利用中级地震激发的自由振荡简振模研究我国大陆中部地区上地幔介质横向特性

选取2004~2015年发生在我国大陆附近的14个中级地震(6.5相似文献   

南海北部荔湾3区块天然气水合物分布特征及目标识别

针对天然气水合物钻探与取样难以解决的水合物矿体空间展布等问题,利用白云-荔湾凹陷高密度分析重新处理的三维地震资料,首先基于模糊数学的多属性融合技术对水合物分布进行刻画;再通过高分辨率速度场对浅层开展高分辨率宽频无井反演技术,提高了水合物层分辨率;最后,利用岩石物理方法及多种模型对水合物饱和度进行定量预测,实现了对5～6m厚水合物层的有效辨别,进而形成了一套适合于孔隙充填型的水合物矿藏目标识别评方法。结果表明:应用该技术可有效对荔湾3水合物富集区第四条带水合物空间刻画,揭示出该区水合物饱和度最高可超40%,同时薄层与厚层水合物具有明显互层分布特征,在水合物矿体刻画及饱和度预测基础上,进一步对该区实施了井位优选,该方法预测的水合物层与实际钻探H1和H2站位吻合较好。这些结果说明常规三维油气地震数据在经过宽频处理后可应用于高分辨率水合物勘探,节约经济成本,同时提高了常规地震在水合物勘探中精度与实用性。     

���̨��б��ϫ�α�۲�����������ӳ��Ч������

??????????????????б??1994??2008?????б????????????????????????????14?????б????????????????????????????????????5???????????????????????????е??????????????????????б?????????????????????????????3???????????????????????????????????????????????????5.7??????8.0????????????????     

JCZ-1T超宽频带地震计作为综合观测仪器的拓展应用

JCZ-1T超宽频带地震计具有全频带覆盖特性,其低频端输出延伸到固体潮汐,提出了获取稳定的低频端数据的观测条件.利用地震计LP通道连续观测数据中的垂直分向数据经过处理获得的重力资料,以及水平分向数据经过处理获得的倾斜资料做了Venedikov调和分析.对印尼8.7级大地震数据进行处理,获得地球自由振荡的功率谱密度.仪器可获取与地震事件密切相关的综合观测数据.     

宽带啁啾脉冲激光非线性传输过程中的时空微扰研究

基于非线性薛定谔方程推导出大啁啾脉冲的传输方程,利用微扰理论,分析了啁啾脉冲激光的时空不稳定性. 理论上比较清楚的阐述了宽带脉冲激光在大啁啾情况下,其时空噪声的相互影响与相互作用情况及脉冲啁啾对噪声微扰调制的影响,发现在相同γI₀(非线性系数与峰值强度乘积)的情况下脉冲啁啾对噪声调制的增长没有直接影响. 最后我们在实验上利用非线性介质对啁啾脉冲的空间小尺度自聚焦过程进行了部分验证,同时也在数值上对宽带啁啾脉冲的时间噪声调制的增长进行了模拟分析,发现实验结果和模拟分析结论     

递归型多业务宽带GEO卫星网络跨层流量控制算法研究

提出了一种递归型多业务跨层流量控制算法。该算法首先将多业务输入的流量控制问题抽象为具有输入端速率控制机制的缓冲区门限优化问题,建立多输入递归型SFM单节点模型MRSFM;确定了反映用户应用层QoS丢包和延时性能要求的系统代价函数,建立了用于跨层流量控制优化模型。在跨层优化模型的基础上,以建立的MRSFM模型为基础,运用IPA方法推导了代价函数相对于优化参数(缓冲区门限)的IPA导数,并利用SA理论进行优化。仿真实验验证了宽带GEO卫星网络跨层流量控制算法的正确性。     

宽带太阳漫射辐射法反演辐射加权平均的气溶胶一次散射反照率研究

引入了一个辐射加权平均的宽带气溶胶一次散射反照率(SSA)的定义,提出了一个从宽带的漫射信息反演该SSA的方法.数值模拟结果表明,在Junge气溶胶谱分布情形下,对气溶胶光学厚度、(A)ngstr(o)m 指数与气溶胶虚部的通常变化范围,应用该SSA所计算的2160组宽带太阳辐射反射率、漫射透过率、总透过率和吸收率的相对标准误差都在1.107%以内; 绝对标准差在0.00287以内.对非Junge的大陆性和都市工业污染气溶胶模式(由水溶性、沙尘和碳粒子组成),在72组反射率、漫射透过率、总透过率和吸收率计算中,相对标准差都在2.047%以内,绝对标准差在0.0075以内.在Junge气溶胶假设下,作者提出了一个综合应用宽带太阳直射和漫射信息同时反演气溶胶光学厚度与辐射加权平均SSA的方法,并通过模拟反演分析了SSA反演的3个主要误差因子.从反演结果可以看出:(1)如果(A)ngstr(o)m指数误差在±0.2以内,对0.55 μm气溶胶光学厚度大于0.312大陆性气溶胶,SSA误差在±0.0418以内;(2)波长无关的宽带地表反照率适用于SSA反演;(3)气溶胶光学厚度越大,辐射资料误差所引起的SSA解误差越小.当辐射误差在±2%以内以及0.55 μm气溶胶光学厚度大于0.312时,SSA解的误差在±0.0149以内; 辐射误差在±4%以内时,SSA解的误差在±0.0317以内.     

Comment on 'Systematic determination of earthquake rupture directivity and fault planes from analysis of long-period P-wave spectra' by L. M. Warren and P. M. Shearer

Warren and Shearer describe a method of estimating the duration of P pulses radiated by earthquakes, on the assumption that the source is a unilateral fracture. The estimates are made in the frequency domain. The estimates obtained by Warren and Shearer for seven of the earthquakes are compared to durations estimated here in the time domain; the time-domain measurements being made on broad-band seismograms (∼0.1–4.0 Hz) derived by filtering from short-period recordings. Overall, the time-domain method indicates that the pulse duration of the earthquakes studied here range from 2.0 to 7.6 s, whereas the estimates from the results of Warren and Shearer range from 7.1 to 9.8 s. This suggests that the method of Warren and Shearer cannot resolve pulse lengths less than about 7 s. The suggestion is supported by the estimates of the duration of rupture—fault length/speed of rupture—implied by the results of Warren and Shearer. For, although the estimated fault-length ranges from 0.8 km to over 40 km most rupture durations are around 8 s.     

Differences in the Crustal and Uppermost Mantle Structure of the Bohemian Massif from Teleseismic Receiver Functions

A target of our study was the Bohemian Massif in Central Europe that was emplaced during the Variscan orogeny. We used teleseismic records from ten broadband stations lying within and around the massif. Different techniques of receiver function interpretation were applied, including 1-D inversion of R- and Q-components, forward modelling of V _s velocity, and simultaneous determination of Moho depth and Poissons ratio in the crust. These results provide new, independent information about the distribution of S wave velocity down to about 60 km depth. In the area of Bohemian Massif, the crustal thickness varies from 29 km in the NW to 40 km in the SE. A relatively simple velocity structure with gradually increasing velocities in the crust and uppermost mantle is observed in the eastern part of the Bohemian Massif. The western part of the massif is characterized by more complicated structure with low S wave velocities in the upper crust, as well as in the uppermost mantle. This could be related to tectono-magmatic activity in the Eger rift that started in the uppermost Cretaceous and was active in the West Bohemia-Vogland area till the late Cenozoic.     

RADIATIVE COOLING AND BROADBAND PHENOMENON IN LOW-FREQUENCY WAVES

In this paper, we analyze the effects of radiative cooling on the pure baroclinic low-frequency waves under the approximation of equatorial β-plane and semi-geostrophic condition. The results show that radiative cooling does not, exclusively, provide the damping effects on the development of low-frequency waves.Under the delicate radiative-convective equilibrium, radiative effects will alter the phase speed and wave period,and bring about the broadband of phase velocity and wave period by adjusting the vertical profiles of diabaticheating. When the intensity of diabatic heating is moderate and appropriate, it is conductive to the development and sustaining of the low-frequency waves and their broadband phenomena, not the larger, the better. The radiative cooling cannot be neglected in order to reach the moderate and appropriate intensity of diabatic heating.