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由于预测的2015年至2065年主磁场变化导致的电离层-热层气候模拟趋势

Simulated Trends in Ionosphere-Thermosphere Climate Due to Predicted Main Magnetic Field Changes From 2015 to 2065.

作者信息

Cnossen I, Maute A

机构信息

British Antarctic Survey Cambridge UK.

National Center for Atmospheric Research Boulder CO USA.

出版信息

J Geophys Res Space Phys. 2020 Mar;125(3):e2019JA027738. doi: 10.1029/2019JA027738. Epub 2020 Mar 13.

Abstract

The strength and structure of the Earth's magnetic field is gradually changing. During the next 50 years the dipole moment is predicted to decrease by 3.5%, with the South Atlantic Anomaly expanding, deepening, and continuing to move westward, while the magnetic dip poles move northwestward. We used simulations with the Thermosphere-Ionosphere-Electrodynamics General Circulation Model to study how predicted changes in the magnetic field will affect the climate of the thermosphere-ionosphere system from 2015 to 2065. The global mean neutral density in the thermosphere is expected to increase slightly, by up to 1% on average or up to 2% during geomagnetically disturbed conditions ( ). This is due to an increase in Joule heating power, mainly in the Southern Hemisphere. Global mean changes in total electron content (TEC) range from 3% to +4%, depending on season and UT. However, regional changes can be much larger, up to about 35% in the region of 45°S to 45°N and 110°W to 0°W during daytime. Changes in the vertical drift are the most important driver of changes in TEC, although other plasma transport processes also play a role. A reduction in the low-latitude upward drift weakens the equatorial ionization anomaly in the longitude sector of 105-60°W, manifesting itself as a local increase in electron density over Jicamarca (12.0°S, 76.9°W). The predicted increase in neutral density associated with main magnetic field changes is very small compared to observed trends and other trend drivers, but the predicted changes in TEC could make a significant contribution to observationally detectable trends.

摘要

地球磁场的强度和结构正在逐渐变化。预计在未来50年内,偶极矩将减少3.5%,南大西洋异常区将扩大、加深并继续向西移动,同时磁倾极向西北移动。我们使用热层-电离层-电动力学通用环流模型进行模拟,以研究预测的磁场变化将如何影响2015年至2065年热层-电离层系统的气候。热层中的全球平均中性密度预计将略有增加,平均增加幅度高达1%,在地磁扰动条件下( )增加幅度高达2%。这是由于焦耳加热功率增加,主要发生在南半球。总电子含量(TEC)的全球平均变化范围为-3%至+4%,具体取决于季节和世界时。然而,区域变化可能要大得多,在白天,南纬45°至北纬45°、西经110°至0°的区域变化幅度高达约35%。垂直漂移的变化是TEC变化的最重要驱动因素,尽管其他等离子体输运过程也起作用。低纬度向上漂移的减少削弱了西经105°至60°经度扇区的赤道电离异常,表现为奇卡马尔卡(南纬12.0°,西经76.9°)上空电子密度的局部增加。与观测趋势和其他趋势驱动因素相比,与主磁场变化相关的中性密度预测增加非常小,但TEC的预测变化可能对可观测到的趋势做出重大贡献。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/51ab/7375146/686aab926121/JGRA-125-e2019JA027738-g001.jpg

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