2D Coupled 3D:A New Numerical Model for Dual - Structured - Aquifer System     

Chen Chongxi  Fang Shuzhen  Lin Min 《中国地质大学学报(英文版)》1995,(1)

２Ｄ　Ｃｏｕｐｌｅｄ　３Ｄ：Ａ　Ｎｅｗ　Ｎｕｍｅｒｉｃａｌ　Ｍｏｄｅｌ　ｆｏｒＤｕａｌ－Ｓｔｒｕｃｔｕｒｅｄ－Ａｑｕｉｆｅｒ　Ｓｙｓｔｅｍ￥ＣｈｅｎＣｈｏｎｇｘｉ；ＦａｎｇＳｈｕｚｈｅｎ；ＬｉｎＭｉｎ（ＦａｃｕｌｔｙｏｆＥｎｖｉｒｏｎｍｅｎｔａｌＳｃ...  相似文献   

聚煤盆地富煤规律研究综述及展望     

解习农  程守田 《地球科学进展》1993,8(3):45-48

聚煤盆地富煤规律是煤地质学研究之焦点。富煤规律研究的突出进展主要包括聚煤模式、富煤带和富煤单元以及现代泥炭比较沉积学研究。尤其是近年来富煤单元和现代泥炭比较沉积学研究更清楚地揭示煤赋存规律与成因煤相和工艺煤相之间的内在联系,从而为聚煤盆地优质煤的预测提供有效的方法。  相似文献   

中国西部及邻区的地壳三维速度结构     

单新建  冯德益 《内陆地震》1993,7(2):142-150

用网格频散反演技术计算了155条瑞利面波混合频散数据,将中国大陆分为目前最小分格2°×2°,得到了中国西部及邻区深至80km地壳和上地幔顶部的三维剪切波SV速度结构。结果表明:(1)天山褶皱系地壳平均厚度为54km,上地壳平均速度为3.3km/s,下壳平均速度3.93km/s,上地幔盖层平均速度为4.64km/s,都偏大。北天山壳厚比天山薄,壳和上地幔盖层下均有低速层。(2)塔里木盆地中部地壳厚46km,到其边缘的昆仑山、天山地带壳厚增加到52～55km。壳内无低速层,壳平均速度很低,为3.49km/s,地表有9km的沉积层。(3)青藏高原莫霍面呈凹形,平均壳厚为67km,平均壳速度为3.58km/s。东西端存在壳内低速层,埋深为15～35km。(4)南北带为构造复杂的区域,莫霍面深度具有东高西低,南北两端高、中间低的特点,带内普遍存在壳内低速层。南北带从群速度、速度、莫霍面等深线都可看到明显的横向差异。(5)准噶尔盆地地壳厚47km,无壳内低速层,中地壳不明显。该区呈稳定的大陆壳结构。(6)柴达木盆地在正常速度的中壳顶部有一高速夹层,速度为3.72km/s,厚10km,上顶部埋深14km。  相似文献   

模糊识别的隶属原则及其应用     

罗晓峰 《新疆地质》1993,(1)

由于模糊识别之最大隶属原则,在实际应用中存在着某种上程度上的不足。本文提出了加势隶属原则、积势隶属原则及加权加势隶属原则、加权积势隶属原则。以此可综合考虑各种变量因素,并在最大限度上综合利用各种变量因素间的信息,以达到模糊识别的最佳效应。  相似文献   

风城碱性杂岩与有关含金刚石岩类对比的意义     

冉清昌  刘学珍 《吉林大学学报(地球科学版)》1993,(3)

迄今为止,对金刚石矿床的研究已取得了新的进展,国内外学音认为:“金伯利岩不是金刚石矿床的唯一母岩”,并且在碱性杂岩体中发现了许多具有工业价值的金刚石矿床。 通过对比辽宁凤城碱性杂岩与有关含金刚石矿床母岩(主要是钾镁煌斑岩)及其共生岩类的构造背景、岩石类型组合、矿物成分组合及岩石的主元素、微量元素和稀土元素特征,发现本区碱性杂岩体岩石与西澳钾镁煌斑岩很相似,尤其是与西澳白榴石钾镁煌斑岩最为接近,而在岩石类型和矿物组合特点上,又与美国阿肯色碱性岩区金刚石矿床母岩及其共生岩类组合颇为相似,这为我们进一步找寻金刚石矿床提供某些有益的信息。  相似文献   

新疆天山地震活动图象缺信量Iq值的研究     

周仕勇 《内陆地震》1993,7(2):114-120

从信息量的角度出发,研究定量描述地震活动时空分布异常图象的方法,并定义缺信量I_q值来定量分析地震活动在时间轴上或空间上分布图象的异常程度。文中还根据1978～1990年新疆天山部分地区的地震资料,计算出了4条I_q——t曲线,发现在研究的时段和区域内发生的10多次M_s≥5.0级地震,绝大多数有I_q低值异常。  相似文献   

Statistical Properties of the Highest Pulses in Gamma-Ray Bursts   总被引：1，自引：0，他引：1  

Yi-Ping Qin  En-Wei Liang  Guang-Zhong Xie  Cheng-Yue SuNational Astronomical Observatories  Yunnan Observatory  Chinese Academy of Sciences  Kunming  qinyp@public.km.yn.cnDepartment of Physics  Guangxi University  Nanning  eloy@iaa.esDepartment of Physics  Guangdong Industry University  Guangzhou 《中国天文和天体物理学报》2003,3(1):38-48

We study the statistical properties of the highest pulses within individual gamma-ray bursts (GRBs). A wavelet package analysis technique and a developed pulse-finding algorithm have been applied to identify the highest pulses from burst profiles observed by BATSE on board CGRO from 1991 April 21 to 1999 January 26. The statistical light curves of the highest pulses in four energy channels have been derived by an aligning method, which illustrate the temporal evolution of the pulse emission. Our result that narrower pulses go with higher energies is consistent with previous findings. By normalizing both the pulse durations and counts to unity, “characteristic” profiles of the highest pulses in the four channels are also derived. The four characteristic profiles are turned out to be almost the same, thus strongly support the previous conclusion that the temporal profiles in different energy channels are self-similar and the previous conjecture on GRB pulses, implying that the emission process is similar at different energies. The cosmological time dilation effect is examined by investigating the relationship between the pulse flux and pulse duration. An anti-correlation between the two was found, which agrees with the expectation of the cosmological time dilation effect. Also, the evolution of the pulse duration with the observational epoch is studied. The result shows that the pulse duration tends to be shorter in later epochs. This trend cannot be explained by the present theoretical models, and may represent a great challenge to current theories.  相似文献   

低质量X射线双星的毫秒级准周期信号——最近的进展     

YU Wen-fei 《天文研究与技术》2003,(1):12-15

最近对低质量X射线双星中的千赫兹准周期振动的研究表明 ,是辐射压力 ,而不是盘和磁球的相互作用以及处于盘内边界的广义相对论效应在短时标的盘切断机制上起作用。本文给出了一些研究结果及讨论。  相似文献   

History of Star Formation and Chemical Enrichment in the Milky Way Disk   总被引：2，自引：0，他引：2  

Rui-Xiang Chang  Cheng-Gang Shu  Jin-Liang Hou Shanghai Astronomical Observatory  Chinese Academy of Sciences  Shanghai CAS-Peking University Joint Beijing Astronomical Center  Beijing 《中国天文和天体物理学报》2002,2(3)

Based on a physical treatment of the star formation law similar to that given by Efstathiou, we have improved our two-component chemical evolution model for the Milky Way disk. Two gas infall rates are compared, one exponential, one Gaussian. It is shown that the star formation law adopted in this paper depends more strongly on the gas surface density than that in Chang et al. It has large effects on the history of star formation and gas evolution of the whole disk. In the solar neighborhood, the history of chemical evolution and star formation is not sensitive to whether the infall rate is Gaussian or exponential. For the same infall time scale, both forms predict the same behavior for the current properties of the Galactic disk. The model predictions do depend on whether or not the infall time scale varies with the radius, but current available observations cannot decide which case is the more realistic. Our results also show that it would be inadequate to describe the gradient evolution along the Gala  相似文献   

使用小波技术自动搜寻天体谱线     

罗阿理  赵永恒 《中国天文和天体物理学报》2000,20(4)

使用小波技术对包括恒星、近邻星系和ＡＧＮ等不同的天体光谱进行了自动处理．用小波滤波的方法将光谱中的连续谱与诸线分离;然后使用小波域隐含马尔可夫模型（ＨＭＭ）,对已去掉连续谱的光谱进行降噪,同时得到了噪声在每个光谱中的分布;在训练ＨＭＭ的过程中,使用改进的Ｔｙｉｎｇ方法增加训练数据以保证训练的可靠性;利用噪声分布确定出谱线信号的局部阈值,在已经降噪的光谱中找到吸收线和发射线;用高斯函数拟会出谱线的形状,标出线心的波长值,作为自动证认的基础．  相似文献