Lieberman Ruth S, Harding Brian J, Heelis Roderick A, Pedatella Nicholas M, Forbes Jeffrey M, Oberheide Jens
NASA Goddard Space Flight Center Greenbelt MD USA.
University of California Berkeley CA USA.
Geophys Res Lett. 2022 Jun 16;49(11):e2022GL098078. doi: 10.1029/2022GL098078. Epub 2022 May 31.
We present simultaneous, independent measurements of the atmospheric semidiurnal lunar tide in neutral winds and plasma velocities from NASA's Ionospheric Connection Explorer, and in atomic oxygen 135.6 nm airglow measured by the Global-scale Observations of the Limb and Disk. Westward tidal winds near 115 km at the magnetic equator occur during part of the upward phase of the in-situ plasma drift. Vertical motions associated with the field-aligned plasma velocity occur away from the magnetic equator. The morphology of the lunar tide, and the phasing between the airglow and plasma velocities are consistent with × drift as a mechanism for linking neutral wind and plasma perturbations. This work provides the first observational quantification of global-scale E- and F-region coupling through × and field-aligned vertical drifts.
我们展示了来自美国国家航空航天局电离层连接探测器对中性风及等离子体速度中大气半日太阴潮的同步、独立测量结果,以及通过全球尺度临边和盘面观测对原子氧135.6纳米气辉的测量结果。在磁赤道附近115千米处,向西的潮汐风出现在原位等离子体漂移向上阶段的部分时间。与场向等离子体速度相关的垂直运动出现在远离磁赤道的地方。太阴潮的形态以及气辉和等离子体速度之间的相位与作为连接中性风与等离子体扰动机制的×漂移一致。这项工作首次对通过×和场向垂直漂移实现的全球尺度E区和F区耦合进行了观测量化。