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来自潮汐、超快速开尔文波及其相互作用的电离层-热层系统变化。

Variations in the ionosphere-thermosphere system from tides, ultra-fast Kelvin waves, and their interactions.

作者信息

Triplett Colin C, Immel Thomas J, Wu Yen-Jung, Cullens Chihoko

机构信息

Space Sciences Laboratory, University of California, Berkeley, Berkeley, CA 94720, USA.

出版信息

Adv Space Res. 2019 Nov 15;64(10):1841-1853. doi: 10.1016/j.asr.2019.08.015. Epub 2019 Aug 23.

DOI:10.1016/j.asr.2019.08.015
PMID:33867620
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC8050945/
Abstract

Large scale waves, such as the atmospheric tides and ultra-fast Kelvin waves (UFKW), have direct effects on the neutral wind and temperature fields of the ionosphere-thermosphere (I-T) system. In this study we examine the response of the I-T system to the atmospheric tides, one UFKW, and the secondary waves generated from their interactions using the Thermosphere-Ionosphere-Electrodynamics General Circulation Model (TIEGCM). We find that forcing an UFKW at the lower boundary of the TIEGCM is all that is required for it to setup in the model. We see variations around 10% in the zonal winds that lead to similar variations in the total electron content (TEC) depending on the phase of the UFKW. From these simulations, we expect the Ionospheric Connection Explorer (ICON) mission will be able to fully capture these wave interactions by observing winds and temperatures at the mesopause and above.

摘要

大规模波动,如大气潮汐和超快速开尔文波(UFKW),对电离层-热层(I-T)系统的中性风场和温度场有直接影响。在本研究中,我们使用热层-电离层-电动力学通用环流模型(TIEGCM),研究I-T系统对大气潮汐、一个UFKW以及它们相互作用产生的二次波的响应。我们发现,在TIEGCM的下边界强迫一个UFKW,是使其在模型中建立起来所需要的全部条件。我们看到纬向风有10%左右的变化,这会导致总电子含量(TEC)根据UFKW的相位产生类似的变化。从这些模拟中,我们预计电离层连接探测器(ICON)任务将能够通过观测中间层顶及以上的风和温度,充分捕捉这些波的相互作用。

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本文引用的文献

1
The Ionospheric Connection Explorer Mission: Mission Goals and Design.电离层连接探测器任务:任务目标与设计
Space Sci Rev. 2018;214. doi: 10.1007/s11214-017-0449-2. Epub 2017 Dec 6.
2
Retrieval of Lower Thermospheric Temperatures from O A Band Emission: The MIGHTI Experiment on ICON.从氧A波段发射中反演低热层温度:ICON卫星上的MIGHTI实验
Space Sci Rev. 2018 Feb;214(1). doi: 10.1007/s11214-017-0434-9. Epub 2017 Nov 30.
3
On the Specification of Upward-Propagating Tides for ICON Science Investigations.关于用于ICON科学研究的向上传播潮汐的规范
Space Sci Rev. 2017 Oct;212(1-2):697-713. doi: 10.1007/s11214-017-0401-5. Epub 2017 Aug 3.
4
Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI): Monolithic Interferometer Design and Test.用于全球高分辨率热层成像的迈克尔逊干涉仪(MIGHTI):单片干涉仪设计与测试
Space Sci Rev. 2017 Oct;212(1-2):601-613. doi: 10.1007/s11214-017-0374-4. Epub 2017 Jun 12.
5
The MIGHTI Wind Retrieval Algorithm: Description and Verification.MIGHTI风场反演算法:描述与验证
Space Sci Rev. 2017 Oct;212(1-2):585-600. doi: 10.1007/s11214-017-0359-3. Epub 2017 Apr 10.
6
Thermosphere-Ionosphere-Electrodynamics General Circulation Model for the Ionospheric Connection Explorer: TIEGCM-ICON.用于电离层连接探测器的热层-电离层-电动力学通用环流模型:TIEGCM-ICON。
Space Sci Rev. 2017 Oct;212(1-2):523-551. doi: 10.1007/s11214-017-0330-3. Epub 2017 Apr 3.
7
Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI): Instrument Design and Calibration.用于全球高分辨率热层成像的迈克尔逊干涉仪(MIGHTI):仪器设计与校准
Space Sci Rev. 2017 Oct;212(1-2):553-584. doi: 10.1007/s11214-017-0358-4. Epub 2017 Apr 20.