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TIDI视线风与ICON - MIGHTI测量值的比较。

Comparison of TIDI Line of Sight Winds With ICON-MIGHTI Measurements.

作者信息

Wu Chen, Ridley Aaron J

机构信息

Climate and Space Sciences and Engineering University of Michigan Ann Arbor MI USA.

出版信息

J Geophys Res Space Phys. 2023 Feb;128(2):e2022JA030910. doi: 10.1029/2022JA030910. Epub 2023 Feb 2.

Abstract

The Thermosphere-Ionosphere-Mesosphere Energetics and Dynamics (TIMED) satellite has been making observations of the mesosphere and lower thermosphere (MLT) region for two decades. The TIMED Doppler Interferometer (TIDI) measures the neutral winds using four orthogonal telescopes. In this study, the line of sight (LOS) winds from individual telescopes are compared to the measurements from the Ionospheric Connection Explorer's (ICON's) Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI) instrument from 90 to 100 km altitude during 2020. With the MIGHTI vector winds projected onto the LOS direction of each TIDI telescope, coincidences of the two data sets are found. The four telescopes perform differently and the performance depends on the satellite configuration and local solar zenith angle. Measurements from the coldside telescopes, Telescope 1 (Tel1) and Telescope 2 (Tel2), are better correlated with the MIGHTI winds in general with Tel2 having higher correlation coefficients across all conditions. The performance of Tel1 is comparable to that of Tel2 during backward flight while showing systematic errors larger than the average wind speeds during forward flight. The warmside LOS winds from Telescope 3 (Tel3) and Telescope 4 (Tel4) vary widely in magnitude, especially on the nightside. Compared with MIGHTI winds, the Tel4 measurements have the weakest correlation, while the Tel3 performance is comparable to that of the coldside telescopes during the ascending phase but deteriorates during the descending phase. Based on the TIDI/MIGHTI comparisons, figures of merit are generated to quantify the quality of measurements from individual telescopes in different configurations.

摘要

热层-电离层-中间层能量学与动力学(TIMED)卫星已经对中间层和低热层(MLT)区域进行了二十年的观测。TIMED多普勒干涉仪(TIDI)使用四个正交望远镜测量中性风。在本研究中,将各个望远镜的视线(LOS)风与电离层连接探测器(ICON)的用于全球高分辨率热层成像的迈克尔逊干涉仪(MIGHTI)仪器在2020年90至100千米高度的测量结果进行了比较。通过将MIGHTI矢量风投影到每个TIDI望远镜的LOS方向上,发现了两个数据集的一致性。四个望远镜的表现各不相同,其性能取决于卫星配置和当地太阳天顶角。一般来说,冷侧望远镜(望远镜1(Tel1)和望远镜2(Tel2))的测量结果与MIGHTI风的相关性更好,在所有条件下Tel2的相关系数更高。Tel1在倒飞期间的性能与Tel2相当,而在正飞期间显示出比平均风速更大的系统误差。望远镜3(Tel3)和望远镜4(Tel4)的暖侧LOS风在大小上变化很大,尤其是在夜间。与MIGHTI风相比,Tel4的测量结果相关性最弱,而Tel3在上升阶段的性能与冷侧望远镜相当,但在下降阶段会变差。基于TIDI/MIGHTI的比较,生成了品质因数以量化不同配置下各个望远镜测量的质量。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2f03/10078375/b61f2f812556/JGRA-128-0-g012.jpg

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