Frequency characteristics of the troposphere and ionosphere variations in periods of solar terminator passage

An analysis of the results of lidar observations in the lower atmosphere and observations of the total electron content in the ionosphere (TEC) in Kaliningrad (53°N, 22°E) during the period of solar terminator passage is presented. The observations at troposphere altitudes were performed with a two-wavelength atmospheric lidar (532 and 1064 nm). The ionospheric TEC was determined using signals from GLO-NASS navigation satellites. The observations in the lower atmosphere were performed in February and March 2012, starting ～1 h before sunrise and ending ～1–2 h after sunrise, whereas ionospheric observations were performed continuously throughout the day. Analysis of the spectrum of the observed parameters showed that, during solar terminator passage, the lower atmosphere and ionosphere parameters vary with periods of 4–6 min. Variations of the parameters in the atmosphere with these periods are associated with the propagation of acoustic-gravity waves (AGW). Analysis of the experimental results shows that AGW arise in the lower atmosphere and propagate vertically to ionospheric altitudes. It is assumed that AGW with these periods can be efficiently excited in the lower atmosphere and play an important role in the dynamic interactions between the lower and upper atmosphere.     

Observations of Acoustic Gravity Waves during the Solar Eclipse of March 20, 2015 in Kaliningrad

Results of observations of atmospheric and ionospheric parameters during the solar eclipse of March 20, 2015 have been described. The observations have been conducted by lidar sensing in the lower atmosphere and analysis of the total electron content (TEC) in the ionosphere in Kaliningrad. Observations at the troposphere altitudes have been conducted using an atmospheric lidar. Ionospheric parameter TEC has been determined according to observations of navigation satellite signals. The spectral analysis of the monitored parameters during the solar eclipse has shown that, in the lower atmosphere and the ionosphere in a period range of 2–20 min, internal gravity waves (IGWs) and infrasonic waves are excited. During the main phase of the eclipse, the major contribution to variations in the parameters of the medium comes from infrasonic vibrations. Changes in the variations in the atmospheric and ionospheric parameters with IGW periods are observed only in the initial and final phases of the eclipse.     

A study of propagation of nonlinear acoustic-gravity waves in the middle and upper atmosphere by means of numerical modeling

numerical model of the vertical propagation and decay of nonlinear acoustic-gravity waves (AGW) from the Earth surface to the upper atmosphere is described. Monochromatic vertical velocity variations at the Earth surface are used as the AGW source in the model. The numerical method for solving three-dimensional hydrodynamic equations is based on finite-difference representation of the fundamental laws of conservation, which makes it possible to calculate not only smooth, but also physically correct generalized solutions of the hydrodynamic equations. The equations are solved in a range of altitudes from the ground up to 500 km. The background temperature, density, molecular viscosity and thermal conductivity coefficient are specified according to standard atmosphere models. The dependence of the characteristics of the waves on the amplitude of the wave source at the lower boundary is examined. The amplitudes of the AGW increase with the altitude, and the waves can break down due to nonlinear effects in the middle and upper atmosphere, depending on the amplitude of the source.     

Acoustic-gravity waves in the earth’s atmosphere (review)

We present the modern theory of small-amplitude acoustic-gravity waves (AGWs) in the Earth’s atmosphere. Main attention is paid to the propagation and radiation of AGWs by different sources. We also consider problems of their dissipation, stability, and interaction with the ionospheric plasma. Basic methods of detecting the wave processes in the upper atmosphere in the AGW frequency range are briefly discussed. Experimental data on atmospheric inhomogeneities are compared with theoretical findings. Radiophysical Research Institute, Nizhny Novgorod, Russia. Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 42, No. 1, pp. 3–25, January, 1999.     

Investigation of acoustic gravity waves in the upper atmosphere by the artificial periodic inhomogeneities method at Nizhny Novgorod

We present the results of observation of acoustic gravity waves in the height range 60–120 km. AGW were studied by means of plasma velocity measurements. The observations, based upon use of a newly-developed diagnostic technique, were carried out during September 1990–May 1991. The method uses the artificial periodic inhomogeneities (API) which occur in the ionosphere illuminated by high- power HF radio waves. This method, based upon measurements of phases of waves back scattered from API, has a time resolution sufficient to observe short-term variations in the atmosphere. Seasonal variations of daily averaged vertical velocities were obtained. Above the turbopause height upward vertical motions dominated. Wave-like oscillations in the vertical velocity, which are most probably caused by AGW, occurred.Published from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 39, No. 3, pp. 329–334, March, 1996.     

Acoustic-gravity waves in atmospheric and oceanic waveguides

A theory of guided propagation of sound in layered, moving fluids is extended to include acoustic-gravity waves (AGWs) in waveguides with piecewise continuous parameters. The orthogonality of AGW normal modes is established in moving and motionless media. A perturbation theory is developed to quantify the relative significance of the gravity and fluid compressibility as well as sensitivity of the normal modes to variations in sound speed, flow velocity, and density profiles and in boundary conditions. Phase and group speeds of the normal modes are found to have certain universal properties which are valid for waveguides with arbitrary stratification. The Lamb wave is shown to be the only AGW normal mode that can propagate without dispersion in a layered medium.     

Ultralow-frequency variations of the magnetic field during the propagation of acoustic-gravitaty waves in the ionosphere

The effect of the generation of ULF variations of the magnetic field during the propagation of acoustic-gravitaty waves (AGW) in the ionosphere is analyzed within a simple model. It is shown that AGW-induced ionospheric irregularities can significantly contribute to the ground magnetic field variations. Some changes in ULF variations associated with seismic events are considered as application of this mechanism.     

Acoustic-gravity waves in the Earth’s atmosphere generated by surface sources

The generation of acoustic-gravity waves and their propagation in the Earth’s atmosphere is analyzed numerically on the basis of a computer model of the stratified atmosphere with dissipation. Atmospheric and ionospheric wavelike disturbances from different surface sources such as earthquakes, explosions, seiches, temperature heating, and tsunamis are studied.     

次声波在非均匀大气中的超视距传播特性研究

本文基于Nonlinear Progressive Equation (NPE方程)开展了对非均匀大气中次声波超视距传播特性的研究, 通过数值模拟实验对武汉上空四季次声波传播情况以及路径传输损耗进行了模拟, 获取了次声波在非均匀大气中的超视距传播特性. 计算结果表明, 非均匀大气的性质及其中存在的风对次声波传播有明显的影响, 平流层折射与风速和声波传播方向密切相关, 数值模拟结果表明, 当高斯声源主频为0.1 Hz时, 在不同的背景风场传播条件下, 存在着两个反射高度, 其中40 km 高度反射传输损耗约为25 dB, 110 km反射传输损耗约为50 dB. 关键词： 次声波 超视距传播 非均匀大气 平流层折射     

汤加火山喷发所产生的次声波

2022年1月15日汤加火山发生了剧烈的喷发。在火山喷发后的8 h 39 min,距离火山喷发位置10151 km的昆明次声台阵记录到很强的次声波信号。次声波波列前几个周期平均为443 s,传播速度约为321 m/s,其波形幅度与频率随时间变化与核爆炸产生的次声波形相似。采用相关检测方法估计次声信号的方位角为119°。在持续监测中,还观测到了火山喷发产生的次声信号沿反方向绕地球到达的信号和沿正方向绕地球一周后再次到达的信号。      

Responses of the Ionosphere to the Great Sumatra Earthquake and Volcanic Eruption of Pinatubo

A sudden ionospheric disturbance was detected by the Doppler shift sounding equipment at Beijing, about 25 min later after the outbreak of the Sumatra earthquake on 26 December 2004. This ionospheric disturbance appeared less than lOmin after the earthquake was first recorded at Beijing seismological station by the arrival of the seismic Rayleigh wave. The analysis shows that about 18rain is the time necessary for the seismic Rayleigh wave to propagate from the epicentre to Beijing and then about 5-10min for acoustic waves to propagate from the surface of the Beijing area to the altitude of the ionosphere. Also, a report was made as another example to show the ionospheric response of Doppler shift observation at Beijing area during the Mount Pinatubo eruption of 1991. These two examples show clear evidence of the lithosphere-atmosphere-ionosphere coupling. The former case is in the frequency domain of infrasonic waves of the Earth surface oscillation due to the Rayleigh waves caused by the earthquake, while the latter is in the acoustic-gravity wave category directly excited in the atmosphere by the mass and energy eruptions of Mount Pinatubo.     

Study on generation mechanism of anomalous acoustic-gravity waves before the 2011 Beijing earthquake(M_L=3.0)

Observation results of abnormal acoustic-gravity waves before a Beijing earthquake(M_L=3.0) are presented.During this period,abnormalities of earth surface tilt variations were also recorded.The cross-correlations between the both values are high,which reach maximal values of 0.5 in the area close to the epicenter.The correlations decrease with increasing distances from the epicenter.It was proposed that generation of the anomalous waves may be associated with the pressure and wind perturbations in the air flow caused by slowly shaking mountains during slow surface motion preceding the earthquake in Beijing.Based on the wind velocity data taken from a 350 m meteorological tower in Beijing,the propagation of ducted acoustic-gravity waves in a two-layer model of the atmosphere was numerically simulated.It is shown that characteristic periods,amplitudes and velocities of the simulated phases which were assumed from non-stationary air flow relative to mountains are approximate to the observed phases.A consistency between the simulated results and observation data indicates that a slow surface motion may be a possible source of the anomalous acoustic-gravity waves observed prior to the earthquake.     

Model of interaction between decameter-decimenter radio waves and a strongly inhomogeneous mid-latitude ionosphere

A model of decameter-decimeter radio wave propagation in a strongly inhomogeneous mid-latitude ionosphere is constructed using a modified method of radio wave refractive scattering. The model establishes the relationship between the basic statistical radio wave characteristics and the turbulence parameters of the upper ionosphere. Different aspects of the theory of radio wave refractive scattering are considered in application to the study of amplitude and phase fluctuations of decameter-decimeter radio waves propagating in a three-dimensional randomly inhomogeneous ionosphere with an arbitrary electron density distribution. Radiophysical Research Institute, Nizhny Novgorod, Russia. Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 40, No. 11, pp. 1323–1341, November, 1997.     

北京一次小震级地震前异常声-重力波产生机理的研究

观测到北京一次小震级地震(ML=3.0)前的异常声-重力波,并同时记录到异常地表倾斜信号。二者相关系数比较高,在接近震中的地区相关系数达到最大值0.5,相关系数随着远离震中的距离增大而减小。经过研究表明,异常声-重力波的产生与震前的地表缓慢活动引发的山体缓慢晃动导致的气流风速波动变化有关。基于350 m高的气象铁塔观测的风速数据,对两层大气模型传播的声-重力波进行了数值计算,得到的相对山体非平稳气流引起的声-重力波与观测信号在特征周期、幅度和速度三个参数上近似。以地表倾斜为例的模型与观测数据的一致性表明该震前声-重力波与地震存在关联性。      

On small-scale plasma inhomogeneities of the traveling ionospheric disturbances

We report on the results of the first special experiment on radio sounding of the midlatitude ionosphere by signals from in-orbit satellites at a frequency of 150 MHz under quiet geophysical conditions. Along with the conventional correlation processing, fractal processing of the received signals was also performed. Using the fractal approach, we obtained first data on the sources and generation mechanisms of small-scale plasma inhomogeneities of the traveling ionospheric disturbances (TIDs) in the upper ionosphere. It is noted that the phenomenon of nonlinear “ breaking” of the acoustic-gravity waves entering the ionosphere from the underlying atmosphere plays the crucial role in the formation of plasma inhomogeneities of the TIDs. __________ Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 49, No. 7, pp. 561–569, July 2006.     

Wave ionosphere perturbations with small periods under magnetic storm conditions

The characteristics of total electron content (TEC) variations obtained using the data of middle-latitude stations for receiving GPS satellite signals were studied. An analysis showed that perturbations of diurnal TEC variations during a geomagnetic storm were determined by strengthening of harmonics with periods of 4–5 and 6–8 h. Perturbations in diurnal TEC variations were retained for several days after a geomagnetic storm. An analysis of the frequency and amplitude characteristics of perturbed variations showed that differences between variations at different latitudes could be explained by the propagation of Poincaré planetary waves in an atmospheric wave channel. The atmospheric channel was formed because of increased heating of pole regions during geomagnetic storms. A comparative analysis of observations made at different stations was used to estimate the width of the atmospheric channel and Poincaré wave frequencies and wave vector components.     

Infrasonic waves generated from the volcano eruption in Tonga

The Hunga-Tonga-Hunga-Ha'apai volcano in Tonga erupted violently on January 15, 2022. After 8 hours and 39 minutes, an infrasound array in Kunming at a distance of 10151 km away from the volcano recorded a sequence of strong infrasonic waves. The average period of the first four infrasonic waves is 443 s with propagation speed of 321 m/s. The azimuth angle of this event has been estimated by applying the progressive multi-channel correlation(PMCC) method to process the received signals. During continuous monitoring, the infrasonic waves propagating along and opposite to the direction towards the Kunming array around the earth are recorded respectively.     

Solar-Atmosphere Oscillations due to the Instability of Acoustic-Gravity Waves

In this paper, we study the possibility for generating oscillations of the nonisothermal solar atmosphere. Analytical solutions describing wave perturbations in the entire solar atmosphere are sought for the first time. Based on the model temperature profile, we find an analytical dependence for the fundamental mode of fast acoustic-gravity waves and draw a conclusion on the limiting acoustic frequency in the solar atmosphere. Using this solution, we study the instability of acoustic-gravity waves, estimate the instability parameters, and compare them with the characteristics of the five-minute oscillations of the solar atmosphere.     

Effect of Acoustic Gravity Waves on Variations in the Lower-Ionosphere Parameters as Observed using Artificial Periodic Inhomogeneities

We study the effect of acoustic gravity waves on variations in the atmospheric parameters of the lower ionosphere. The observations were carried out by the method of radio-wave scattering on artificial periodic inhomogeneities of the ionospheric plasma, induced by powerful radio-wave heating of the ionosphere. Measuring the altitude profile of the relaxation time of the scattered signal allowed us to determine the atmospheric temperature and density at heights 95 to 120 km, while recording the signal phase made it possible to obtain the vertical velocity of the plasma. The joint analysis of variations in the vertical velocity and the atmospheric temperature and density showed the simultaneous existence of oscillations with the same periods ranging from 5–10 min to a few hours. The amplitudes of these oscillations were, respectively, 1.5 to 4 m s^-1 for the vertical velocity and 6–20% for the temperature and density. We simulate the characteristics of acoustic gravity waves using the linear theory of their free propagation in an unbounded isothermal undisturbed atmosphere. Based on the polarization relations for low-frequency waves, we calculate the corresponding relative amplitudes of variations in the atmospheric temperature and density with periods from 15 min to 4 h using the measured amplitudes of the vertical velocity. Comparison of the calculation results with the measured values shows their good agreement for waves with periods 15–30 min.     

Simulation of seismo-ionospheric effects initiated by internal gravity waves

Experimental studies have repeatedly demonstrated that, a few days before a strong earthquake, local increases (sometimes decreases) in the electron density in the ionosphere over the epicentral area emerge. Simulations with the help of the GSM TIP (global self-consistent model “Thermosphere-Ionosphere-Protonosphere”) and UAM (Upper Atmosphere Model) models show that account of local disturbances of the zonal electric fields makes it possible to reproduce the morphology of ionospheric disturbances. However, these model experiments do not explain the formation of such ionospheric features over the epicentral area of the impending earthquake. In this paper, we propose a mechanism for the formation of ionospheric disturbances before strong earthquakes due to propagation and dissipation of small-scale internal gravity waves (IGWs) in the upper atmosphere. Using the GSM TIP model, we calculated the ionospheric parameters with account of small-scale IGWs in the near-epicenter area. It is shown that disturbances in the TEC (total electron content) predicted by calculations are in satisfactory agreement with observations from GPS (Global Position System) satellites before the strong mid-latitude earthquake in Greece on January 8, 2006.