Long-term seismic noise investigations on Shikotan Island: First results

In 2003–2004, long-term seismic noise observations were launched on Shikotan Island (Lesser Kuril Range) based on the “Shikotan” dormant regional seismic station. The geological and geophysical data on the registration area are reported. Information about the equipment and its technical specifications is given. The precursors to the strongest local earthquakesthat occurred in the Shikotan Island region in January 2005–March 2007 are identified.     

土地利用对溶丘洼地土壤容重、水分和有机质空间异质性的影响——以南洞流域驻马哨洼地为例

为了探究溶丘洼地土壤空间异质性及其影响因素,本文以驻马哨溶丘洼地为研究对象,利用经典统计学和地统计学的方法,从不同土地利用、坡度、坡向、土壤深度分析土壤容重、水分及有机质的空间异质性。结果表明:（1）土壤有机质为强变异,变异系数为0.71,容重和水分变异系数分别为0.15、0.11,属中等变异,土壤容重和水分呈极显著负相关,和有机质呈显著负相关,相关系数分别为-0.609、-0.581;（2）块基比介于0.78~0.97,随机部分引起的空间变异程度较大,空间自相关较小,且模型拟合较好。（3）耕地土壤有机质、水分含量最低,容重最大,而灌木土壤反之;（4）北坡土壤容重高于南坡,变异系数小于南坡;而土壤水分、有机质低于南坡,变异系数高于南坡。从不同坡位、坡向的比较中,皆体现了土地利用对土壤空间异质性的影响。在土地利用作为主要因素的影响下,驻马哨洼地土壤水分、容重、有机质由随机部分引起的空间变异增加,空间自相关减小。      

湖北省山区与平原雷电分布及其参数特征

为进一步了解山区与平原雷电参数分布特征及其差异,为山区和平原地区雷电防护工程设计和雷击风险评估提供参考,根据湖北省ADTD地闪定位系统2006年12月至2016年12月监测的资料,采用数理统计方法,对山区和平原地区的地闪频次、极性、雷电流幅值和波头陡度等参数分布特征进行了对比研究。结果表明:①山区地闪密度略高于平原地区,平原正地闪百分比稍高于山区,近10年的正地闪百分比呈上升趋势。②正地闪平均强度山区比平原大1.16kA,负地闪平均强度山区比平原小3.67kA,平原总地闪平均强度比山区大3.46kA。③总地闪小雷电流幅值(I≤30kA)概率山区比平原大8.9%,大雷电流幅值(I100kA)概率平原比山区大0.6%。④山区正地闪平均陡度分别比负、总地闪平均陡度大2.44kA/μs和2.31kA/μs,平原正、负、总地闪平均陡度分别比山区大3.41kA/μs、5.77kA/μs和5.64kA/μs。可以得出,山区小雷电流绕击率大于平原,正地闪雷电感应的危害大于负地闪和总地闪;平原地区大雷电流反击率比山区大,雷电感应的危害大于山区。     

THE INFLUENCE OF HORIZONTALLY NON-UNIFORM HEATING UPON THE DEVELOPMENT OF STRONG CONVECTIVE MESOSCALE DISTURBANCES

It is shown by observational data and synoptic analysis that the development of strong convective echo is influenced by the horizontally non-uniform heating, such as the one caused by lake-land distribution. In this paper, a simple linear cell-convection model is established using an appropriate heating field, and the instability of heating convection is theoretically studied. It is found that the heating convection development will be unstable if the heating-caused temperature gradient dT0/dy is greater than the critical value (dT0/dy)c which is approximately 0.64℃/10 km, and that the development of convective band has a preferred width of 12.5 km. It will take 25 min for the initial disturbance to increase intensity by 10 times. All these results are in rather good agreement with the squall line process in the lake-land region of Jiangsu Province on June 8, 1979.     

Incoherent radiation from relativistic electrons with power energetic spectrum

It is shown that an incoherent high-frequency radiation from an ensemble of relativistic particles with the power energy distribution is described by a certain general expression which covers practically all the cases of particle radiation in random electromagnetic fields of cosmic radiation sources.     

黄河下游及河口区超铀元素Pu的浓度测定

本文测定研究了黄河口及下游区表层沉积物中的Pu浓度。结果表明,该区表层沉积物中存在微量的Pu污染;黄河口的Pu浓度高于下游区;该区的Pu,~(137)Cs两个同位素有相似的变化规律。     

X-ray activity from different types of stars

X-ray emission is an important indicator of stellar activity. In this paper, we study stellar Xray activity using the XMM-Newton and LAMOST data for different types of stars. We provide a sample including 1259 X-ray-emitting stars, of which 1090 have accurate stellar parameter estimations. Our sample size is much larger than those used in previous works. We find a bimodal distribution of the X-ray to optical flux ratio(log(fX/fV)) for G and K stars. We interpret that this bimodality is due to two subpopulations with different coronal heating rates. Furthermore, using the full widths at half maxima calculated from Hα and Hβ lines, we show that these stars in the inactive peaks have smaller rotational velocities. This is consistent with the magnetic dynamo theory that presumes stars with low rotational velocities have low levels of stellar activity. We also examine the correlation between log(fX/fV) and luminosity of the excess emission in the Hα line, and find a tight relation between the coronal and chromospheric activity indicators.     

圆弧状沉积盆地与软土单覆盖层出平面地表运动对比

采用解析方法，通过圆弧状沉积盆地与同样参数的软土均匀单覆盖层的对比，研究沉积盆地对平面SH波二维散射效应和其出平面地表运动。数值对比结果表明：（1）波垂直入射时盆地中央地表位移幅值反应，其随频率变化形式与软土单覆盖层的地表运动有较强的对应性，且此时单覆盖层地表位移幅值为其下降；（2）盆地的二维散射效应特点显著波的汇聚作用使盆地中的地表运动显著放大，总体上较软土单覆盖层的地表位移幅值要大，其频域内的最大反应则明显大于单覆盖层情况，但最大反应在盆地表面出现的位置依赖于入射波角度、盆地深宽比和盆地的软硬程度；（3）沉积盆地中地表位移运动有强烈扭转效应，且随盆地变软和入射波频率增高而增强。     

分形理论用于洪水分期的初步探讨

用分形理论对洪峰散点序列进行了分析,发现洪峰散点序列在一定尺度范围内表现出了自相似性,初步证明洪峰散点序列是一种分形。提出了用分形理论划分洪水分期的方法,并以雅垄江小得石站洪水分期研究为例。结果显示,用分形法划分的洪水分期和传统的经验方法划分的洪水分期基本一致,但和传统方法相比,新方法的优点较为客观。