利用区域辐射特性优化获取光学遥感数据

通过分析成像过程及其影响因素,提出了对成像积分时间进行控制的优化成像方法。首先建立成像参数模型,探讨了模型参数计算、成像过程中模型参数的选择,分析了图像后处理问题,并利用北京一号小卫星进行了遥感数据优化获取实验。实验结果表明,根据地物特性进行成像参数优化后获取的图像具有更宽的动态范围和更高的辐射分辨率,信息量和信噪比也大幅增强。     

Correlated Radio-Optical Variations on Intraday Timescales

Correlated radio-optical variations on intraday timescales have been observed (e.g. In BLO 0716 714) and such radio intraday variability is suggested to have an intrinsic ori- gin. Recently, multi-wavelength observations, simultaneous at radio, mm-submm, optical and hard X-rays, of 0716 714, show that during a period of intraday/interday variations at ra- dio and mm wavelengths, the apparent brightness temperature of the source exceeded the Compton-limit (～1012 K) by 2--4 orders of magnitude, but no Compton catastrophe (or no high luminosity of inverse-Compton radiation) was detected. It is also found that the intra- day/interday variations at mm-submm wavelengths are consistent with the evolutionary be- havior of a standard synchrotron source and for the intraday/interday variations at centimeter wavelengths opacity effects can play a significant role, which is consistent with the interpreta- tion suggested previously by Qian et al. Thus the apparent high brightness temperatures may probably be explained in terms of Doppler boosting effects due to bulk relativistic motion of the source. We will argue a scenario to simulate the correlations between the radio and optical variations on intraday timescales observed in BLO 0716 714 in terms of a relativistic shock propagating through a jet with a dual structure.     

New active galactic nuclei among the INTEGRAL and SWIFT X-ray sources

We present the results of our optical identifications of a set of X-ray sources from the INTEGRAL and SWIFT all-sky surveys. The optical data have been obtained with the 1.5-m Russian-Turkish Telescope (RTT-150). Nine X-ray sources have been identified with active galactic nuclei (AGNs). Two of them are located in the nearby spiral galaxies MCG-01-05-047 and NGC 973 seen almost edge-on. One source, IGR J16562-3301, is probably a BL Lac object (blazar). The remaining AGNs are observed as the starlike nuclei of spiral galaxies whose spectra exhibit broad emission lines. The relation between the hard X-ray (17–60 keV) luminosity and the [O III] 5007 line luminosity, log L _x/L _{[O III]} ≈ 2.1, holds good for most of the AGNs detected in hard X rays. However, the luminosities of some AGNs deviate from this relation. The fraction of such objects can reach ～20%. In particular, the [O III] line flux is lower for two nearby edge-on spiral galaxies. This can be explained by the effect of absorption in the galactic disks.     

Optical identifications of five INTEGRAL hard X-ray sources in the Galactic plane

The results of optical identifications of five hard X-ray sources in the Galactic plane from the INTEGRAL all-sky survey are presented. The X-ray data on one source (IGR J20216+4359) are published for the first time. The optical observations were performed with the 1.5-m RTT-150 telescope (Turkish National Observatory, Antalya, Turkey) and the 6-m BTA telescope (Special Astrophysical Observatory, Nizhny Arkhyz, Russia). A blazar, three Seyfert galaxies, and a high-mass X-ray binary are among the identified sources.     

矿物白度的影响因素与增白机理研究

白度是矿物的重要光学性质之一。为了深化矿物的光学性质及白色矿物功能材料的研究与应用,根据测试分析结果和叶大年的结构光性矿物学理论,系统研究了影响矿物白度的主要因素,以及矿物增白效果的差异性及其产生机理。研究结果表明:(1)晶体化学是决定不同种类透明矿物白度的最主要因素,但对于某种透明矿物来说,影响其白度的主要因素是矿物中的碳质有机质、含铁钛矿物杂质、杂质元素的价态与晶体化学环境、介质环境、矿物中的水和粒度大小等。(2)证明了透明矿物白度大小与折射率呈正相关。白度相同的不同矿物的增白效果存在很大差异性,其根本原因是由矿物折射率所决定的反射率存在很大差别。(3)提出了真白度和假白度的概念,即主要由自色产生的白度称为真白度,主要由假色产生的白度称为假白度;真白度高的矿物具有增白作用,而真白度低的矿物,即使粉末白度高,也没有增白作用。(4)在影响矿物白度的主要因素中,矿物中的碳质有机质、含铁钛矿物杂质、杂质元素的价态等杂质成分对矿物白度和增白效果起负面作用。(5)矿物中与晶体结构相关的水所产生的颜色属于自色,脱去结晶水、层间水和结构水都有利于提高矿物的真白度或增白效果,但脱去沸石水的效果正好相反;由矿物粒度大小变化产生的颜色属于假色;通过降低粉体粒度大小所提高的白度属于假白度,由此增加的白度没有增白作用。另外,矿物粉体与使用介质之间的折射率大小差别越大,增白效果越明显。     

珠江口盆地惠州地区珠江组砂体上倾尖灭的地质-地球物理“逐级预测”方法

砂体上倾尖灭油气藏是岩性油气藏中重要类型之一,砂体上倾尖灭的刻画与描述是上倾尖灭圈闭有效性评价的关键。在以三角洲前缘沉积为主构成的三级层序内,三角洲沉积相关砂体上倾尖灭的地质-地球物理“逐级预测”描述方法对于认识上倾尖灭油气藏分布规律及其油气勘探具有重要意义。该方法由5个部分组成:在三级层序识别的基础上,运用高精度层序地层划分技术建立了四级层序构成的高频层序地层格架;在高频层序约束下,利用地震沉积学技术描述沉积相的平面分布;在地质模型指导下,利用频谱成像技术定性确定尖灭带的分布;利用相控储层反演半定量、定量预测砂体尖灭线;根据不同成因砂体的沉积特点,利用正演模拟技术开展尖灭线的外推预测。     

多信息多技术深度速度建模技术在复杂构造中的应用研究

中国西部等复杂区的油气勘探潜力较大,但地质条件复杂,造成常规偏移成像的精度不够,给解释带来了诸多困难。根据其地质特点,围绕高精度成像的需求,开展高精度速度建模技术研究,形成了配套的技术策略,为其进一步改善复杂区的成像精度,落实勘探目标奠定了基础。在该配套技术中:基于真地表的速度建模技术可以通过真地表数据准备来解决现有大圆滑偏移基准面对成像波场的改变、初至层析近地表建模技术的应用弥补了反射建模技术在近地表应用的不足、多信息约束速度建模可提高速度模型的可靠性、各向异性假设的成像技术更加接近复杂构造地下介质的假设,这些技术的配套应用可以有效提高复杂区成像位置的精度和准确度。在实际资料中的应用充分说明该技术的有效性。     

基于MODIS的长江口表层水体盐度时空分异

长江河口地处海陆交汇地区,其海表盐度受到长江流域、东海和三角洲社会经济活动的复合影响。水体盐度直观反映了河口区域冲淡水分布,对于研究淡水羽状锋、长江物质输送与河口环境变化等具有重要意义。本文分别对枯季和洪季的长江口盐度实测数据,以及中分辨率成像光谱仪（moderate-resolution imaging spectroradiometer,MODIS）遥感反射率与反射率的比值进行拟合回归分析,建立长江口表层盐度反演经验模型,得到枯季的相关系数和均方根误差（root-mean-square error,RMSE）分别为-0.930 3、0.45‰,洪季的相关系数和RMSE分别为-0.818 5、0.88‰;并分析模型在时间尺度上的适用性。利用该盐度反演模型对长江口2007-2016年的表层盐度进行反演,结合大通站记录的长江径流量观测资料,分析长江口表层水体盐度的时空变化规律。结果表明：长江口表层盐度受径流量影响较大,空间上呈自西向东递增趋势,具有季节性分异;枯季近岸盐度较高,高盐度海水可以到达长江口南北支分叉122.5°E附近;洪季冲淡水影响范围广,高盐度海水聚集在123°E以东、31°N以南,长江口北部出现低盐区域;2007-2016年间枯季大通站流量呈上升趋势,平均盐度为29.27‰,总体呈降低趋势,洪季大通站流量呈降低趋势,平均盐度为27.10‰,呈上升趋势,盐度和径流量在年际变化中存在良好的负相关关系。     

Stretching correction for amplitude-preserving vector wavefield reverse-time migration

The migration of multi-wave seismic data is aimed at obtaining the P- and S-wave imaging results of the amplitude preserving. But the P- and S-wave stretching effect produced by the reverse time migration of the elastic wave equation will not only reduce the vertical resolution of the migration results and the amplitude preserving of the large reflection angle. In this paper, the reverse time migration technique of amplitude preserving vector wave-field separating is used. Based on the analysis of the stretch mechanism and the influencing factors of stretch magnitude, the paper gave the stretch correcting factors. Then, realize the stretch correction method at the time that after the reverse extrapolation and before the imaging by solving the problem which is how to calculate the P-wave and Ps-wave propagation directions of imaging points at different times. The stretch correction method can improve the vertical resolution and amplitude fidelity of the imaging results and provide high fidelity input data for seismic data interpretation and inversion.© 2019 China Geology Editorial Office.     

绝对重力仪激光器光纤对准调节方法概述

绝对重力仪激光器光纤由于应力变化、形状改变、震动或耦合器维护等原因破坏了输出激光的偏振态,使其在光纤内的传输变得非常不稳定,导致光纤输出激光的消光比值小于100,无法满足绝对重力观测条件。针对该问题,介绍了光纤对准调节的方法,通过设计消光比检测装置检验消光比值是否大于100。对#181和#250两台WEO100型He-Ne激光器的光纤进行对准调节实验,并通过消光比检测装置实测,两台激光器输出的光束消光比值满足绝对重力测量的条件,表明该对准调节方法科学有效。