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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >The influence of atmospheric tide and planetary wave variability during sudden stratosphere warmings on the low latitude ionosphere
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The influence of atmospheric tide and planetary wave variability during sudden stratosphere warmings on the low latitude ionosphere

机译:大气潮和行星的影响波变化在突如其来的平流层也在低纬电离层

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[1] Numerical simulations are performed for a sudden stratosphere warming (SSW) under different atmospheric tide and planetary wave forcing conditions to investigate the tidal variability in the mesosphere and lower thermosphere (MLT). The influence of variability of different tides in the MLT on generating perturbations to the low latitude ionosphere is also investigated. Significant changes are found to occur in the migrating semidiurnal solar (SW2) and lunar (M2) tides as well as in the westward propagating nonmigrating semidiurnal tide with zonal wave number 1 (SW1). The changes in the zonal mean atmosphere that occur during SSWs lead to an enhancement in the SW2 and M2 tides. The vertical wavelength of the SW2 is also changed, resulting in phase variability in the SW2 at a constant altitude. Significant enhancements in the SW1 are found to occur only in the presence of additional planetary wave forcing, and this demonstrates that nonlinear planetary wave-tide interactions lead to the enhanced SW1 during SSWs. The amplitude and phase variability of the SW2 is found to be capable of producing temporal variability in the vertical plasma drift velocity that is similar to the observed variability. Changes in the M2 during SSWs can contribute up to an additional ~30% of the total ionosphere variability; however, the overall influence of the lunar tide is found to be dependent upon the phase of the moon relative to the timing of the SSW. Although the influence is relatively minor, the SW1 also contributes to the low latitude ionosphere variability during SSWs. The simulation results for the vertical plasma drift velocity and total electron content (TEC) further illustrate that significant longitude variability occurs in the ionosphere response to SSWs.
机译:[1]进行了数值模拟突然平流层变暖(f)不同大气潮和行星波强迫条件探讨潮汐变化在中间层和较低的热电离层(MLT)。潮汐变化的影响不同MLT产生扰动的低纬度电离层也是调查。发现显著变化的发生迁移半日太阳能(SW2)和月球(M2)潮汐以及向西传播与纬向波nonmigrating半日潮1号(SW1)。在量导致大气中发生的增强SW2和M2的潮汐。波长的SW2也改变,产生的在阶段变化SW2一个常数高度。发现只出现在附加的存在行星波强迫,这说明行星wave-tide非线性相互作用导致增强SW1量。SW2的振幅和相位变化发现生产时间的能力变化在垂直的等离子体漂移速度这是类似于观察到的变化。平方米的变化量可以贡献一个额外的~电离层总数的30%可变性;月球潮汐是依赖于阶段的月球相对于的时机量。SW1也导致了较低的纬度电离层的变化量。仿真结果的纵向等离子体漂移速度和总电子含量(TEC)说明重要的经度变化发生在电离层响应量。

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