唐山地震发震构造的浅层地震探测

利用浅层地震探测方法,研究了唐山地震区１年前出现在卫星图像上的异常现象与发震构造的关系,探讨地震中长期预测的途径。结果表明：唐山地震断层是一条倾向ＮＷ的右旋走滑第四纪同生断裂,它错断了全新统,晚更新统,中更新统,和早更新统地层。     

福州盆地活动断裂的探槽研究

在前人对福州盆地及其周缘活动断裂 1/ 1万填图研究的基础上 ,通过室内航卫片判读、野外详细调查等方法 ,经过详细论证 ,在福州盆地及周缘 6条活动断裂上选择了 11个认为可能是断层通过的位置 ,进行了探槽开挖。大部分探槽只揭露到了基岩中的断层 ,有些探槽在开挖深度内既没有揭露到基岩 ,在第四系中也没有揭露到断层。对于没有揭露到断层的探槽 ,认为断层没有错断开挖深度内的第四纪地层 ,以探槽最底部的地层年代作为断层最新活动时代的上限。有些探槽揭露到了基岩中的断层 ,这些断层向上没有错断第四系 ,就以上覆第四系底部的时代作为断层最新活动时代的上限。只有在沿桐口 -洪山桥断裂开挖的探槽中 ,揭露出 2条断层 ,它们向上都错断了相同层位的第四纪地层 ,并被更新的第四系所覆盖。根据测年结果 ,这些断裂不是全新世活动断裂 ,其中 ,闽侯 -南屿断裂可能为晚更新世活动断裂 ,其它断裂晚更新世以来都已不活动     

The AGNS and their host galaxies as seen in the mid-infrared

We present a new diagnostic diagram based on ISOCAMspectra (5-16 m) to distinguish the emission inducedby the active galactic nucleus (AGN) from that associated with thestar formation activity. This diagnostic based on the mid-IRcontinuum and the Unidentified Infrared Band (UIB) intensity allowsus to estimate the relative importance of the three components (HIIregions, diffuse/photo-dissociation regions (PDRs), and AGN) contained ingalaxy mid-infrared emission. In AGN spectra, we confirm the absenceof UIBs presumably photodissociated by the X-UV radiation field. Inaddition, a non-negligible continuum below 9 m commonlyassociated with emission from hot dust is present in AGNs. Adiagnostic diagram derived from these two results can be used fordetecting obscured AGNs embedded in a large concentration of dust.     

Identification of newly discovered radio-emitting X-ray sources: results from spectroscopy

We present optical identifications for a sample of 20 previously unknown X-ray/radio sources that are present both in the source catalogue of ROSAT PSPC pointed observations ( ROSAT SRC) and in the NRAO VLA Sky Survey (NVSS). The optical spectroscopy was carried out with the 2.1-m telescope at San Pedro Martir (Mexico) during 1995 April and September. We have identified 15 active galactic nuclei [including 12 broad-emission-line (FWHM >1000 km s⁻¹) objects, one bona fide BL Lac, one BL Lac candidate and one narrow-line (FWHM < 1000 km s⁻¹) radio galaxy] and five radio galaxies. We derive the X-ray fluxes and luminosities by analysing the PSPC exposures, and show the radio morphology from the NVSS maps.  We find that the correlation between the monochromatic X-ray luminosity at 2 keV and the core radio luminosity at 5 GHz for the radio galaxies in our sample follows that found for the 3CR radio galaxies, suggesting a possible nuclear origin for the X-ray emission in these sources. This correlation is weaker in the case of broad-line objects, indicating the presence of another (unbeamed) mechanism for the X-ray emission only weakly related to the radio emission.     

高密度电阻率法在城市活断层调查中的应用

目的 在城市活断层调查中应用高密度电阻率层析成像测量方法。资料和方法 利用电阻率层析成像测量方法，在北京某地的活断层、郑州老鸦陈断层、安阳南断裂等处理进行了地震活断层调查，采用正、反演处理软件进行资料处理和解释。结果 取得了较理想的勘探效果。结论 在城市活断层调查中，电阻率层析成像测量方法是一种十分有效的勘探方法。     

Expulsion of geopressured hydrothermal system along active faults and its relation to the occurrence of earthquakes in the Shinanogawa seismic belt,Japan

The 1995 Northern Niigata Earthquake (M 6.0) occurred at a shallow depth in the Niigata seismic gap. The anomaly areas in temperature, electrical conductivity and Cl- concentration of groundwater trend northeast as linear distribution in the epicentral area and are approximately coincident with the area of the seismic intensity 6 (JMA scale). The distributions of seismic intensity 6 and groundwater anomalies convincingly imaged the presence of a buried active fault beneath the epicentral area. The occurrence of this earthquake and the anomalies of groundwater were related to the expulsion of geopressured hydrothermal system (GHS). All epicenters of the destructive earthquakes along the Shinanogawa seismic belt are actually located in the buried active fault zones characterized by the areas of temperature and geochemical anomalies of groundwater. These earthquakes might have been triggered by the activity of GHS. The expulsion of GHS along an active fault in combination with the thermal softening of fault     

张家口-宣化盆地断裂特征与活动性研究

运用地质地貌调查、地球物理勘探和年代测定等方法,对张家口—宣化盆地的四条主要断裂(张家口断裂、万全断裂、洗马林—水泉断裂和洋河断裂)的空间展布特征和活动性进行分析和研究,获得其活动时代、活动速率等参数。研究表明:上述断裂第四纪期间持续活动,以脆性变形为特征;总体上NW向断裂以高角度的正(或逆)倾滑断层为主,NE或NEE向的断裂以高角度的正断层为主;盆地内活动断裂总体来说活动强烈,多处可见断裂正断运动及左旋走滑运动的地质剖面,早更新世以来单条断层的平均垂直活动速率大于0.07~0.30mm/a,总垂直活动速率可能达到1.33mm/a。     

沙质河床冲刷过程中床沙级配的模拟

研究了沙质河床冲刷过程中床沙级配的模拟方法。在该方法中采用了新的描述床沙级配变化的动力学方程和床沙级配在交换层内垂向变化与水流强度、河床冲刷强度的关系,反映了冲刷过程中交换层内向床面补充的物理过程。通过室内实验率定了相关参数,建立了床沙级配变化动力学方程的数值求解方法,模拟了床沙冲刷粗化。计算结果与室内实验结果符合较好,表明所建议的方法反映了河床冲刷中床沙级配变化的物理事实,可用于沙质河床冲刷粗化模拟。     

The anticorrelation between the hard X-ray photon index and the Eddington ratio in low-luminosity active galactic nuclei

We find a significant anticorrelation between the hard X-ray photon index Γ and the Eddington ratio   L _bol/ L _Edd  for a sample of low-ionization nuclear emission-line regions and local Seyfert galaxies, compiled from literature with Chandra or XMM–Newton observations. This result is in contrast with the positive correlation found in luminous active galactic nuclei (AGN), while it is similar to that of X-ray binaries (XRBs) in the low/hard state. Our result is qualitatively consistent with the spectra produced from advection-dominated accretion flows (ADAFs). It implies that the X-ray emission of low-luminosity active galactic nuclei (LLAGN) may originate from the Comptonization process in ADAF, and the accretion process in LLAGN may be similar to that of XRBs in the low/hard state, which is different from that in luminous AGN.