The application of microwave remote sensing technology in rock mechanics

Ｔｈｅａｐｐｌｉｃａｔｉｏｎｏｆｍｉｃｒｏｗａｖｅｒｅｍｏｔｅｓｅｎｓｉｎｇｔｅｃｈｎｏｌｏｇｙｉｎｒｏｃｋ　ｍｅｃｈａｎｉｃｓＮａｉ－ＧｕａｎｇＧＥＮＧ（耿乃光）；Ｚｈｅｎｇ－ＦａｎｇＦＡＮ（樊正芳）；Ｑｕａｎ－ＱｕａｎＪＩ（籍全权）；Ｃｈｅｎｇ－...     

Theoretical researches on three-dimensional coda wave scattering problem

Ｔｈｅｏｒｅｔｉｃａｌｒｅｓｅａｒｃｈｅｓｏｎｔｈｒｅｅ－ｄｉｍｅｎｓｉｏｎａｌｃｏｄａｗａｖｅｓｃａｔｔｅｒｉｎｇｐｒｏｂｌｅｍＹｏｎｇ－ＡｎＮＩＥ；ＪｉａｎＺＥＮＧａｎｄＤｅ－ＹｉＦＥＮＧ（聂永安，曾健，冯德益）（ＳｅｉｓｍｏｌｏｇｉｃａｌＢｕｒ...     

A case study:cross-well acoustic tomography in Fuyu oil-field

Ａｃａｓｅｓｔｕｄｙ：ｃｒｏｓｓ－ｗｅｌｌａｃｏｕｓｔｉｃｔｏｍｏｇｒａｐｈｙｉｎＦｕｙｕｏｉｌ－ｆｉｅｌｄＲｕｉ．ＦＥＮＧ；（冯锐）ＲｕｉＹＡＮ；（＠２阎锐）ＹｉＴＡＮＧ；（汤毅）Ｚｈｏｎｇ－ＹｕａｎＷＡＮＧ；（王忠元）Ｊｉａｎ－ＰｉｎｇＷＵ；（吴...     

Features of isostatic gravity anomaly and seismic activity in the Central Asian region

Ｆｅａｔｕｒｅｓｏｆｉｓｏｓｔａｔｉｃｇｒａｖｉｔｙａｎｏｍａｌｙａｎｄｓｅｉｓ┐ｍｉｃａｃｔｉｖｉｔｙｉｎｔｈｅＣｅｎｔｒａｌＡｓｉａｎｒｅｇｉｏｎＳＨＥＮＧ－ＭＩＮＧＦＡＮＧ１）（方盛明）ＲＵＩＦＥＮＧ２）（冯锐）ＣＨＡＮＧ－ＺＨＥＮＧＴＩＡＮ...     

The subterranean electric structure at the Chinese Great Wall Station on Antarctic（CGWSA）

ＴｈｅｓｕｂｔｅｒｒａｎｅａｎｅｌｅｃｔｒｉｃｓｔｒｕｃｔｕｒｅａｔｔｈｅＣｈｉｎｅｓｅＧｒｅａｔＷａｌｌＳｔａｔｉｏｎｏｎＡｎｔａｒｃｔｉｃ（ＣＧＷＳＡ）曾小萍，林云芳，赵跃辰Ｘｉａｏ－ＰｉｎｇＺＥＮＧ；Ｙｕｎ－ＦａｎｇＬＩＮａｎｄＹｕｅ－Ｃｈｅｎ...     

Observation and research on ULF and VLF seismo－electromagnetic radiation

ＯｂｓｅｒｖａｔｉｏｎａｎｄｒｅｓｅａｒｃｈｏｎＵＬＦａｎｄＶＬＦｓｅｉｓｍｏ－ｅｌｅｃｔｒｏｍａｇｎｅｔｉｃｒａｄｉａｔｉｏｎＪＩＡ－ＺＨＩＹＵＡＮ（袁家治）；ＫｏｚｏＴａｋａｈａｓｈｉ；ＳＨＵ－ＱＩＮＧＱＩＡＮ（钱书清），ＹｏｋｉｏＦｕｊｉｎａｗ...     

Maximum likelihood spectrum estimation method and its application in seismo－magnet－icrelation

Ｍａｘｉｍｕｍｌｉｋｅｌｉｈｏｏｄｓｐｅｃｔｒｕｍｅｓｔｉｍａｔｉｏｎｍｅｔｈｏｄａｎｄｉｔｓａｐｐｌｉｃａｔｉｏｎｉｎｓｅｉｓｍｏ┐ｍａｇｎｅｔ┐ｉｃｒｅｌａｔｉｏｎＸＩＡＯ－ＰＩＮＧＺＥＮＧ１）（曾小苹），ＹＵＮ－ＦＡＮＧＬＩＮ１）（林云芳），...     

The relation between the response spectrum and the phase diference spectrum

ＴｈｅｒｅｌａｔｉｏｎｂｅｔｗｅｅｎｔｈｅｒｅｓｐｏｎｓｅｓｐｅｃｔｒｕｍａｎｄｔｈｅｐｈａｓｅｄｉｆｅｒｅｎｃｅｓｐｅｃｔｒｕｍＦＥＮＧ－ＸＩＮＺＨＡＯ（赵凤新）ａｎｄＹＵ－ＸＩＡＮＨＵ（胡聿贤）ＩｎｓｔｉｔｕｔｅｏｆＧｅｏｐｈｙｓｉｃｓ，Ｓｔａ...     

The origin of the crustal conductive layer and the conductivity of supercritical brine（Ⅱ）

Ｔｈｅｏｒｉｇｉｎｏｆｔｈｅｃｒｕｓｔａｌｃｏｎｄｕｃｔｉｖｅｌａｙｅｒａｎｄｔｈｅｃｏｎｄｕｃｔｉｖｉｔｙｏｆｓｕｐｅｒｃｒｉｔｉｃａｌｂｒｉｎｅ（Ⅱ）ＣＨＡＮＧ－ＦＡＮＧＸＵ（徐常芳）ＩｎｓｔｉｔｕｔｅｏｆＧｅｏｌｏｇｙ，ＳｔａｔｅＳｅｉｓｍｏ...     

StudyofCurieisothermalsurfaceinSichuanBasinandtheseismicareaonitswesternmar┐gin

ＳｔｕｄｙｏｆＣｕｒｉｅｉｓｏｔｈｅｒｍａｌｓｕｒｆａｃｅｉｎＳｉｃｈｕａｎＢａｓｉｎａｎｄｔｈｅｓｅｉｓｍｉｃａｒｅａｏｎｉｔｓｗｅｓｔｅｒｎｍａｒ┐ｇｉｎＸＩＡＮＺＨＡＮＧ（张先），ＸＩ－ＦＥＮＧＨＵ（虎喜凤），ＪＩＮＧ－ＸＩＵＳＨＥＮ（沈京秀...     

Geomagnetic solar flare effect on February 4 and 6, 1986 at the China Antarctic Great Wall Station

Taking the sampled every minute values of the horizontal, declination and vertical componentsH, D, Z and the intensity of total field F calculated fromH andZ on the magnetograms at ten geomagnetic observatories in China in the same periods, and at the China Antarctic Great Wall Station (CAGWS), the authors conducted the maximum entropy analysis and band-pass filtration of these data and obtained the following results: (1) At the periodT=10 ? 90 min geomagnetic solar flare effect (sfe) is evident on the sunlit hemisphere. It is more pronounced at periods 15, 20, 25 and 30 min, and most prominent at 30 – 35 min. The solar X-ray spectra at the same time showed their peaks at 10 and 15 min; (2) The periodT=10 ? 70 min of sfe at the CAGWS in the western Hemisphere was also recognizable after spectral analysis and filtration, but the corresponding period of the maximum amplitude was different from that in the sunlit hemisphere. The results further proved that the geomagnetic effect of solar flares could also be observed in the dark hemisphere; (3) The subsolar points of two solar flares were found around Lanzhou, and the associated current density in the ionosphere was about 24 A/km. The transitional zone from positive to negative sfe was found around the geographic latitude?=22° ? 24°N, where the sfe inH-crochet was almost illegible.     

Observation and analysis of geomagnetic abnormity associated with the Ms=5.7 Jiujiang-Ruichang earthquake

A three-component geomagnetic survey was carried out during the period from 2002 to 2004 in China including Jiujiang-Ruichang region. Comparing the ＂2005.0 surface spline model of China geomagnetic field＂ created on the basis of the survey data with the ＂1970.0 surface spline model of China geomagnetic field＂, we can see an obvious abnormity in the geomagnetic horizontal component within a range of about 100 km around the epicenter of the Ms=5.7 Jiujiang-Ruichang earthquake occurred on November 26, 2005. After the earthquake, we carded out a repeated geomagnetic survey at 21 stations in the Jiujiang-Ruichang region and created a corresponding ＂2005.0 partially revised surface spline model of China geomagnetic field＂. By comparing the above three models, analyzing the geomagnetic horizontal component at the profile in the Jiujiang-Ruichang region and quantitatively studying the geomagnetic data of every stations around the Ms=5.7 earthquake, we have obtained the geomagnetic abnormity associated with this earthquake. Then the geomagnetic abnormity and its relation with seismic activity are discussed in this paper.     

Geoeffectiveness of XRA events associated with RSP II and/or RSP IV estimated using the artificial neural network

A forecasting scheme of geomagnetic activity is presented, based on the analysis of the geoeffectiveness of X-ray flares, accompanied by Type II and/or Type IV radio bursts (RSP) observed on the solar disc in the years 1996–2004. The neural network was used to construct this scheme enabling us to determine the probability, with which flares will be followed by a geomagnetic response of a particular intensity. The successfulness of forecasts produced after the fact depended on the flare class and on the combination of radio-burst types. In the case of RSP IV, 58% of the geomagnetic responses of X-ray flares of at least B class were successful. If only RSP II was observed, the forecast was successful only for flares of the X class (67% of successful forecasts). In the second step, a strong geomagnetic response was correctly forecast after geoeffective flares in 58% of the cases. The results are in a good agreement with recent papers based on physical modelling. fridrich@geomag.sk ph@ig.cas.cz, jboch@ig.cas.cz     

Geomagnetic diurnal-variation anomalies and their relation to strong earthquakes

The diurnal-variation anomalies of the vertical-component in geomagnetic field are mainly the changes of phase and amplitude before strong earthquakes. On the basis of data recorded by the network of geomagnetic observatories in China for many years, the anomalous features of appearance time of the minima of diurnal variations (i.e, low-point time) of the geomagnetic vertical components and the variation of their spatial distribution (i.e, phenomena of low-point displacement) have been studied before over 30 strong earthquakes with M _S≥6.6 such as Kunlunshan M _S=8.1 earthquake on November 14, 2001; Bachu-Jashi M _S=6.8 earthquake on February 24, 2003; Xiaojin M _S=6.6 earthquake on September 22, 1989, etc. There are good relations between such rare phenomena of geomagnetic anomalies and the occurrence of earthquakes. It has been found that most earthquakes occur in the vicinity of the boundary line of sudden change of the low-point displacement and generally within four days before and after the 27th or 41st day counting from the day of appearance of the anomaly. In addition, the anomalies of diurnal-variation amplitude near the epicentral area have been also studied before Kunlunshan M _S=8.1 earthquake and Bachu-Jiashi M _S=6.8 earthquake. Foundation item: National Science Technology Tackle Key Project during the Tenth Five-year Plan (2001BA601B01-05-04)     

Effects of solar and geomagnetic activities in variations of power spectra of electrical and meteorological parameters in the near-Earth atmosphere in Kamchatka during October 2003 solar events

We perform spectral analysis of records of meteorological (temperature, humidity, pressure of the atmosphere) and electrical (strength of quasi-static electric field and electric conductivity of air) parameters observed simultaneously at the Paratunka observatory during the solar events of October 21–31, 2003. Also, we use simultaneous records of X-ray fluxes of solar radiation, galactic cosmic rays, and the horizontal component of the geomagnetic field. We show that the power spectra of the meteorological parameters under fine weather conditions involve oscillations with a period of thermal tidal waves (T ～ 12 and 24 h) caused by the influx of thermal radiation of the Sun. During strong solar flares and geomagnetic storm of October 29–31 with a prevailing component of T ～ 24 h, their spectra involve an additional component of T ～ 48 h (the period of planetary-scale waves). With the development of solar and geomagnetic activities, the power spectra of atmospheric electric conductivity and electric field stress involve components of both thermal tidal and planetary-scale waves, which vary highly by intensity. In the power spectra of galactic cosmic rays accompanying the strong solar flares, components with T ～ 48 h were dominant with the appearance of additional (weaker by intensity) components with T ～ 24 h. The simultaneous amplification of components with T ～ 48 h in the power spectra of electric conductivity and electric field strength provides evidence of the fact that the lower troposphere is mainly ionized by galactic cosmic rays during strong solar flares and geomagnetic storms. The specified oscillation period with T ～ 48 h in their spectra, as well as in the spectra of X-ray radiation of the sun, is apparently caused by the dynamics of solar and geomagnetic activities with this time scale.     

地磁钩扰的全球响应特征研究与初步统计结果

地磁钩扰是太阳耀斑效应的直观表现之一,其研究有助于深入理解太阳爆发对地球空间环境的影响过程,并能为空间天气建模和预报提供科学依据.本文利用山东大学威海地磁台和Intermagnet地磁链与子午工程的地磁观测数据,联合GOES卫星及数字测高仪等的数据,研究了一个由M5.6级太阳耀斑引发的地磁钩扰事件的全球响应特征.研究发现：地磁钩扰特征呈现出南北半球与午前/午后的差异,且地磁响应相对于太阳耀斑存在约3 min的滞后现象,而夜侧无明显扰动;利用位于日侧的50余个地磁台站的数据统计分析后发现地磁钩扰幅度呈现正态分布,且在当地时正午附近达到峰值;利用地磁数据反演出钩扰发生时电离层的电流体系S_s和宁静日电流S_q,并用该电流体系解释了此事件中地磁数据的变化特征.另外,本文初步统计了1996-2015年的地磁钩扰事件数以及相关的太阳耀斑事件数,分析后发现X级耀斑引发地磁钩扰的可能性最大,达42%,由M级耀斑引发的地磁钩扰事件数最多,A、B、C级等小耀斑引发地磁钩扰的可能性很小.     

短論——太阳活动对地磁場影响的南北不对称性

苏联Р.Γ.阿芬尼娜研究急始型磁暴的十一年出現頻数分布吋,发現1944-1959这两个太阳黑子活动周期內,急始型磁暴的頻数分布曲线与太阳北半球黑子面积的十一年变化曲线相似。     

On the geomagnetic and ionospheric responses to an intense storm associated with weak IMF Bz and high solar wind dynamic pressure

A study of the geomagnetic storm of July 13–14, 1982, and its ionospheric response is presented using the low-latitude magnetic index, Dst, and interpreted using solar wind interplanetary data: proton number density, solar wind flow speed, interplanetary magnetic field southward component B _Z , and solar wind dynamic pressure. The F2 region structure response to the geomagnetic storm was studied using foF2 data obtained during the storm from a network of various ionosonde stations. Our results appear to show simultaneous abrupt depletion of foF2 that occurred at all latitudes in both the East Asian and African/European longitudinal zone during the period: 18:00–19:00 UT on July 13 and is as result of an abrupt increase in the dynamic pressure between 16:00 and 17:00 UT. The dynamic pressure increased from 3.21 to 28.07 nPa within an hour. The aforementioned abrupt depletion of foF2 simultaneously resulted in an intense negative storm with peak depletion of foF2 at about 19:00 at all the stations in the East Asian longitudinal zone. In the African/European longitudinal zone, this simultaneous abrupt depletion of foF2 resulted in intense negative storm that occurred simultaneously at the low latitude stations with peak depletion at about 20:00 UT on July 13, while the resulting negative storm at the mid latitude stations recorded peak depletion of foF2 simultaneously at about 2:00 UT on July 14. The present results indicate that most of the stations in the three longitudinal zones showed some level of simultaneity in the depletion of foF2 between 18:00 UT on July 13 and 2:00 UT on July 14. The depletion of foF2 during the main phase of the storm was especially strongly dependent on the solar wind dynamic pressure.     

Solar origin of geomagnetic storms and prediction of storms with the use of neural networks

This review deals with how the changes of the large-scale solar magnetic fields are related to the occurrence of solar phenomena, which are associated with geomagnetic storms. The review also describes how artificial neural networks have been used to forecast geomagnetic storms either from daily solar input data or from hourly solar wind data. With solar data as input predictions 1–3 days or a month in advance are possible, while using solar wind data as input predictions about an hour in advance are possible. The predictions one hour ahead of the geomagnetic storm indexD _st from only solar wind input data have reached such high accuracy, that they are of practical use in combination with real-time solar wind observations at L1. However, the predictions days and a month ahead need to be much improved in order to be of real practical use.     

高压直流输电线对甘肃地磁观测的影响分析及应对措施

随着国家电网建设规模的不断扩大,越来越多的高压直流输电工程陆续投入使用,对线路两侧的地磁观测资料造成了不可避免的影响。目前有5条高压直流输电线路对甘肃地磁台站的观测造成一定程度的干扰。通过单台及多台观测资料对比的方法,识别高压直流输电线对地磁观测资料的影响,研究干扰特征,对正确预处理观测资料有重要的意义。结果表明:①高压直流输电对地磁Z分量影响明显,D、H分量不明显;②对地磁观测影响产生的形态主要表现为方波型、缓变型、梯形型、复合型等。通过总结高压直流输电对地磁观测资料影响特征及形态,有助于正确预处理观测资料及为今后实现计算机自动化处理提供依据。