. Correlation between the onset of PMC seasons and the zonal mean wind in the Southern Hemisphere (SH). (a) The interannual variation between the onset of PMC seasons and the reversal time of zonal mean wind, (b) the correlation between them
图 3 1979-2023年北半球夜光云季起始时间与纬向平均风的相关性. (a) 季节起始时间与纬向平均风反转时间的年际变化, (b) 表示季节起始时间与纬向平均风反转时间的相关性
Figure 3. Correlation between the onset of PMC seasons and the zonal mean wind in the Northern Hemisphere (NH). (a) The interannual variation between the onset of PMC seasons and the reversal time of zonal mean wind, (b) the correlation between them
图 4 2009年南半球的温度与纬向平均风的时空分布. (a) 60°S-90°S纬度范围的ERA5平均温度场; (b) SOFIE每日平均温度数据, 纬度覆盖范围为64°S-82°S, ERA5与SOFIE二者可相互验证温度数据的可用性; (c) 60°S-90°S纬度范围的ERA5纬向平均风场; (d) SOFIE四个不同垂直高度层的温度廓线
Figure 4. Spatio-temporal distributions of temperature and zonal mean wind over the Southern Hemisphere during 2009. (a) Zonal mean temperature field from ERA5 reanalysis data within 60°S-90°S latitude. (b) Daily-averaged temperature observations from SOFIE, covering 64°S-82°S latitude. These two datasets enable cross-validation of temperature measurements. (c) Zonal mean wind field from ERA5 across 60°S-90°S latitude. (d) Vertical temperature profiles from SOFIE at four distinct altitude layers
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孙韶阳 女, 硕士研究生, 研究方向为中高层大气动力学、夜光云物理等. E-mail:
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