辽河盆地新生代多期构造热演化模拟

针对辽河盆地新生代拉张多期性的特点,提出一种适用于多期拉张盆地构造热演化模拟的纯剪切模型．该模型考虑了多期拉张的继承性、横向不均匀性以及拉张速率的可变性。通过几种拉张速率模式的对比,指出拉张速率模式的选择对模拟年轻盆地热演化过程具有重要意义．最后,利用该模型模拟研究了辽河盆地新生代的构造热演化历史．     

能见度的观测及其仪器

该文介绍了目前世界上普遍应用的几种能见度仪的工作原理,比较了其优缺点,阐述了我国与其他国家在此方面的差距,并对今后我国能见度观测工作提出建议。     

利用SAR图像监测海上石油污染的实验分析

本文讨论了利用ＳＡＲ 图像监测海上石油污染的理论依据和环境条件,并根据ＲＡＤＡＲＳＡＴ 卫星装载的合成孔径雷达（ＳＡＲ）图像对渤海ＣＢ－６Ａ 井组发生的原油（气）泄漏事件进行了初步的研究和分析。     

Low frequency radio emission from the &;#x2018;quiet&;#x2019; Sun

We present observations of the ‘quiet’ Sun close to the recent solar minimum (Cycle 22), with the Gauribidanur radioheliograph. Our main conclusion is that coronal streamers also influence the observed radio brightness temperature.     

Scattering characteristics in heterogeneously fractured reservoirs from waveform estimation

Offset-dependent characteristics of seismic scattering are useful for characterizing fractured reservoirs. We use two models that have different background medium properties and different azimuthal AVO responses to study elastic wave propagation and scattering in gas-saturated, heterogeneously fractured reservoirs. Heterogeneous fracture density distributions are built through stochastic modelling. Synthetic seismograms are generated by 3-D finite difference modelling, and waveforms along crack-normal and strike directions are considered in this paper. The multiple signal classification (MUSIC) frequency estimator is used in waveform estimation to provide frequency-domain attributes related to seismic wave scattering by fracture heterogeneity. Our results indicate that the strength of the scattering field is a function of the background medium. The strength also increases with increasing fracture scatterer density and with decreasing correlation length of spatial variations of fracture density. The scattering field is weak at the top of the fractured reservoir. The first-order results are dominated by velocity anisotropy of the mean fracture density field. However, the base of the fractured reservoir corresponds to a strong scattering field on which fracture heterogeneity has a larger effect and is characterized by the loss of coherence.     

Circular polarization by scattering from spheroidal dust grains

Large degrees of circular polarization at near-infrared wavelengths have been reported in the OMC1 star-forming region. This discovery, in combination with compelling evidence for the existence of non-spherical aligned grains in star formation regions, has prompted us to investigate scattering from spheroidal particles as a possible mechanism for the production of large circular polarization in reflection nebulae. We use a dipole calculation to model the small particle limit and a T -matrix code to treat arbitrarily sized particles. We find that size distributions of perfectly aligned spheroids, with only modest 2:1 axis ratios, are capable of producing circular polarization of up to 50 per cent when scattering unpolarized incident light. This is the case even for dielectric materials, such as 'astronomical silicate', as long as sufficient large particles are included in the size distribution. We consider the effects of particle alignment and find that spinning oblate spheroids should be much more efficient circular polarizers than equivalent prolate spheroids.     

纳米碳纤维红外消光数值计算

为探讨纳米碳纤维作为烟幕粒子的红外消光特性,基于电磁场理论建立了细直的纳米碳纤维感应电流积分方程,并利用矩量法进行了求解,导出了纳米碳纤维散射场及吸收、散射和消光截面的计算式.通过与变分法的计算结果相比较,表明了该方法的有效性.利用该方法数值分析了纳米碳纤维红外消光截面与入射场波长、入射角、纤维长度和半径的关系,计算结果为纳米碳纤维用于红外烟幕干扰提供了理论依据.