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181.
182.
利用大型通用有限元分析软件ANSYS简单模拟辽西地区中生代末期岩石圈动力学演化过程。为了与现今实际地质观测一致,我们分两步模拟了辽西中生代岩石圈的动力学演化。第一阶段,中国东部显著的地幔上升热柱导致本研究区壳-幔边界上升,岩石圈减薄,同时伴有少量断层发育;第二阶段,地幔热柱上涌活动逐渐减弱,地表产生沉降。这一地质模型可重塑与现代观测一致的裂谷沉降、裂谷侧翼地形、壳-幔边界隆升。研究结果表明:ANSYS软件及有限元方法在岩石圈动力学数值模拟领域是一个非常有效的分析工具,具有非常广阔的应用前景。今后将建立与实际情况更吻合的岩石圈结构模型,真正动态地实现辽西中生代盆地区岩石圈结构的演化过程模拟。 相似文献
183.
陕西省矿床成矿系列的初步划分 总被引:8,自引:4,他引:8
通过系统总结,首次将陕西省主要矿床初步划分为4个矿床成矿系列组合,22个成矿系列类型,42个成矿系列和若干亚系列。其中省内金矿床的主要成矿系列为燕山期与变质一岩浆热液有关的金多金属矿床成矿系列、略勉板内结合带与岩浆热液有关的金矿成矿系列、商丹板块对接带与变质热液有关的金矿床成矿系列、现代河流中的冲一洪积砂金矿床成矿系列、与热水渗滤作用有关的金矿床成矿系列及活动区造山带与碱性碳酸盐类有关的金矿床成矿系列类型,银矿床的主要成矿系列为复理式建造中的菱铁矿银多金属矿床成矿系列,铜矿床的主要成矿系列为与元古代中-酸性岩有关的铁铜矿床成矿系列、加里东-印支期与中性-酸性花岗岩类有关的铁铜金钨萤石矿床成矿系列、与海相中基性火山岩有关的铜锌矿床成矿系列、前寒武系变质火山岩中的铜锌黄铁矿床成矿系列,钼矿床的主要成矿系列为与中酸性浅成-超浅成小岩体(斑岩)有关的钼铁铜矿床成矿系列,铅锌矿床的主要成矿系列为海底热液喷流-沉积铅锌矿床成矿系列、与热水渗滤作用有关的铅锌矿床成矿系列、海底喷流沉积-热液改造铅锌铜矿床成矿系列,汞锑矿床的主要成矿系列为与热水渗滤作用有关的汞锑矿床成矿系列,重晶石矿床的主要成矿系列为寒武系-奥陶系中的钒钼重晶石磷块岩黄铁矿石煤矿床成矿系列、下志留统中的重晶石铀石煤矿床成矿系列,煤矿床的主要成矿系列为大型内陆盆地中的煤油页岩成矿系列及与海陆交互相沉积岩有关的煤铝黄铁矿粘土高岭土矿床成矿系列类型,岩盐矿床的主要成矿系列为产于奥陶系中的岩盐(钠盐)矿床成矿系列。 相似文献
184.
Accelerating the T‐matrix approach to seismic full‐waveform inversion by domain decomposition 下载免费PDF全文
A seismic variant of the distorted Born iterative inversion method, which is commonly used in electromagnetic and acoustic (medical) imaging, has been recently developed on the basis of the T‐matrix approach of multiple scattering theory. The distorted Born iterative method is consistent with the Gauss–Newton method, but its implementation is different, and there are potentially significant computational advantages of using the T‐matrix approach in this context. It has been shown that the computational cost associated with the updating of the background medium Green functions after each iteration can be reduced via the use of various linearisation or quasi‐linearisation techniques. However, these techniques for reducing the computational cost may not work well in the presence of strong contrasts. To deal with this, we have now developed a domain decomposition method, which allows one to decompose the seismic velocity model into an arbitrary number of heterogeneous domains that can be treated separately and in parallel. The new domain decomposition method is based on the concept of a scattering‐path matrix, which is well known in solid‐state physics. If the seismic model consists of different domains that are well separated (e.g., different reservoirs within a sedimentary basin), then the scattering‐path matrix formulation can be used to derive approximations that are sufficiently accurate but far more speedy and much less memory demanding because they ignore the interaction between different domains. However, we show here that one can also use the scattering‐path matrix formulation to calculate the overall T‐matrix for a large model exactly without any approximations at a computational cost that is significantly smaller than the cost associated with an exact formal matrix inversion solution. This is because we have derived exact analytical results for the special case of two interacting domains and combined them with Strassen's formulas for fast recursive matrix inversion. To illustrate the fact that we have accelerated the T‐matrix approach to full‐waveform inversion by domain decomposition, we perform a series of numerical experiments based on synthetic data associated with a complex salt model and a simpler two‐dimensional model that can be naturally decomposed into separate upper and lower domains. If the domain decomposition method is combined with an additional layer of multi‐scale regularisation (based on spatial smoothing of the sensitivity matrix and the data residual vector along the receiver line) beyond standard sequential frequency inversion, then one apparently can also obtain stable inversion results in the absence of ultra‐low frequencies and reduced computation times. 相似文献
185.
NDCI法Ⅱ类水体叶绿素a浓度高光谱遥感数据估算 总被引:1,自引:0,他引:1
以太湖、巢湖为研究区,以Hyperion和HJ-1A卫星HSI高光谱数据以及实测水质浓度数据为实验数据,引入归一化叶绿素指数(NDCI),对Ⅱ类水体的高光谱叶绿素a浓度估算进行分析研究.首先对高光谱数据的光谱通道设置以及水体光谱特征进行分析,研究确定模型的最优波段.然后,将确定最优波段后的NDCI反射率因子作为变量与实测样本点数据进行回归分析,得到NDCI与叶绿素a浓度之间的回归关系,进行叶绿素a浓度的估算.与常用的比值法、一阶微分法和三波段法相比,NDCI的性能优于这3种方法,表明NDCI是一种计算简单、估算精度高、实用性强的Ⅱ类水体叶绿素a浓度估算方法. 相似文献
186.
R. Brajša H. Wöhl B. Vršnak V. Rušdjak F. Clette J.-F. Hochedez G. Verbanac M. Temmer 《Solar physics》2005,231(1-2):29-44
Full-disc full-resolution (FDFR) solar images obtained with the Extreme Ultraviolet Imaging Telescope (EIT) on board the Solar
and Heliospheric Observatory (SOHO) were used to analyse the centre-to-limb function and latitudinal distribution of coronal
bright points. The results obtained with the interactive and the automatic method, as well as for three subtypes of coronal
bright points for the time period 4 June 1998 to 22 May 1999 are presented and compared. An indication of a two-component
latitudinal distribution of coronal bright points was found. The central latitude of coronal bright points traced with the
interactive method lies between 10∘ and 20∘. This is closer to the equator than the average latitude of sunspots in the same period. Possible implications for the interpretation
of the solar differential rotation are discussed. In the appendix, possible differences between the two solar hemispheres
are analysed. More coronal bright points were present in the southern solar hemisphere than in the northern one. This asymmetry
is statistically significant for the interactive method and not for the automatic method. The visibility function is symmetrical
around the central meridian. 相似文献
187.
188.
利用国家气候中心整编的中国160个测站的月降水资料,提取1951—2012年江淮流域26站6、7月份的梅雨量距平场资料进行EOF分析,将梅雨雨型分为北涝南旱型和南涝北旱型。利用NCAR/NCEP再分析资料对两种空间分布的典型年大气环流背景特征进行合成分析,结果表明:北涝南旱年,高纬度鄂霍次克海高压阻塞形势偏强,极涡偏弱,西太平洋副热带高压和南亚高压位置偏北,东亚副热带夏季风偏强,水汽辐合中心偏北;南涝北旱年情形基本相反,高纬度鄂霍次克海高压阻塞形势和极涡偏强,西太平洋副热带高压和200 hPa南亚高压位置偏南,东亚副热带夏季风偏弱,水汽辐合中心偏南。 相似文献
189.
根据车西地区下古生界潜山的岩芯观察与稳定碳氧同位素数据,结合钻井地质、生产动态资料,划分了车西地区下古生界储层裂缝类型;研究了裂缝长度、宽度、倾角、充填等特征参数,并探讨了各参数间的相互关系;总结了裂缝特征参数与构造部位、埋藏深度、油气产量的关系。 相似文献
190.
Vršnak B. Ruždjak V. Brajša R. Zlobec P. Altaş L. Özgüç A. Aurass H. Schroll A. 《Solar physics》2000,194(2):285-303
A sample of 47 importance 1 flares whose H emission occurred or protruded over umbrae of major sunspots (so called Z-flares) was studied to investigate characteristics of the associated dm–m radio, microwave and soft X-ray emission as the energy release site permeats into regions of strong magnetic fields. A close time association was found between the microwave burst peak and the `contact' of the H emission with the sunspot umbra. The H emission attained maximum close to or a few minutes after the contact. The soft X-ray bursts were delayed more, attaining maximum 0–10 min after the contact. The onset of bursts in the dm–m wavelength range was associated with the period of growth or the peak of the microwave burst. Two categories of type III and IV bursts could be recognized: the ones starting some ten minutes before the microwave peak, and those that begin close to the microwave burst peak. Type III bursts occur preferably when the microwave burst peaks simultaneously with or after the contact. The results are explained presuming that the contact reveals a permeation of the energy release process into a region of strong magnetic fields, where the process intensifies, and where the accelerated particles have access to magnetic field lines extending to large coronal heights. Different manifestations of the energy release process in various magnetic field topologies are considered to account for the various time sequences observed. 相似文献