Influence of Lower Atmosphere on Long-Term Total Electron Content Variations of Mid-latitude Ionosphere in Winter Seasons 2012 – 2018

I. Zakharov
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Abstract

Background. In recent decades, new results on the influence of powerful meteorological processes on the ionosphere have been obtained. At the same time, the possibility of tropospheric-ionospheric interaction outside the disturbed periods remains unclear, which is important for assessing the energy of the phenomenon and for modeling the dynamic processes of the lower and upper atmosphere as a single self-organizing system. In this work, for the first time, the possibility of the influence of the lower atmosphere on the median values of ionospheric parameters against the background of processes caused by space weather is considered. Objectives of the work is to search and analyze long-term longitudinal effects of the mid-latitude ionosphere in the winter season and their possible connection with processes in the lower atmosphere. Materials and methods. The studies were carried out using daily data for the winter seasons of 2012 – 2018 at a latitude of 40 °N on the basis of maps of ionospheric total electron content obtained using the global network of navigation satellites and global maps of pressure and temperature of the surface atmosphere. Data on space weather and the magnetosphere (indices of solar and geomagnetic activity) were also used. Statistical analysis methods were used. Results. Significant (up to 40 % of the average level) permanently existing longitudinal extrema of the ionospheric total electron content have been established, which correlate with changes in the pressure and temperature of the surface atmosphere. The relationship is characterized by significant correlation coefficients from +0.34 to +0.48 in the seasons under consideration. The total electron content maxima fall on longitudes with maximum surface atmospheric pressure gradients. The influence of space weather through the mismatch between the geographic and geomagnetic coordinate systems also leads to longitudinal effects in the ionosphere, but without the formation of local extrema. Conclusions. The results obtained indicate the possibility of long-term or continuous interaction of the lower atmosphere with the higher layers of the atmosphere and the ionosphere. Taking into account the constant nature of the longitudinal features of the total electron content, an assumption was made about the important role of stationary planetary waves in the implementation of atmospheric-ionospheric interactions.
低层大气对2012 - 2018年冬季中纬度电离层总电子含量长期变化的影响
背景近几十年来,关于强大的气象过程对电离层的影响,已经获得了新的结果。与此同时,扰动期之外对流层-电离层相互作用的可能性仍然不清楚,这对于评估这一现象的能量和将低层和高层大气的动态过程建模为一个单一的自组织系统非常重要。在这项工作中,首次考虑了在空间天气过程的背景下,低层大气对电离层参数中值的影响的可能性。这项工作的目标是搜索和分析冬季中纬度电离层的长期纵向影响及其与低层大气过程的可能联系。材料和方法。这些研究是在使用全球导航卫星网络获得的电离层总电子含量图和全球地表大气压力和温度图的基础上,利用2012-2018年冬季纬度40°N的每日数据进行的。还使用了关于空间天气和磁层的数据(太阳和地磁活动指数)。采用统计分析方法。后果电离层总电子含量的显著纵向极值(高达平均水平的40%)已经确定,它与地表大气压力和温度的变化有关。在所考虑的季节中,这种关系的特征是显著的相关系数在+0.34到+0.48之间。总电子含量的最大值落在具有最大表面大气压力梯度的经度上。空间天气通过地理坐标系和地磁坐标系之间的不匹配而产生的影响也会导致电离层的纵向效应,但不会形成局部极值。结论。所获得的结果表明,低层大气与高层大气和电离层有可能长期或持续相互作用。考虑到总电子含量纵向特征的恒定性,对静止行星波在实现大气-电离层相互作用中的重要作用进行了假设。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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