Model study of the effect of the main ionospheric trough on oblique HF radiowave propagation

The purpose of this paper is to study the effect of the main ionospheric trough location on the form of oblique sounding ionograms on the Murmansk-St. Petersburg subauroral radio path. Using a mathematical model of the high-latitude ionosphere, we have calculated four different distributions of electron density along the radio path. One of the distributions has been obtained when the trough is absent, and the remaining three distributions contain troughs of approximately identical depth and width but located at different distances from the ends of the radio path. Using the program of two-dimensional ray tracing, we numerically synthesized oblique-incidence ionograms for each of the four obtained distributions of electron density. The calculations have shown that the location of the main ionospheric trough affects considerably the shape of oblique-incidence ionograms.     

利用射线追踪方法研究化学物质释放对高频加热的聚焦效应

电离层化学物质释放能导致释放区域电子密度的损耗,从而产生明显的电离层空洞现象.高频电波通过电离层空洞时,由于电子密度不同,对电波产生折射效果进而形成聚焦效应.本文利用射线追踪方法,评估高频电波通过空洞形成聚焦加热的效果.结果表明,释放水分子与SF6都能对电离层产生明显的空洞,空洞半径约为25~50 km,电子密度的损耗率10%以上,在释放点附近有时能达到90%.不同摩尔数的化学物质释放能带来不同的效果.在300 km高度释放100 mol的水分子并且高频电波频率为15 MHz时聚焦效果最好.聚焦后电波能量吸收可增加10 dB左右,增幅达两倍左右.加热后的温度可以提升约20%.     

Investigation of the relationship between optical auroral forms and HF radar E region backscatter

The SuperDARN HF radars have been employed in the past to investigate the spectral characteristics of coherent backscatter from L-shell aligned features in the auroral E region. The present study employs all-sky camera observations of the aurora from Husafell, Iceland, and the two SuperDARN radars located on Iceland, Þykkvibær and Stokkseyri, to determine the optical signature of such backscatter features. It is shown that, especially during quiet geomagnetic conditions, the backscatter region is closely associated with east-west aligned diffuse auroral features, and that the two move in tandem with each other. This association between optical and radar aurora has repercussions for the instability mechanisms responsible for generating the E region irregularities from which radars scatter. This is discussed and compared with previous studies investigating the relationship between optical and VHF radar aurora. In addition, although it is known that E region backscatter is commonly observed by SuperDARN radars, the present study demonstrates for the first time that multiple radars can observe the same feature to extend over at least 3 h of magnetic local time, allowing precipitation features to be mapped over large portions of the auroral zone.     

Effects of substorms during HF propagation in the auroral oval

The specific features of radio propagation from the viewpoint of physics of processes in the polar ionosphere have been studied in the present work based on the oblique-incidence sounding of the ionosphere (OISI) on the St. Petersburg-Belyi Nos (Amderma) polar radio path during substorm activity in the summer months of 1997. The OISI data were used to find the following parameters: maximum observable frequency during signal reflection from the E _s layer (EsMOF), maximum observable frequency during signal reflection from the F ₂ layer (F2MOF), and lowest observable frequencies for the E _s and F ₂ layers (EsLOF and F2LOF, respectively). Absolute MOF and LOF values were also found out. The total number of received rays was determined in addition to the above parameters. Isolated substorms against a quiet background were selected for the studies. These substorms resulted in substantial changes in the ionospheric radio channel and propagation conditions along the path. The results of the studies are as follows. (1) The following distinct regularities in the HF propagation along the path have been determined: (i) the range of operational frequencies Δ = MOF-LOF becomes substantially narrower during substorms; (ii) the radio propagation mechanism changes during a substorm; (iii) during substorms, the auroral absorption substantially and partially increases in the course of the expansion and recovery phases, respectively; (iv) multiray effect sharply increases at the beginning of the substorm active phase (T ₀). (2) The indications of changes in the radio propagation parameters, which can possibly be used to predict the beginning of substorm development, have been formulated. (3) All revealed regularities in the HF propagation in the auroral zone have been explained from the geophysical viewpoint. It is important to use these regularities to organize radio communication and to solve the problems within the scope of the Space Weather Program.     

Interpretation of experimental data on HF propagation on the St. Petersburg-Spitsbergen path

The experimental ionograms of the oblique-incidence sounding of the ionosphere, obtained on the St. Petersburg-Spitsbergen high-latitude HF radio path during the magnetically quiet period December 14–15, 2001, are compared with the model calculations of radiowave trajectories. For this purpose, the corresponding oblique-incidence ionograms are numerically synthesized using the technique based on the shooting method and the computer program for constructing HF radiowave trajectories. The three-dimensional electron density distribution, calculated using the mathematical model of the high-latitude ionosphere previously developed at the Polar Geophysical Institute (PGI), is used to model radio propagation. The numerical calculations make it possible mainly to explain the specific features of the experimental data on the oblique-incidence sounding of the ionosphere.     

Substorm correlated absorption on a 3200 km trans-auroral HF propagation path

A high-frequency transmitter located at Clyde River, NWT, Canada, and a receiver located near Boston, USA, provide a 3200 km trans-auroral, near-meridional propagation path over which the propagation characteristics have been measured. Out of the fourteen frequencies in the HF band sampled every hour for the duration of the experimental campaign (16 January-8 February 1989), the signal level measurements of 6.800 MHz transmissions were selected in order to determine the extent and occurrence of auroral absorption. The median level of auroral absorption along the path is found to increase with geomagnetic activity, quantified by the index K_p, with the increase being greater in the post-midnight sector than in the pre-midnight sector. This asymmetric behaviour is attributed to the precipitation of high energy electrons into the midnight and morning sector auroral D region. The measured diurnal variation in the median level of absorption is consistent with previous models describing the extent and magnitude of auroral absorption and electron precipitation. Individual substorms, identified from geosynchronous satellite data, are found to cause short-lived absorption events in the HF signal level of \sim30 dB at 6.800 MHz. The occurrence of substorm correlated auroral absorption events is confined to the midnight and morning sectors, consistent with the location of the electron precipitation. The magnitude of absorption is related to the magnetotail stress during the substorm growth phase and the magnetotail relaxation during the substorm expansion phase onset. The absorption magnitude and the occurrence of substorms during the period of the campaign increase at times of high K_p, leading to an increase in median auroral absorption during disturbed periods.     

Ionospheric disturbances in the years of solar activity minimum and their influence on HF radiowave propagation

The oblique sounding data at the Magadan-Irkutsk and Norilsk-Irkutsk paths together with the vertical sounding at stations located in northeastern Russia were used to analyze ionospheric disturbances in September 2005 and during geophysically active period in December 2006. It is found that during the main phase of magnetic storms, wave disturbances with a period of 2–4 h are registered. These disturbances cause variations in the layer maximum height up to 40–100 km and in the critical frequency up to 1.5–2 MHz. Those variations change substantially values of the maximum observed frequencies (MOF) of the ionospheric radio channel at the paths considered. Such wave disturbances can be caused by generation of AGWs in the auroral zone and their propagation to equatorial latitudes.     

The synthesis of travelling ionospheric disturbance (TID) signatures in HF radar observations using ray tracing

Characteristic signatures are often observed in HF radar range-time-intensity plots when travelling ionospheric disturbances (TIDs) are present. These signatures, in particular the variation of the F-region skip distance, have been synthesised using a ray tracing model. The magnitude of the skip variation is found to be a function of the peak electron density perturbation associated with the TID and radar frequency. Examination of experimental observations leads to an estimate of the peak electron density perturbation amplitude of around 25% for those TIDs observed by the CUTLASS radar system. The advantage of using the skip variation over the radar return amplitude as an indicator of density perturbation is also discussed. An example of a dual radar frequency experiment has been given. The investigation of the effect of radar frequency on the observations will aid the optimisation of future experiments.     

多孔岩石波传播的热弛豫模型修正

经研究发现热弛豫模型的衰减比BISQ模型大得较多,与地球介质相比衰减量也过大;反演与实验结果相比在虚模量的低频(或低温)端和高频(或高温)端相差较大,仅在峰值附近符合较好.针对上述不足,将Arrhenius关系直接引进Biot模型,替换原模型引进的峰值点的频率对数和温度关系,并重新调整了模型参数.这样既改善了原模型衰减量过大,又克服了模型反演中虚模量峰值曲线两侧差异较大的缺点.进行了P波和S波的波传播分析,仍然在频率谱和温度谱上获得热弛豫峰和Biot峰.分析显示热弛豫峰导致波速随频率升高而上升的普遍规律,Biot峰导致波速随温度升高而上升的异常现象.在相同条件下对Biot模型,BISQ模型和热弛豫模型的P波波速和衰减进行了对比.热弛豫模型得到的速度频散更强,频散范围更宽,所得的衰减峰值频率比BISQ模型要低,衰减幅度比BISQ模型稍大.这些结果与实验结果相近,更符合实际.     

Effect of magnetic storms (substorms) on HF propagation: A review

The manifestations of the so-called main ionospheric effect during geomagnetic storms (substorms) in the character of decameter-wave propagation are analyzed. On HF radio paths, the main effect is observed as variations in the signal amplitude and the MOF-LOF working frequency band similarly to the critical frequency of the ionospheric F2 layer. Specifically, these parameters increase before the disturbance active phase, decrease during the active phase, and increase again after this phase. The propagation outside the great circle arc, the change in the propagation processes, and the HF radio noise behavior were also considered on these paths during storms (substorms). It is assumed that the storm (substorm) development onset can be predicted.     

The effect of model assumptions on computations of cosmic ray induced ionization in the atmosphere

The longitudinal profile of atmospheric cascades is sensitive to the energy, mass of the primary particle and to atmospheric state. In this work are compared ionization yield functions Y for winter, summer and US standard profiles of Earth's atmosphere. The various profiles are obtained on the basis of CORSIKA 6.52 code simulations using FLUKA 2006 and QGSJET II hadronic interaction subroutines. The energy deposit of proton induced cascade processes in the atmosphere is calculated for different types of atmospheres. The ion pair production in the atmosphere and the contribution of the different shower components, precisely the electromagnetic, muon and hadronic is estimated according applied atmospheric types. In addition simulations with different hadronic interaction models GHEISHA 2002, FLUKA 2006 and QGSJET II are carried out. The ion pair production in the atmosphere and the contribution of different shower components is estimated according the assumed hadronic interaction models. The yield function Y for total ionization, respectively, for the different components is compared. The observed differences are widely discussed. General conclusion concerning the application of various atmospheric profiles and hadron interaction models is carried out.     

The effect of the electron sound speed on wave propagation in the ionospheric plasma

In this study, the effect of the electron sound speed on the extraordinary wave propagation is calculated without an approximation for either collisional or collisionless cases in the ionospheric plasma by using the real geometry of the Earth’s magnetic field for the Northern Hemisphere. It is observed that there is no remarkable effect on the propagation of the extraordinary wave, especially at reflection altitudes. But it is also observed that the magnitudes of k ² (the square of the wave number) have changed every season, and the phase velocity of wave in warm ionospheric plasma has increased.     

高频频率预测方法中国区域的精细化研究

提出了一种适用于中国及邻近区域高频天波传播的精细化频率预测方法:该方法基于ITU-R频率预测方法体系,在应用中国参考电离层模型的基础上,利用1976—2006年10个电离层观测站近三个太阳活动周期电离层特征数据的统计分析结果,充分考虑预测参量随空间位置、昼夜以及太阳活动的变化特性,重建了E层、F1层和F2层OWF-MUF和HPF-MUF转化因子的时空映射.利用中国境内2008年1月6条链路和2012年3月9条链路的观测结果,对本文所述方法和ITU-R建议方法进行对比分析,对比结果显示本文所述方法较ITU-R建议方法在预测精度上有了明显的改善:MUF、OWF、HPF预测的均方误差分别降低了0.28、0.16、0.45 MHz,最大误差降低量为0.90、0.55、1.31 MHz,均方相对误差平均降低了4.79%、2.97%和4.91%,最大误差降低量分别为10.14%、8.63%和11.75%.     

The effect of heating on the propagation speed of tropospheric equatorial waves

Summary An earlier investigation concerning the effect of vertical wind shear in the basic current on the propagation speed and divergence of tropospheric equatorial waves is extended to include the effect of parameterized heating. The combined effct of shear and heating is to decrease the propagation speed, particularly at wavelengths greater than 2000 km. Further, the effect of the heating is to increase the divergence to the correct order of magnitude. As in the no-heating case, the divergence decreases with increasing wavelength.     

人工神经网络在潜在地震危险区估计中的应用

利用环境剪应力较高的地区较容易发生中强地震这一原理,提出了将人工神经网络应用于估计潜在地震危险区的方法。由于该方法是通过人工神经网络技术提前1~2年预测某一地区未来环境应力值的变化来估计潜在地震危险区,因而可大大提高估计的准确性。该方法今后在多震地区的预报工作中值得一试。     

Peculiarities of artificial ionospheric radiation under the action of high-power HF radiowaves, emitted by the SPEAR facility, on the sporadic E layer of the polar ionosphere

The results of the experimental studies of the ionospheric effects originating under the action of high-power HF radiowaves, emitted by the SPEAR heating facility into the sporadic E _s layer of the polar ionosphere, are presented. The experiment was performed on March 2, 2007, simultaneously at two spaced points: Barentsburg (Spitsbergen, a distance of about 40 km from the SPEAR facility) and Gor’kovskaya observatory near St. Petersburg, located at a distance of about 2000 km from SPEAR. The distributions of the heating signal intensity in the 100 kHz frequency band were measured in Barentsburg. Bistatic backscatter of diagnostic HF signals by small-scale artificial ionospheric irregularities was observed at Gor’kovskaya observatory. Based on an analysis of the experimental data obtained in Barentsburg, it has been found out that a broadband noise-like component originated and additional maximums appeared in the heating signal spectrum. The broadband emission intensity was a factor of 1.5–3 as high as the noise level. The additional maximums were formed in the regions of the positive and negative frequency shift relative to the heating signal frequency and were observed when the heating frequency was lower than the critical frequency of the E _s layer; e.g., a high-power HF radiowave reflected from E _s . The expression for determining the frequency shift of the additional maximum in the heating signal spectrum at altitudes of the ionospheric E region, taking into account the ion-electron collision frequency, has been obtained. The heating signal spectrum registration was compared with the observations of small-scale artificial ionospheric irregularities and the trajectory modeling of signals scattered by the considered irregularities. The observation results have been analyzed and interpreted taking into account the magnetic and ionospheric data characterizing the background geophysical conditions.     

Influence of the ionosphere, modified by powerful oblique radiowaves, on HF radio wave propagation

Variations of HF probe radio wave parameters caused by the influence on the ionosphere of oblique powerful HF radiowaves are analysed. The analysis is made on the data obtained from the original experiments carried out on single-hop paths in the middle and subauroral latitudes. Powerful and probe waves with some difference in frequency were chosen near MUF and were transmitted in the same direction. The polar diagrams of both transmitting systems overlapped in both the horizontal and vertical planes. The results obtained indicate that the ionospheric plasma parameters can be varied by powerful oblique HF radiowaves under certain geophysical conditions.     

The effect of underlying geological structures on the propagation of seismic waves

Viewing from the energy angle and taking the Beijing depression as an example, this paper studies the effects of underlying geological structures, mainly bedrock topography and bedrock faults, on the propagation of seismic waves and discusses the effects of the overlying soil layer on seismic waves. From the study, some conclusions are drawn as follows:

1. Underlying bedrock faults affect the duration, frequency spectra and characteristics of energy distribution of seismic waves.
2. Underlying bedrock topography changes the field of ground motion not only because the bedrock at different places receives different amounts of energy from the same source but also because its asperities diverge or converge seismic waves.
3. Overlying soil layer is able both to absorb and to amplify seismic waves.

In the paper, the idea of expressing the intensity of seismic waves in terms of energy is put forward. Comparison between the expressions of the seismic wave intensity in terms of energy and the maximum amplitude shows that the former is better than the latter in reflecting the effects of underlying geological structures on seismic wave propagation.     

Measuring wave propagation characteristics in artificial sand-clay mixtures

Ultrasonic compressional (V _p ) and shear (V _s ) velocities have been measured on artificial sand-clay mixtures. The measurements were carried out in a drained triaxial load cell using a pulse transition method. The measuring device was equiped with a waveform storage facility. The investigated mixtures consisted mainly of kaolinite and quartz sand. Some mixtures also contained Na-montmorillonite, illites or quartz-flour. The acoustic behaviour was observed during a pressure increase up to 72 MPa vertical and 36 MPa horizontal pressure. At a given pressure,V _p andV _s in pure sand turned out to be similar to those in pure kaolinite. As predicted by the sand-clay model of Marion (1990), a velocity maximum corresponds to a minimum in total porosity. This porosity minimum marks the transition from a clayey sand to a sandy clay. It is not only reflected in bothV _p andV _s , but also in the quality of the received pulse. The effective tension of the received signal during 20µs after the first arrival, was used as an indication for P-wave pulse attenuation. This apparent attenuation decreases with increasing clay content and increases with increasing porosity. It is shown that clay mineralogy does not measurably affect wave velocities in clayey sands.