On the importance of middle atmosphere observations on ionospheric dynamics using WACCM-X and SAMI3

IF 1.7 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Annales Geophysicae Pub Date : 2024-01-03 DOI:10.5194/egusphere-2023-3065
Fabrizio Sassi, Angeline Burrell, Sarah McDonald, Jennifer Tate, John McCormack
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Abstract

Abstract. Recent advances in atmospheric observations and modelling have enabled the investigation of thermosphere-ionosphere interactions as a whole atmosphere problem. This study examines how dynamical variability in the middle atmosphere (MA) affects day-to-day changes in the thermosphere and ionosphere. Specifically, this study investigates ionosphere-thermosphere interactions during different time periods of January 2013 using the Specified Dynamics Whole Atmosphere Community Climate Model, eXtended version (WACCM-X) coupled to the Naval Research Laboratory (NRL) ionosphere of the Sami3 is Another Model of the Ionosphere (SAMI3) model. To represent the weather of the day, the coupled thermosphere-ionosphere system is nudged below 90 km toward the atmospheric specifications provided by the Navy Global Environmental Model for High-Altitude (NAVGEM-HA). Hindcast simulations during January 2013 are carried out with the full data set of observations normally assimilated by NAVGEM-HA, and with a degraded dataset where observations above 40 km are not assimilated. Ionospheric regions with statistically significant changes are identified using key ionospheric properties, including the electron density, peak electron density, and height of the peak electron density. Ionospheric changes show a spatial structure that illustrates the impact of two different types of coupling between the thermosphere and the ionosphere: wind-dynamo coupling through electric conductivity and ion-neutral interactions in the upper thermosphere. The two simulations presented in this study show that changing the state of the MA affects ionosphere-thermosphere coupling through changes in the behavior and amplitude of non-migrating tides, resulting in improved key ionospheric specifications.
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利用 WACCM-X 和 SAMI3 研究中间层大气观测对电离层动力学的重要性
摘要大气观测和建模的最新进展使人们能够把热层-电离层的相互作用作为一个整体大气问题来研究。本研究探讨了中间层大气(MA)的动态变化如何影响热层和电离层的逐日变化。具体来说,本研究使用指定动力学全大气层群气候模式扩展版(WACCM-X)与海军研究实验室(NRL)电离层的 Sami3 is Another Model of the Ionosphere(SAMI3)模式耦合,研究了 2013 年 1 月不同时段的电离层-热层相互作用。为了表现当天的天气,热层-电离层耦合系统被推至 90 公里以下,以符合海军高空全球环境模式(NAVGEM-HA)提供的大气规范。2013 年 1 月期间的后报模拟使用了 NAVGEM-HA 通常同化的完整观测数据集,以及未同化 40 公里以上观测数据的降级数据集。利用电离层的关键属性,包括电子密度、电子密度峰值和电子密度峰值高度,确定了在统计上有显著变化的电离层区域。电离层的变化显示了一种空间结构,说明了热层和电离层之间两种不同类型耦合的影响:通过电导率的风-动力耦合和热层上部的离子-中性相互作用。本研究提出的两个模拟结果表明,改变千年生态系统评估的状态会通过改变非迁移潮的行为和振幅影响电离层-热层耦合,从而改善电离层的关键指标。
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来源期刊
Annales Geophysicae
Annales Geophysicae 地学-地球科学综合
CiteScore
4.30
自引率
0.00%
发文量
42
审稿时长
2 months
期刊介绍: Annales Geophysicae (ANGEO) is a not-for-profit international multi- and inter-disciplinary scientific open-access journal in the field of solar–terrestrial and planetary sciences. ANGEO publishes original articles and short communications (letters) on research of the Sun–Earth system, including the science of space weather, solar–terrestrial plasma physics, the Earth''s ionosphere and atmosphere, the magnetosphere, and the study of planets and planetary systems, the interaction between the different spheres of a planet, and the interaction across the planetary system. Topics range from space weathering, planetary magnetic field, and planetary interior and surface dynamics to the formation and evolution of planetary systems.
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