地磁扰动对中纬度中层/低热层平均风和潮汐的影响

IF 0.6 Q4 ENGINEERING, ELECTRICAL & ELECTRONIC
C. Jacobi, F. Lilienthal, D. Korotyshkin, E. Merzlyakov, G. Stober
{"title":"地磁扰动对中纬度中层/低热层平均风和潮汐的影响","authors":"C. Jacobi, F. Lilienthal, D. Korotyshkin, E. Merzlyakov, G. Stober","doi":"10.5194/EGUSPHERE-EGU21-3163","DOIUrl":null,"url":null,"abstract":"<p>Observations of upper mesosphere/lower thermosphere (MLT) wind have been performed at Collm (51&#176;N, 13&#176;E) and Kazan (56&#176;N, 49&#176;E), using two SKiYMET all-sky meteor radars with similar configuration. Daily vertical profiles of mean winds and tidal amplitudes have been constructed from hourly horizontal winds. We analyze the response of mean winds and tidal amplitudes to geomagnetic disturbances. To this end we compare winds and amplitudes for very quiet (Ap &#8804; 5) and unsettled/disturbed (Ap &#8805; 20) geomagnetic conditions. Zonal winds in both the mesosphere and lower thermosphere are weaker during disturbed conditions for both summer and winter. The summer equatorward meridional wind jet is weaker for disturbed geomagnetic conditions. Tendencies over Collm and Kazan for geomagnetic effects on mean winds qualitatively agree during most of the year. For the diurnal tide, amplitudes in summer are smaller in the mesosphere but greater in the lower thermosphere, but no clear tendency is seen for winter. Semidiurnal tidal amplitudes increase during geomagnetic active days in summer and winter. Terdiurnal amplitudes are slightly reduced in the mesosphere during disturbed days, but no clear effect is visible for the lower thermosphere. Overall, while there is a noticeable effect of geomagnetic variability on the mean wind, the effect on tidal amplitudes, except for the semidiurnal tide, is relatively small and partly different over Collm and Kazan.</p>","PeriodicalId":45093,"journal":{"name":"Advances in Radio Science","volume":null,"pages":null},"PeriodicalIF":0.6000,"publicationDate":"2021-03-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"Influence of geomagnetic disturbances on midlatitude mesosphere/lower thermosphere mean winds and tides \",\"authors\":\"C. Jacobi, F. Lilienthal, D. Korotyshkin, E. Merzlyakov, G. Stober\",\"doi\":\"10.5194/EGUSPHERE-EGU21-3163\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>Observations of upper mesosphere/lower thermosphere (MLT) wind have been performed at Collm (51&#176;N, 13&#176;E) and Kazan (56&#176;N, 49&#176;E), using two SKiYMET all-sky meteor radars with similar configuration. Daily vertical profiles of mean winds and tidal amplitudes have been constructed from hourly horizontal winds. We analyze the response of mean winds and tidal amplitudes to geomagnetic disturbances. To this end we compare winds and amplitudes for very quiet (Ap &#8804; 5) and unsettled/disturbed (Ap &#8805; 20) geomagnetic conditions. Zonal winds in both the mesosphere and lower thermosphere are weaker during disturbed conditions for both summer and winter. The summer equatorward meridional wind jet is weaker for disturbed geomagnetic conditions. Tendencies over Collm and Kazan for geomagnetic effects on mean winds qualitatively agree during most of the year. For the diurnal tide, amplitudes in summer are smaller in the mesosphere but greater in the lower thermosphere, but no clear tendency is seen for winter. Semidiurnal tidal amplitudes increase during geomagnetic active days in summer and winter. Terdiurnal amplitudes are slightly reduced in the mesosphere during disturbed days, but no clear effect is visible for the lower thermosphere. Overall, while there is a noticeable effect of geomagnetic variability on the mean wind, the effect on tidal amplitudes, except for the semidiurnal tide, is relatively small and partly different over Collm and Kazan.</p>\",\"PeriodicalId\":45093,\"journal\":{\"name\":\"Advances in Radio Science\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.6000,\"publicationDate\":\"2021-03-03\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Advances in Radio Science\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.5194/EGUSPHERE-EGU21-3163\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"ENGINEERING, ELECTRICAL & ELECTRONIC\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Advances in Radio Science","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.5194/EGUSPHERE-EGU21-3163","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ENGINEERING, ELECTRICAL & ELECTRONIC","Score":null,"Total":0}
引用次数: 1

摘要

使用两个具有类似配置的SKiYMET全天空流星雷达,在Collm(51°;N,13°;E)和Kazan(56°;北,49°;E)进行了上中层/下热层(MLT)风的观测。平均风和潮汐振幅的每日垂直剖面是根据每小时的水平风构建的。我们分析了平均风和潮汐振幅对地磁扰动的响应。为此,我们比较了非常安静(Ap≤;5)和不稳定/扰动(ApͰ;20)地磁条件下的风和振幅。在夏季和冬季的扰动条件下,中间层和较低热层的带状风较弱。夏季赤道向经向风急流在地磁扰动条件下较弱。在一年中的大部分时间里,科尔姆和喀山地磁对平均风影响的趋势在质量上一致。对于昼夜潮,夏季中层的振幅较小,但较低热层的振幅较大,但冬季没有明显的趋势。在夏季和冬季地磁活跃期间,半日潮振幅增加。在受干扰的日子里,中间层的昼夜振幅略有降低,但较低的热层没有明显的影响。总的来说,虽然地磁变化对平均风有明显影响,但对潮汐振幅的影响(半日潮除外)相对较小,并且在科尔姆和喀山有部分不同。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Influence of geomagnetic disturbances on midlatitude mesosphere/lower thermosphere mean winds and tides 

Observations of upper mesosphere/lower thermosphere (MLT) wind have been performed at Collm (51°N, 13°E) and Kazan (56°N, 49°E), using two SKiYMET all-sky meteor radars with similar configuration. Daily vertical profiles of mean winds and tidal amplitudes have been constructed from hourly horizontal winds. We analyze the response of mean winds and tidal amplitudes to geomagnetic disturbances. To this end we compare winds and amplitudes for very quiet (Ap ≤ 5) and unsettled/disturbed (Ap ≥ 20) geomagnetic conditions. Zonal winds in both the mesosphere and lower thermosphere are weaker during disturbed conditions for both summer and winter. The summer equatorward meridional wind jet is weaker for disturbed geomagnetic conditions. Tendencies over Collm and Kazan for geomagnetic effects on mean winds qualitatively agree during most of the year. For the diurnal tide, amplitudes in summer are smaller in the mesosphere but greater in the lower thermosphere, but no clear tendency is seen for winter. Semidiurnal tidal amplitudes increase during geomagnetic active days in summer and winter. Terdiurnal amplitudes are slightly reduced in the mesosphere during disturbed days, but no clear effect is visible for the lower thermosphere. Overall, while there is a noticeable effect of geomagnetic variability on the mean wind, the effect on tidal amplitudes, except for the semidiurnal tide, is relatively small and partly different over Collm and Kazan.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Advances in Radio Science
Advances in Radio Science ENGINEERING, ELECTRICAL & ELECTRONIC-
CiteScore
0.90
自引率
0.00%
发文量
3
审稿时长
45 weeks
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信