Tidally Driven Intra-Seasonal Oscillations in the Thermosphere From TIEGCM-ICON and Connections to the Madden-Julian Oscillation

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2025-01-23 DOI:10.1029/2024JA033178
Federico Gasperini, Astrid Maute, Houjun Wang, Owen McClung, Deepali Aggarwal, Komal Kumari
{"title":"Tidally Driven Intra-Seasonal Oscillations in the Thermosphere From TIEGCM-ICON and Connections to the Madden-Julian Oscillation","authors":"Federico Gasperini,&nbsp;Astrid Maute,&nbsp;Houjun Wang,&nbsp;Owen McClung,&nbsp;Deepali Aggarwal,&nbsp;Komal Kumari","doi":"10.1029/2024JA033178","DOIUrl":null,"url":null,"abstract":"<p>Recent evidence has revealed that strong coupling between the lower atmosphere and the thermosphere (<span></span><math>\n <semantics>\n <mrow>\n <mo>&gt;</mo>\n </mrow>\n <annotation> ${ &gt;} $</annotation>\n </semantics></math>100 km) occurs on intra-seasonal (IS) timescales (<span></span><math>\n <semantics>\n <mrow>\n <mo>∼</mo>\n </mrow>\n <annotation> ${\\sim} $</annotation>\n </semantics></math> 30–90 days). The Madden-Julian Oscillation (MJO), a key source of IS variability in tropical convection and circulation, influences the generation and propagation of atmospheric tides and is believed to be a significant driver of thermospheric IS oscillations (ISOs). However, limited satellite observations in the “thermospheric gap” (100–300 km) and challenges faced by numerical models in characterizing this region have hindered a comprehensive understanding of this connection. This study uses an Ionospheric Connection Explorer (ICON)-adapted version of the Thermosphere Ionosphere Electrodynamics General Circulation Model, incorporating lower boundary tides from Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI) observations, to quantify the impact of the upward-propagating tidal spectrum on thermospheric ISOs and elucidate connections to the MJO. Thermospheric zonal and diurnal mean zonal winds exhibit prominent (<span></span><math>\n <semantics>\n <mrow>\n <mo>∼</mo>\n </mrow>\n <annotation> ${\\sim} $</annotation>\n </semantics></math> 20 m/s) tidally driven ISOs throughout 2020–2021, largest at low latitudes <span></span><math>\n <semantics>\n <mrow>\n <mo>(</mo>\n <mrow>\n <mo>±</mo>\n <mn>30</mn>\n <mo>°</mo>\n </mrow>\n <mo>)</mo>\n </mrow>\n <annotation> $(\\pm 30{}^{\\circ})$</annotation>\n </semantics></math> near 110–150 km altitude. Correlation analyses confirm a robust connection <span></span><math>\n <semantics>\n <mrow>\n <mo>(</mo>\n <mrow>\n <mi>r</mi>\n <mo>&gt;</mo>\n <mn>0.6</mn>\n </mrow>\n <mo>)</mo>\n </mrow>\n <annotation> $(r &gt; 0.6)$</annotation>\n </semantics></math> between thermospheric ISOs, tides, and the MJO. Additionally, Hovmöller diagrams show eastward tidal propagation consistent with the MJO and concurrent Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) observations. This study demonstrates that vertically propagating tides play a crucial role in linking IS variability from the lower atmosphere to the thermosphere, with the MJO identified as a primary driver of this whole-atmosphere teleconnection. Understanding these connections is vital for advancing our knowledge in space physics, particularly regarding the dynamics of the upper atmosphere and ionosphere.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 1","pages":""},"PeriodicalIF":2.9000,"publicationDate":"2025-01-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024JA033178","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

Recent evidence has revealed that strong coupling between the lower atmosphere and the thermosphere ( > ${ >} $ 100 km) occurs on intra-seasonal (IS) timescales ( ${\sim} $ 30–90 days). The Madden-Julian Oscillation (MJO), a key source of IS variability in tropical convection and circulation, influences the generation and propagation of atmospheric tides and is believed to be a significant driver of thermospheric IS oscillations (ISOs). However, limited satellite observations in the “thermospheric gap” (100–300 km) and challenges faced by numerical models in characterizing this region have hindered a comprehensive understanding of this connection. This study uses an Ionospheric Connection Explorer (ICON)-adapted version of the Thermosphere Ionosphere Electrodynamics General Circulation Model, incorporating lower boundary tides from Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI) observations, to quantify the impact of the upward-propagating tidal spectrum on thermospheric ISOs and elucidate connections to the MJO. Thermospheric zonal and diurnal mean zonal winds exhibit prominent ( ${\sim} $ 20 m/s) tidally driven ISOs throughout 2020–2021, largest at low latitudes ( ± 30 ° ) $(\pm 30{}^{\circ})$ near 110–150 km altitude. Correlation analyses confirm a robust connection ( r > 0.6 ) $(r > 0.6)$ between thermospheric ISOs, tides, and the MJO. Additionally, Hovmöller diagrams show eastward tidal propagation consistent with the MJO and concurrent Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) observations. This study demonstrates that vertically propagating tides play a crucial role in linking IS variability from the lower atmosphere to the thermosphere, with the MJO identified as a primary driver of this whole-atmosphere teleconnection. Understanding these connections is vital for advancing our knowledge in space physics, particularly regarding the dynamics of the upper atmosphere and ionosphere.

查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
从TIEGCM-ICON看热层潮汐驱动的季节内振荡及其与Madden-Julian涛动的关系
最近的证据表明,低层大气和热层之间的强耦合(>;${>} $ 100公里)发生在季节内(IS)时间尺度上(~ ${\sim} $ 30-90天)。麦登-朱利安涛动(MJO)是热带对流和环流中IS变率的一个重要来源,它影响大气潮汐的产生和传播,被认为是热层IS振荡(ISOs)的一个重要驱动因素。然而,在“热层间隙”(100-300公里)有限的卫星观测和数值模式在表征该区域所面临的挑战阻碍了对这种联系的全面理解。本研究使用电离层连接探测器(ICON)的热层电离层电动力学环流模型,结合迈克尔逊全球高分辨率热层成像干涉仪(MIGHTI)观测的下边界潮汐,量化了向上传播的潮汐谱对热层iso的影响,并阐明了与MJO的联系。在2020-2021年期间,热层纬向风和日平均纬向风表现出明显的(~ ${\sim} $ 20 m/s)潮汐驱动的iso,在110-150 km高度附近的低纬度(±30°)$ (\pm 30{}^{\circ})$最大。相关分析证实了两者之间的紧密联系(r >;0.6) $(r >;0.6)$在热层iso,潮汐和MJO之间。此外,Hovmöller图表显示了与MJO一致的向东潮汐传播,以及使用宽带发射辐射测量(SABER)观测的同步大气探测。这项研究表明,垂直传播的潮汐在连接从低层大气到热层的IS变率方面起着至关重要的作用,MJO被认为是这种全大气遥相关的主要驱动因素。了解这些联系对于提高我们在空间物理学方面的知识至关重要,特别是关于高层大气和电离层的动力学。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
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
期刊最新文献
Reduced Geomagnetic Shielding During the Laschamps Excursion and Its Impact on Cosmic-Ray-Induced Atmospheric Radiation Finding the Magnetopause Standoff Distance Using Soft X-Ray Images: Application for the SMILE Mission Kinetic-Based Macro-Modeling of the Solar Wind at Large Heliocentric Distances: Kappa Electrons at the Exobase Great North American Eclipse: A Multi-Platform Study of Ionospheric and Geomagnetic Disturbances on 8 April 2024 Lower Thermospheric Zonal Winds Change Interhemispheric Field-Aligned Current Directions Over Asian-Pacific Region
×
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
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术
文献互助 智能选刊 最新文献 互助须知 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 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1