{"title":"太阳活动影响下对流层和平流层下层27天纬向风波动","authors":"I. G. Zakharov, L. F. Chernogor","doi":"10.3103/S0884591325010052","DOIUrl":null,"url":null,"abstract":"<p>Longitudinal, latitudinal, and altitudinal features of the zonal wind in the Northern Hemisphere under the influence of 27-day variations of solar activity (SA) were studied. The research aims to improve the accuracy of weather forecasts and deepening our knowledge about dynamic processes of the interaction of atmospheric layers. Zonal wind data by 5° latitude from the website https://psn.noaa.gov at the longitudes of Europe and North America from 15 altitude levels (from 1000 to 10 hPa) and SA data from the website https://www-app3.gfz-potsdam.de were used. Twenty high-amplitude 27-day SA cycles during the decline phase of the 23rd 11-year solar cycle from 2002 to 2004 were studied. The average 27-day wind changes for each latitude and altitude are calculated by the superposed epoch analysis separately for the winter and summer seasons. For the first time, 27-day latitudinal and altitudinal variations of zonal wind with an amplitude of ~8 m/s, capable of influencing the weather in the extratropical atmosphere, were established. Despite the significant difference in the background wind field in winter and summer, the response of the wind field to SA influence is similar for both seasons. The maximum wind changes occur in the southern part of the polar atmospheric cell and the northern part of the Ferrell cell (50°–70° N) and gradually decrease in magnitude to the south and north. Wind changes are many times smaller in the tropical troposphere. At the boundaries of the global circulation cells, the direction of disturbed wind changes to the opposite. Changes in the position of jet streams by more than 1° in latitude and changes in the size of atmospheric circulation cells are also observed. In terms of height, the largest changes in the wind at all latitudes occur in the upper troposphere. There is a close relationship between the magnitude of the perturbed wind and changes in the tropopause height. The impact is realized through two-way dynamic stratospheric-tropospheric interaction, primarily in the area of the polar night jet and polar front jet stream. The presence of significant wind changes for the summer season indicates an important role not only of planetary-scale Rossby waves but also of shorter-wavelength waves. At the same time, their upward propagation can be ensured by nonlinear interaction between them.</p>","PeriodicalId":681,"journal":{"name":"Kinematics and Physics of Celestial Bodies","volume":"41 1","pages":"14 - 25"},"PeriodicalIF":0.5000,"publicationDate":"2025-02-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Twenty-Seven-Day Zonal Wind Fluctuations in the Troposphere and Lower Stratosphere under the Influence of Solar Activity\",\"authors\":\"I. G. Zakharov, L. F. Chernogor\",\"doi\":\"10.3103/S0884591325010052\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>Longitudinal, latitudinal, and altitudinal features of the zonal wind in the Northern Hemisphere under the influence of 27-day variations of solar activity (SA) were studied. The research aims to improve the accuracy of weather forecasts and deepening our knowledge about dynamic processes of the interaction of atmospheric layers. Zonal wind data by 5° latitude from the website https://psn.noaa.gov at the longitudes of Europe and North America from 15 altitude levels (from 1000 to 10 hPa) and SA data from the website https://www-app3.gfz-potsdam.de were used. Twenty high-amplitude 27-day SA cycles during the decline phase of the 23rd 11-year solar cycle from 2002 to 2004 were studied. The average 27-day wind changes for each latitude and altitude are calculated by the superposed epoch analysis separately for the winter and summer seasons. For the first time, 27-day latitudinal and altitudinal variations of zonal wind with an amplitude of ~8 m/s, capable of influencing the weather in the extratropical atmosphere, were established. Despite the significant difference in the background wind field in winter and summer, the response of the wind field to SA influence is similar for both seasons. The maximum wind changes occur in the southern part of the polar atmospheric cell and the northern part of the Ferrell cell (50°–70° N) and gradually decrease in magnitude to the south and north. Wind changes are many times smaller in the tropical troposphere. At the boundaries of the global circulation cells, the direction of disturbed wind changes to the opposite. Changes in the position of jet streams by more than 1° in latitude and changes in the size of atmospheric circulation cells are also observed. In terms of height, the largest changes in the wind at all latitudes occur in the upper troposphere. There is a close relationship between the magnitude of the perturbed wind and changes in the tropopause height. The impact is realized through two-way dynamic stratospheric-tropospheric interaction, primarily in the area of the polar night jet and polar front jet stream. The presence of significant wind changes for the summer season indicates an important role not only of planetary-scale Rossby waves but also of shorter-wavelength waves. 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引用次数: 0
摘要
研究了太阳活动27天变化对北半球纬向风的纵向、纬向和纬向特征的影响。这项研究旨在提高天气预报的准确性,加深我们对大气各层相互作用动态过程的认识。使用了欧洲和北美经度15个海拔高度(1000至10 hPa)的5°纬向风资料https://psn.noaa.gov和来自https://www-app3.gfz-potsdam.de网站的SA资料。研究了2002 ~ 2004年第23个11年太阳活动周期衰退期的20个高振幅27 d SA周期。每个纬度和海拔的平均27天风变化是通过冬季和夏季的叠加年代分析分别计算出来的。首次建立了能够影响温带大气天气的~8 m/s纬向风的27 d纬向和高度变化。尽管冬季和夏季背景风场存在显著差异,但两个季节风场对SA影响的响应相似。最大的风变化发生在极大气单体的南部和Ferrell单体的北部(50°~ 70°N),并向南和向北逐渐减弱。在热带对流层,风的变化要小很多倍。在全球环流单元的边界,扰动风的方向改变为相反的方向。还观测到急流位置在纬度上的变化超过1°,以及大气环流单体大小的变化。就高度而言,所有纬度上风的最大变化发生在对流层上层。扰动风的大小与对流层顶高度的变化有密切的关系。这种影响是通过平流层-对流层的双向动态相互作用实现的,主要发生在极夜急流和极锋急流区域。夏季显著的风向变化表明,不仅行星尺度的罗斯比波,短波长的波也起着重要作用。同时,它们之间的非线性相互作用保证了它们的向上传播。
Twenty-Seven-Day Zonal Wind Fluctuations in the Troposphere and Lower Stratosphere under the Influence of Solar Activity
Longitudinal, latitudinal, and altitudinal features of the zonal wind in the Northern Hemisphere under the influence of 27-day variations of solar activity (SA) were studied. The research aims to improve the accuracy of weather forecasts and deepening our knowledge about dynamic processes of the interaction of atmospheric layers. Zonal wind data by 5° latitude from the website https://psn.noaa.gov at the longitudes of Europe and North America from 15 altitude levels (from 1000 to 10 hPa) and SA data from the website https://www-app3.gfz-potsdam.de were used. Twenty high-amplitude 27-day SA cycles during the decline phase of the 23rd 11-year solar cycle from 2002 to 2004 were studied. The average 27-day wind changes for each latitude and altitude are calculated by the superposed epoch analysis separately for the winter and summer seasons. For the first time, 27-day latitudinal and altitudinal variations of zonal wind with an amplitude of ~8 m/s, capable of influencing the weather in the extratropical atmosphere, were established. Despite the significant difference in the background wind field in winter and summer, the response of the wind field to SA influence is similar for both seasons. The maximum wind changes occur in the southern part of the polar atmospheric cell and the northern part of the Ferrell cell (50°–70° N) and gradually decrease in magnitude to the south and north. Wind changes are many times smaller in the tropical troposphere. At the boundaries of the global circulation cells, the direction of disturbed wind changes to the opposite. Changes in the position of jet streams by more than 1° in latitude and changes in the size of atmospheric circulation cells are also observed. In terms of height, the largest changes in the wind at all latitudes occur in the upper troposphere. There is a close relationship between the magnitude of the perturbed wind and changes in the tropopause height. The impact is realized through two-way dynamic stratospheric-tropospheric interaction, primarily in the area of the polar night jet and polar front jet stream. The presence of significant wind changes for the summer season indicates an important role not only of planetary-scale Rossby waves but also of shorter-wavelength waves. At the same time, their upward propagation can be ensured by nonlinear interaction between them.
期刊介绍:
Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.