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1.
江苏地区地电场变化特征与差异性分析   总被引:1,自引:0,他引:1  
处理、分析了江苏省4个台的地电场日变化资料,结合地磁场水平分量H、线应变理论固体潮,研究了地电场日变化特征和差异,得到:(1)4个台地电场日变化明显,主要以12小时的半日波成分最强,8小时周期和全日波成分次之;(2)地电场日变化存在地磁场和固体潮影响。靠近海边及湖泊的台站,受固体潮的影响较为明显,各方向还具有明显的固体潮半月波,但没有像固体潮一样大小的波;而远离江、海、湖的一些台站观测到的地电场日变与地磁水平分量比较相关,其差异性与台站的位置、电性结构有关系。  相似文献   

2.
选择黑龙江省延寿地震台CZB-1型竖直摆倾斜仪2005年的固体潮观测资料,提取了2005年7月25日黑龙江省林甸M5.1和9月19日内蒙古牙克石M4.7地震前,倾斜固体潮半日波(M2)的潮汐因子γ及相位滞后因子Δφ等参量,综合分析了中强地震前区域倾斜形变潮汐的短临变化特征。认为:1)对潮汐频段参数潮汐因子、相位滞后因子异常信息进行提取,有利于捕捉地震前兆异常。2)潮汐因子的变化特征从时间上给出了震源的短临前兆信息。从图形变化看,这种变化过程可归纳为趋势性背景变化→增大(或减小)→极值→恢复→等待→发震。3)固体潮调和分析方法具有较强的抗干扰能力,图形变化稳定、异常突出明显  相似文献   

3.
根据月球与太阳相对于地球位置的关系,建立一个三维正交分解模型来揭示重力固体潮中包含的谐波成分。在此基础上,提出一种基于单形邻域与多角色进化策略智能优化算法的独立分量分析方法,用以提高算法效率和全局寻优能力;并结合谱相关方法,对重力固体潮观测数据进行处理和分析,观察其频域和时域的变化。最后引入理论信号和理论计算值作为参考背景,以凸显其异常变化特征。研究表明,利用该方法可以有效地反映出重力固体潮潮汐的日波、半日波、长周期波等特征。同时,发现重力固体潮潮汐的异常变化中隐含有地震前兆信息,通过对云南地区观测数据的分析,在排除测量误差和环境影响外,发现在地震前2~5个月内,重力固体潮的长周期波均呈现出规律性的异常变化。这反映出地震的前兆异常信息,可能对地震时间和地点的预测提供依据。  相似文献   

4.
利用别尔采夫滤波、一般多项式拟合等方法将库尔勒地震台地倾斜、气温、气压观测数据分解为日波、半日波、1~2月周期的月波和年周期变化的年波,然后再利用相关性分析研究库尔勒地倾斜不同频段的观测数据一致性及与气象干扰因素的关系。结果表明:(1)库尔勒地倾斜在日波、半日波频段一致性较好,均能较好地反映出固体潮的变化;(2)库尔勒地倾斜在月波频段的一致性较差,仅垂直摆EW分量与气压月波具有一定的相关性;(3)库尔勒地倾斜年波经相位平移之后,均与气温具有较高的线性相关性,结合物理机理分析库尔勒地倾斜年周期变化受温度影响的原因。  相似文献   

5.
正地震预测是世界难题,目前还没有哪个科学家能准确的预测未来地震发生的情况,主要原因有3点:(1)目前我们还只能在地球表面开展地震观测(地球的不可入性);(2)破坏性地震的发生相对于天气预测来讲还是极小的概率事件,特别是7级以上的大地震,其孕育周期可能超过人的寿命。因此,一个科学家研究某一地区的地震活动规律时,可能毕生都难以经历一个活动周期。因此实验数据样本极少;(3)各地的地震分别具有不同的活动特点,无法借  相似文献   

6.
地震的发生与固体潮   总被引:1,自引:0,他引:1  
固体潮是指由月亮和太阳的引力而引起的地球弹性变形现象。通过对全球地震资料的分析,已明确了固体潮对地震的发生有着不可忽视的影响(Tsuruoka,et al,1995;鶴岡 弘,1995)。不过,由固体潮引起的地球内部的应力变化,充其量为10~3 Pa的  相似文献   

7.
以固体潮极值时刻与地震发震时刻的时间差为参数,统计了唐山老震区M_L≥2.0地震的时差在月、半月、日、半日尺度下的各时间分段内的频度分布。结果显示唐山地区的地震活动高频度时段与固体潮极值时刻有对应性,表明其在一定程度上受到了固体潮作用的影响。其中唐山断裂中东段的地震落入触发时段内的几率更大,似乎意味着唐山地区的应力集中区主要还是集中在唐山断裂中东段。另外,强震之后1~3周余震受固体潮极值的影响显著,所以此时间内应更加注意在固体潮接近极值时发生强余震的可能性。  相似文献   

8.
本文以巴彦岱1号井静水位为研究对象,分别应用别尔采夫滤波、小波分析与相关分析等方法,研究巴彦岱1号井静水位周期变化主要影响因素。分析结果表明,巴彦岱1号井静水位在日波、半日波频段主要受固体潮的影响;气压影响频段可能为64—256min、32—2048h(1—2个月周期的月波)2个频段,年周期变化与气温变化具有较强的线性相关性。  相似文献   

9.
固体潮观测中的震颤异常波   总被引:8,自引:1,他引:7       下载免费PDF全文
在地震与固体潮台站的日常监测中,常发现有一些异常"脉动"信号叠加在固体潮曲线上.这些异常"脉动"与宽频带数字地震计的观测在时间上同步、一致,其中的一部分由发生在西太平洋上的热带气旋引起,而其他的则大多与强地震相伴随,统称为震颤异常波.本文介绍了华中科技大学的地震与固体潮观测台站(HUST)的概况,报道了该台应用 DZW重力仪和VS-1倾斜仪观测记录到的大量震颤异常波事例.大量观测事实表明:中国固体潮台站记录的震颤异常波,绝大多数只在DZW重力仪和VS-1倾斜仪的低通滤波1 通道(LP1)出现,而在其低通滤波2通道(LP2)和其他固体潮仪器中则罕有发现;震颤异常波的包络线大多呈"纺锤状"或"尾巴状",持续时间多为1~3天. 通过对震颤异常波和固体潮观测仪器的分析研究,得到以下结论:震颤异常波实际上就是一种来源复杂的地球脉动信号,响应范围广泛,可被宽频带数字地震计和固体潮仪器记录.由西太平洋上的热带气旋引起的震颤异常波的主要周期在3~7 s范围,而强震前的震颤异常波则除此外,还包含10~60 s及更长周期的信号.固体潮仪器对震颤异常波响应的差异是因为仪器的传递函数不同和特性所致. DZW重力仪和VS-1倾斜仪分钟值采样数据中的震颤异常波,只是真实信号的一种"混叠"或映射.强震前的震颤异常波是否与地震有关?是否是震兆?尚需做更深入细致的分析和研究.  相似文献   

10.
研究地震发震时的地方平太阴时τ和地震断层走向两者之间的关系.共计算了24组53个地震的地方平太阴时τ.根据月亮在地球内任一点形成的起潮力是一个主要周期大约为12小时25分钟左右的周期性函数、月亮在地方平太阴时相隔180°的两个位置上,对地球内任一点的起潮力基本上相同这一现象,计算了原地重复发生的两个地震τ1-τ2或τ1-τ2±180°的值ΔΤ.计算结果表明:①如果同一地点的前后地震断层走向一致.则Δτ一般较小;如果断层走向不一致,则Δτ一般较大;②不同地区的地震,即使断层走向相近,其地方平太阴时τ的分布也较分散,且不表现出有在月亮的上、下中天附近集中的倾向.这些结果说明:月亮固体潮对地震的触发作用和地震断层走向有关;在研究月亮固体潮与地震的关系时,不宜把不同地区的地震放在一起进行统计,必须考虑不同震源区孕震环境的差异.  相似文献   

11.
The last of a cycle of three papers aimed at searching for the influence of the gravitational tide on regional Greece seismicity using different techniques is presented. Twenty-five nonintersecting samplings of earthquakes in Greece compiled from events with different energy and time intervals were studied in the two previous papers (Desherevskii and Sidorin, 2012d, 2014). Stable diurnal and semidiurnal periodicities (24:00 and 12:00 h) were revealed in the seismicity spectra. Periodicities with a small amplitude with periods close to M2 and O1 tidal waves were also found in some samples. The correlation coefficients of all time series of earthquakes were calculated with the following theoretical tide parameters: volume deformation, strain rate, of strain rate modulus, and smoothed diurnal tidal amplitude. As the main result, stable significant correlation of seismicity was revealed with some tidal parameters. However, this could be the result of coincidence in periods of sub-harmonics of the diurnal seismicity rhythm with solar tidal waves. This means that the discovered correlation could simply be caused by the coincidence of two regular components in variations of the compared processes, but not with the gravitational tide. Correlations of seismic activity with solar and lunar tides are studied separately in this paper. This makes possible to separate the influence of gravitational and nongravitational factors. Strong correlation of seismicity was observed only with the solar tide. No stable correlation of seismicity with the lunar tide was revealed. The results can be considered evidence for the nongravitational origin of seismic activity variations that correlate with the tidal parameters. This means that tidal seismicity variations, if they are real, should have a much smaller amplitude in comparison with diurnal solar variations of nongravitational origin. Similar effects could cause wrong conclusions on the tidal influence on seismicity in some studies.  相似文献   

12.
Summary Results of sunspot cycle influence on solar and lunar ranges at a low latitude station, Alibag, outside the equatorial electrojet belt, show that the sunspot cycle association in solar ranges is three times that of the lunar ranges in thed- andj-seasons. This is in general agreement with the earlier results for non-polar latitude stations. The association with sunspot number of individual lunar amplitudes is greatest for lunar semidiurnal harmonic in thej-season. During this season, the sunspot cycle influence on lunar variations is more than that on solar variations, thereby indicating that the lunar current is situated at a level more favourable for sunspot cycle influence than the level of the current associated with solar variations. With the increase in solar activity a shift appears in the times of maxima of semidiurnal lunar variation towards a later lunar hour ine- andj-seasons and in the year.  相似文献   

13.
Based on the horizontal winds measured using SKiYMET meteor wind radar during the period of June 2004–May 2007, the seasonal and interannual variability of the diurnal and semidiurnal amplitudes and phases in the mesospheric and lower thermospheric (MLT) region over a low-latitude station Trivandrum (8.5°N) are investigated. The monthly values of amplitudes and phases are calculated using a composite day analysis. The zonal and meridional diurnal tidal amplitudes exhibit both annual and semiannual oscillations. The zonal and meridional components of semidiurnal tide show a significant annual oscillation. The phase values of both diurnal and semidiurnal tides exhibit annual oscillation above 90 km. The effect of background wind in the lower atmosphere on the strength of diurnal tidal amplitudes in the MLT region is studied. The effect of diurnal tides on the background wind in the lower thermosphere is also discussed.  相似文献   

14.
In this paper we investigate the tidal triggering evidence on the earthquakes of the seismic area of the Hellenic Arc using the Hist(ogram)Cum(mulation) method. We analyze the series of the earthquakes occurred in the area which is confined by the longitudes 22° and 28°E and latitudes 34° and 36°N in the time period from 1964 to 2012. In this time period 16,137 shallow and of intermediate depth earthquakes with ML up to 6.0 and 1,482 deep earthquakes with ML up to 6.2 occurred. The result of the this analysis indicate that the monthly variation of the frequencies of earthquake occurrence is in accordance with the period of the tidal lunar monthly variations, and the same happens with the corresponding daily variations of the frequencies of earthquake occurrence with the diurnal luni-solar (K1) and semidiurnal solar (S2) tidal variations. These results are in favor of a tidal triggering process on earthquakes when the stress in the focal area is near the critical level.  相似文献   

15.
Lunar seismicity and tectonics   总被引:1,自引:0,他引:1  
Seismic signals from 300–700 deep moonquakes and about four shallow moonquakes are detected by the long-period seismometers of two or more of the Apollo seismic stations annually. Deep-moonquake activity detected by the Apollo seismic network displays tidal periodicities of 0.5 and 1 month, 206 d and 6 a. Repetitive moonquakes from 60 hypocenters produce seismograms characteristic of each. At each hypocenter, moonquakes occur only within an active period of a few days during a characteristic phase of the monthly lunar tidal cycle. An episode of activity may contain up to four quakes from one hypocenter. Nearly equal numbers of hypocenters are active at opposite phases of the monthly cycle, accounting for the 0.5-month periodicity. The 0.5- and 1-month activity peaks occur near times of extreme latitudinal and longitudinal librations and earth-moon separation (EMS). The 206-d and 6-a periodicities in moonquake occurrence and energy release characteristics are associated with the phase variations between the librations and EMS. Because of the exact relationship between tidal phases and the occurrence of deep moonquakes from a particular hypocenter, it is possible to predict not only the occurrence times from month to month, often to within several hours, but also the magnitudes of the moonquakes from that hypocenter. The predicted occurrence of large A1 moonquakes in 1975, following a 3-a hiatus, confirms the correlation between A1-moonquake activity and the 6-a lunar tidal cycle and implies a similar resurgence for all of the deep moonquakes. Because no matching shallow moonquake signals have been identified to date, tidal periodicities cannot be identified for the individual sources. However, shallow moonquakes generally occur near the times of extreme librations and EMS and often near the same tidal phase as the closest deep moonquake epicenters. With several possible exceptations, the deep-moonquake foci located to date occur in three narrow belts on the nearside of the moon. The belts are 100–300 km wide, 1,000–2,500 km long and 800–1,000 km deep and define a global fracture system that intersects in central Oceanus Procellarum. A fourth active, although poorly defined, zone is indicated. The locations of 17 shallow-moonquake foci, although not as accurate as the deep foci, show fair agreement with the deep-moonquake belts. Focal depths calculated for the shallow moonquakes range from 0–200 km. Deep-moonquake magnitudes range from 0.5 to 1.3 on the Richter scale with a total energy release estimated to be about 1011 erg annually. The largest shallow moonquakes have magnitudes of 4–5 and release about 1015–1018 erg each. Tidal deformation of a rigid lunar lithosphere overlying a reduced-rigidity asthenosphere leads to stress and strain concentrations near the base of the lithosphere at the level of the deep moonquakes. Although tidal strain energy can account for the deep moonquakes in this model, it cannot account for the shallow moonquakes. The tidal stresses within the lunar lithosphere range from about 0.1 to 1 bar and are insufficient to generate moonquakes in unfractured rock, suggesting that lunar tides act as a triggering mechanism. The largest deep moonquakes of each belt usually occur near the same characteristic tidal phases corresponding to near minimum or maximum tidal stress, increasing tidal stress, and alignments of tidal shear stresses that correspond to thrust faulting along planes parallel to the moonquake belts and dipping 30–40°. With few exceptions, the shallow moonquakes occur at times of near minimum tidal stress conditions and increasing tidal stress that also suggest thrust faulting. The secular accumulation of strain energy required for the shallow moonquakes and implied by the uniform polarities of the deep moonquake signals probably results from weak convection. A convective mechanism would explain the close association between moonquake locations and the distribution of filled mare basins and thin lunar crust, the earth-side topographic bulge, and the ancient lunar magnetic field. The low level of lunar seismic activity and the occurrence of thrust faulting both at shallow and great depths implies that the moon is presently cooling and contracting at a slow rate.  相似文献   

16.
We report the results from a search for statistically significant (at a significance level of <0.05) periodicities that synchronize the occurrence of large shallow (h ≤ 100 km) earthquakes in the eight world regions with the highest level of seismicity. The periodicities in question include the synodic periods of planets of the solar system (Mercury, Venus, Mars, and Jupiter), as well as the precession period of the lunar orbit. In five of the eight regions we have found statistically significant results for the period T ≈ 780 days, corresponding to the synodic period of Mars. The lunar cycle and the period of Mercury were significant in two regions. These results cannot be accounted for by invoking the disturbing influence of gravitational and tidal forces due to planets other than the Earth. The significant periodicities were used to develop a forecast (for the period 2004–2009) of the most probable time intervals for the occurrence of large earthquakes in four regions: Kamchatka, the South Kurils, northeastern Japan, and the Nankai trough.  相似文献   

17.
Long-term wind measurements carried out at 6 northern midlatitude sites (Saskatoon, Sheffield, Juliusruh, Collm, Obninsk, Kazan) are investigated to establish a climatology of the semidiurnal tide in the mesopause region for the narrow latitudinal range between 52°N and 56°N. Comparison of zonal and meridional components shows that in general the horizontal components are circularly polarized. Intercomparison of amplitudes and phases generally shows good agreement between the results from the different measuring systems. The results are compared with an empirical model of the semidiurnal tide. The longitudinal variation of the semidiurnal tide is small in summer, but the tidal amplitudes in winter are larger at Saskatoon and Kazan, compared with the results from the other sites. The possible influence of wave–tidal interaction in the stratosphere on the interannual variability of this difference is discussed.  相似文献   

18.
In the first part of this paper (Deshcherevskii and Sidorin, 2012b), the spectra and periodograms of time series of earthquakes in Greece were studied for various magnitude ranges and five calendar epochs. As the main result, the stable diurnal (24-h) and semidiurnal (12-h) periodicities of earthquakes were revealed. Periodicities of small amplitude related to tidal waves M2 and O1 were also revealed in some samplings. This part of the paper deals with the problems of searching for tidal effects in seismicity with traditional techniques. An alternative approach of the task is applied. The time series of earthquakes with various magnitude and representativity (magnitude of completeness) were formed. Correlation coefficients of all the time series of earthquakes were calculated with the following theoretical tide parameters: volume deformation, strain rate, module of strain rate, and smoothed diurnal tidal amplitude. Stable significant correlation of seismicity was revealed with some tidal parameters. However, it can be a result of coincidence in periods of subharmonics of diurnal seismicity rhythm with the solar tidal waves. It means that the correlation discovered could be simply caused with coincidence of two regular components in variations of the compared processes but not with gravitational tide.  相似文献   

19.
武汉台重力潮汐长期观测结果   总被引:5,自引:1,他引:4       下载免费PDF全文
采用武汉台超导重力仪(SG C032)14年多的长期连续观测资料,研究了固体地球对二阶和三阶引潮力的响应特征,精密测定了重力潮汐参数,系统研究了最新的固体潮模型和海潮模型在中国大陆的有效性.采用最新的8个全球海潮模型计算了海潮负荷效应,从武汉台SG C032的观测中成功分离出63个2阶潮汐波群和15个3阶潮汐波群信号,3阶潮波涵盖了周日、半日和1/3日三个频段.重力潮汐观测的精度非常高,标准偏差达到1.116 nm·s-2,系统反映了非流体静力平衡、非弹性地球对2阶和3阶引潮力的响应特征.结果表明,现有的武汉国际重力潮汐基准在半日频段非常精确,但在周日频段存在比较明显的偏差,需要进一步精化.对于中国大陆的大地测量观测,固体潮可以采用Dehant等考虑地球内部介质非弹性和非流体静力平衡建立的固体潮理论模型或Xu 等基于全球SG观测建立的重力潮汐全球实验模型作为参考和改正模型,海潮负荷效应应该采用Nao99作为改正模型.  相似文献   

20.
Dilatation of aquifer and associated water level fluctuation in groundwater well is known to be driven periodically from lunar, solar, or other tidal forces. Time‐dependent variables in groundwater system, such as water level, can be converted to power spectra in the frequency domain using Fourier transform to evaluate significant fluctuation. The major innovation of this research is to develop spectral representation in frequency domain for the groundwater system that the storage in confined aquifer can be determined considering dilatation affected by Earth tides and barometric effect. In order to verify applicability of the evolved method, time series of Earth tides and barograph are collected; aquifer storage is then determined inversely by selecting significant semidiurnal and diurnal components in spectra computation. It suggests that to discover groundwater storage using groundwater level with barograph and tidal potential of Earth in frequency domain becomes accessible and feasible.  相似文献   

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