Liu Jann-Yenq, Wu Tsung-Yu, Lin Chi-Yen, Chang Loren C
Center for Astronautical Physics and Engineering, National Central University, Taoyuan, Taiwan.
Department of Space Science and Engineering, National Central University, Taoyuan, Taiwan.
Sci Rep. 2022 Dec 5;12(1):21003. doi: 10.1038/s41598-022-25449-y.
The semidiurnal (12.42 h) and semimonthly (14.76 days) lunar tides have been well-known by fishermen for several centuries. The gravitational force of the relative positions between the Sun, the Moon, and the Earth results in two symmetrical tidal bulges (double bulges) appearing at equatorial latitudes directly under and opposite the Moon. We utilize ionospheric GNSS (Global Navigation Satellite System) radio occultation soundings to show the global three-dimensional structures and dynamics of the double bulges of ionospheric lunar tides for the first time. The double-bulge amplitude of ionospheric F2-peak height hmF2, lagging the sublunar or antipodal point by about 2-3 h, is about 3-5 km at the equator and 1.5-2.0 km at ± 35° magnetic latitude. The electron density further depicts global three-dimensional plasma flows in the ionosphere.
半日(12.42小时)和半月(14.76天)的太阴潮在几个世纪以来一直为渔民所熟知。太阳、月球和地球相对位置的引力导致在月球正下方和对跖点的赤道纬度处出现两个对称的潮汐隆起(双隆起)。我们首次利用电离层全球导航卫星系统(GNSS)无线电掩星探测来展示电离层太阴潮双隆起的全球三维结构和动力学。电离层F2层峰值高度hmF2的双隆起幅度在赤道处约为3 - 5千米,在磁纬±35°处为1.5 - 2.0千米,滞后于月心或对映点约2 - 3小时。电子密度进一步描绘了电离层中的全球三维等离子体流。