京西北地区地震重定位及构造特征

采用双差定位法对京西北地区（39.5°—41.5° N,113°—117° E）2013年1月1日至2017年12月31日6 223次有效地震进行精确定位,得到该区震源分布的精细图像和震源深度剖面图。结果显示,重新定位后地震的水平分布更集中,沿断裂带分布特征更加明显,震中在断裂带呈更明显的条带状、簇状分布,地震与线状的深浅断裂构造的关系密切;大部分地震发生在中上地壳,震源分布为典型震源密集区的空间形态,呈纵深约15 km、直径20—40 km的近圆形“厚饼状”。     

细粒含量对粗粒土冻胀特性影响的试验研究

为了得到同时满足冻胀率和击实效果的最大细粒土含量,通过葡氏击实和冻胀试验,研究了不同细粒土含量、不同干密度条件下细圆砾土填料的冻胀特性。研究结果表明,9%细粒土含量下细圆砾土试样的压实效果最好;细圆砾土试样的冻结过程可以划分为快速冻结区、过渡区、似稳定区和稳定区;细粒土含量低于10%时,细圆砾土属于弱冻胀填料;同时满足冻胀率和压实效果的最大细粒土含量为9%;细粒土含量相同时,细圆砾土试样的冻胀率随干密度的增加,先增大而后减小,即存在一个最不利干密度;冻结48 h后,细圆砾土试样冻土段的含水率均大于初始含水率,其不同位置含水率分布曲线呈S型,且随着细粒土含量的增加逐渐呈现倒三角形分布;细圆砾土试样干密度的增大有效地阻断了水分迁移路径。     

西非加蓬盆地深水盐下局部盐胶结储层精细预测技术

西非加蓬盆地是一个典型的大西洋被动大陆边缘盆地,其深水盐下为一个高风险与高潜力并存的勘探新领域。近年来,在加蓬深水区M气田的勘探中,遇到了盐胶结型储层预测的新难题。在钻井数量少、地震资料品质有限以及缺乏成熟技术体系参考的条件下,通过对盐胶结成因机制进行深入研究,结合岩石物理分析、地震属性分析、盐胶结型砂岩储层岩石物理模型以及正、反演等关键地球物理技术手段,对盐胶结储层进行精细综合预测,探索形成了“基于地质成因机制指导下的盐胶结储层精细预测技术组合”。运用该技术有效预测了M气田的有利储层分布区,指导了M气田的勘探及评价。     

气溶胶气候效应的一维模式分析

本文首先采用一线辐射对流模式，分析了乡村型、城市型气溶胶和平流层气溶胶含量增加对全球地表气温的直接影响以及硫酸盐粒子含量增加对全球地表气温的间接影响。然后利用考虑了海洋热惯性作用的ＥＢＭ／ＢＤ模式，模拟了近百年来由于大气中硫酸盐粒子含量变化、火山爆发和大气温室气体浓度增加共同引起的全球地表平均气温变化。结果表明：气溶胶的气候效应在地气系统辐射收支和全球气温变化研究中起着非常重要的作用。     

94/220 GHz星载雷达双波长比对非球形冰晶云参数敏感性分析

利用不同形状冰晶的散射特性,获得了非球形冰晶云的94/220 GHz测云雷达双波长比,探讨了非球形冰晶云的双波长比与云内微物理参数的关系,分析了衰减前后的星载雷达反射率因子及双波长比的垂直廓线。结果表明:（1）双波长比可以反映小到0.1 mm中值尺度的冰粒子,对粒子总数、谱的形状参数不敏感,对粒子大小、形状、云衰减较敏感。（2）雷达灵敏度一定时,星载雷达可测云厚与雷达波长、冰含水量（IWC）的垂直分布、云厚及衰减有关;没有进行衰减订正时,双波长比和衰减有关,冰含水量越大,波长越短,衰减越大,双波长比最大值与可探测云厚有关。两部雷达可探测冰含水量为0.001—0.1 g/m3、厚2 km的冰云;当云厚5 km、冰含水量垂直分布在0.001—0.2 g/m3时,云厚的94%基本可以被220 GHz云雷达探测到。（3）如果两部雷达气象方程中用水的介电因子,测量回波强度应进行介电因子的订正后再计算双波长比。      

Fog and rain water chemistry at Mt. Fuji: A case study during the September 2002 campaign

Measurements of fog and rain water chemistry at the summit of Mt. Fuji, the highest peak in Japan, as well as at Tarobo, the ESE slope of Mt. Fuji in September 2002. The pH of fog and rain water sampled at Mt. Fuji varied over a range of 4.0–6.8. Acidic fogs (pH < 5.0) were observed at the summit when the air mass came from the industrial regions on the Asian continent. The ratio of [SO₄²⁻]/[NO₃⁻] in the fog water was lower at Tarobo than at the summit. High concentrations of Na⁺ and Cl⁻ were determined in the rain water sampled at the summit, possibly because of the long-range transport of sea-salt particles raised by a typhoon through the middle troposphere. The vertical transport of sea-salt particles would influence the cloud microphysical properties in the middle troposphere. Significant loss of Mg²⁺ was seen in the rain water at the summit. The concentrations of peroxides in the fog and rain water were relatively large (10–105 μM). The potential capacity for SO₂ oxidation seems to be strong from summer to early autumn at Mt. Fuji. The fog water peroxide concentrations displayed diurnal variability. The peroxide concentrations in the nighttime were significantly higher than those in the daytime.     

Contribution of domain rotation to the magnetic susceptibility of spherical two-domain particles of magnetite

Summary. Starting with a simplified picture of the presumed magnetization configuration in a two-domain sphere of magnetite, the initial susceptibility due to rotation of the magnetization in the domains has been calculated. In particles between 100 and 300 nm in diameter the calculated susceptibility for randomly oriented particles drops rapidly from about 6 to a little over 3, which is the value to be expected for large multidomain particles. The results agree well with the available experimental results and imply that in magnetite particles in this size range the low field susceptibility is dominated by the domain rotation and that wall motion is effectively inhibited.     

Measuring proton energies and fluxes using EIT (SOHO) CCD areas outside the solar disk images

An indirect proton flux measuring tool based on discrimination of the energy deposited by protons in 128 × 128 pixel EIT CCD areas outside the solar disk images is presented. Single pixel intensity events are converted into proton incident energy flux using modeled energy deposition curves for angles of incidence ±60° in four EIT spatial areas with different proton stopping power. The extracted proton flux is corrected for both the loss of one‐pixel events in the range of angles of incidence as well as for the contribution to the single pixel events resulting from scattered middle‐energy protons (low‐energy or high‐energy particles are stopped by the EIT components or pass through them, accordingly). A simple geometrical approach was found and applied to correct for a non‐unique relation between the proton‐associated CCD output signal and the incident proton energy. With this geometrical approximation four unique proton incident energy ranges were determined as 45–49, 145–154, 297–335, and 390–440 MeV. The indirect proton flux measuring tool has been tested by comparing Solar Energetic Particles (SEP) flux temporal profiles extracted from the EIT CCD frames and downloaded from the GOES database for the Bastille Day (BD) of 2000 July 14 and the more recent 2005 January 20 events. The SEP flux temporal profiles and proton spectra extracted from the EIT in the relatively narrow energy ranges between 45 and 440 MeV reported here are consistent with the related GOES profiles. The four additional EIT extracted ranges provide higher energy resolution of the SEP data. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Primordial black holes

Primordial black holes (PBHs) are a profound signature of primordial cos-mological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The mechanisms of PBH formation are discussed and observational constraints on the PBH spectrum, or effects of PBH evaporation, are shown to re-strict a wide range of particle physics models, predicting an enhancement of the ul-traviolet part of the spectrum of density perturbations, early dust-like stages, first or-der phase transitions and stages of superheavy metastable particle dominance in the early Universe. The mechanism of closed wall contraction can lead, in the inflation-ary Universe, to a new approach to galaxy formation, involving primordial clouds of massive BHs created around the intermediate mass or supermassive BH and playing the role of galactic seeds.     

Potential particles: a method for modelling non-circular particles in DEM

Options for defining non-circular (or non-spherical) particles in DEM codes are briefly reviewed before introducing a new concept: potential particles. This method can be used to define convex particles with a wide variety of shapes, from almost polygonal to circular. It is readily applicable in both two and three dimensions. Although contact detection and overlap calculations are not as fast as for circular particles, they can nevertheless be made sufficiently simple and fast for implementation in DEM codes.