藏北长江源地区河流地貌特征及其对新构造运动的响应   总被引：9，自引：1，他引：9       下载免费PDF全文

李亚林  王成善王 谋 伊海生 李 勇 《中国地质》2006,33(2):374-382

对藏北长江源地区河谷地貌和新构造变形调查发现,该区具有平行式水系格局,河谷地貌以形态不同的窄谷和宽谷为特点,新近纪以来该区主要经历了早期挤压和晚期伸展构造演化过程,产生了褶皱-逆冲、走滑剪切、正断层和地堑构造3种构造变形样式。长江源区河谷地貌的形成演化明显受新构造运动的影响,新构造运动不仅控制了河谷地貌形态与水系格局,而且影响了河流阶地分布以及洪(冲)积扇的形态、结构。长江源地区主要水系至少自全新世以来是沿新构造运动产生的不同性质断裂构造溯源侵蚀发育而成。  相似文献   

一矿山开采崩落区的岩体变形及崩落角确定          下载免费PDF全文

牟会宠 《地质科学》1974,9(2):133-145

矿山地下开采过程中,由于采出了大量的矿体,上部岩体失去支撑,破坏了原有的平衡,因此岩体就破裂、变形,地表上则表现为塌陷、裂缝以及肉眼难以分辨的地面变形,矿坑内则表现为片帮、冒顶、底鼓等。  相似文献   

Growth and energy budget of juvenile lenok Brachymystax lenok in relation to ration level     

刘洋  李钟杰  张堂林  苑晶  牟振波  刘家寿 《中国海洋湖沼学报》2015,33(2):347-355

We evaluated the effect of ration level(RL) on the growth and energy budget of lenok Brachymystax lenok. Juvenile lenok(initial mean body weight 3.06±0.13 g) were fed for 21 d at five different ration levels: starvation,2%,3%,4% bwd(body weight per day,based on initial mean values),and apparent satiation. Feed consumption,apparent digestibility,and growth were directly measured. Specific growth rates in terms of wet weight,dry weight,protein,and energy increased logarithmically with an increase in ration levels. The relationship between specific growth rate in terms of wet weight(SGRw,%/d) and RL(%) was characterized by a decelerating curve: SGRw=-1.417+3.166ln(RL+1). The apparent digestibility coefficients of energy exhibited a decreasing pattern with increasing ration level,and there was a significant difference among different RLs. Body composition was significantly affected by ration size. The relationship between feed efficiency rate in terms of energy(FERe) and RL was: FERe=-14.167+23.793RL–3.367(RL)2,and the maximum FERe was observed at a 3.53% ration. The maintenance requirement for energy of juvenile lenok was 105.39 k J BW(kg)-0.80/d,the utilization efficiency of DE for growth was 0.496. The energy budget equation at satiation was: 100IE=29.03FE+5.78(ZE+UE)+39.56 HE+25.63 RE,where IE is feed energy,FE is fecal energy,ZE+UE is excretory energy,HE is heat production,and RE is recovered energy. Our results suggest that the most suitable feeding rate for juvenile lenok aquaculture for wet weight growth is 2.89% bwd,whereas for energy growth,the suggested rate is 3.53% bwd at this growth stage.  相似文献   

Slow and Fast Rotating Coronal Holes from Geomagnetic Indices     

Mikhail G. Shnirman  Jean-Louis Le Mouël  Elena M. Blanter 《Solar physics》2010,266(1):159-171

The evolution of the 27-day recurrence in the series of two solar indices (Wolf number WN and 10.7 cm radio flux F) and two geomagnetic indices (Dst and ζ, variance of the geomagnetic field recorded at a magnetic observatory) have been studied over the 1957 – 2007 time span. Spectral energies contained in two period domains (25 – 27.3 and 27.3 – 31 days), designated as E ₁ and E ₂, have been computed. Whereas the evolution of E ₁ is the same for the four indices, that of E ₂ is essentially different for WN and F on the one hand, Dst and ζ on the other hand. Some general conclusions on the dynamics of the solar outer layers are inferred from these results. First the solar activity, as measured by WN, and when averaged over a few years, evolves in the same way whatever the latitude. Second, two families of coronal holes (CHs) are identified; the rapidly and the slowly rotating CHs evolve quite differently.  相似文献   

四川盆地南部下三叠统飞仙关组一段台内鲕滩的主控因素   总被引：2，自引：0，他引：2  

谭秀成  牟晓慧  罗冰  刘宏  刘晓光  丁熊  吴晓庆  吴兴波 《古地理学报》2010,12(1):49-55

四川盆地飞仙关组台缘鲕滩气田的发现,激励了人们重新认识台内鲕滩的发育分布规律及其勘探前景。根据野外露头及钻孔资料的分析,认为四川盆地南部飞仙关组一段的台内鲕滩具有发育向上变浅序列、单滩体厚度一般小于3m、横向连续性较差的特征。着重分析了沉积期古地貌、古水深、海水动荡程度以及古海平面相对升降变化对台内鲕滩的控制作用,并把滩体的发育阶段分为雏滩期(低速建造期)、滩核期(高建造期)及衰亡期3个阶段。结果表明,在缓慢等效的海退过程中,处于高能沉积界面附近的水下古高地有利于台内鲕滩的形成,继承性的泸州古隆起核部是区内有利的滩体发育区,形成的台内滩体具有一定的厚度规模和较大的分布面积。这一认识可为该区飞仙关组台内鲕滩的下一步勘探提供必要的地质支持。  相似文献   

黔东南地区新元古代下江群的地层年代及其地质意义   总被引：3，自引：0，他引：3       下载免费PDF全文

覃永军  杜远生  牟军  卢定彪  龙建喜  王安华  张厚松  曾昌兴 《地球科学》2015,40(7):1107-1120

黔东南地区下江群是分布在江南造山带西段的一套前寒武纪浅变质陆源碎屑岩夹火山碎屑岩组合, 其地层时代归属与划分特别是区域地层对比一直未能得到很好解决.在对该区前寒武纪地层广泛而详细的剖面测制和地质调查基础上, 运用LA-ICP-MS技术, 对地层中沉凝灰岩、含凝灰质碎屑岩和碎屑岩进行锆石U-Pb年代学测试, 获得一批高精度的年龄.四堡群河村组顶部的碎屑岩和下江群乌叶组第1段顶部的含凝灰质碎屑岩、清水江组底部与中部的沉凝灰岩、平略组中上部的含凝灰质碎屑岩、隆里组中下部的碎屑岩等样品中锆石U-Pb最小年龄组的加权平均年龄分别为819.8±6.4Ma和779.5±4.7Ma、764.0±6.3Ma与(756.8±7.6Ma、756.0±13.0Ma)、733.9±8.8Ma及725.0±10.0Ma.这些数据将四堡群和下江群的时代限制为新元古代.结合研究区隆里组与长安组整合接触关系和全球低纬度南华系冰期起始年龄(717.4Ma)的地质事实, 将下江群沉积时限约束在815~717Ma之间.根据区域岩浆事件进一步约束了下江群各组段的地层时限, 并开展江南造山带下江群及其相当层位的地层划分与对比, 认为新元古代岩浆作用制约着黔东南下江群盆地的演化.   相似文献   

一种亮星识别算法及其在天文定向中的应用     

詹银虎  郑勇  张超  李铸洋  张中凯 《测绘学报》2015,44(3):257-263

基于全站仪对任意亮星的观测采样,提出了一种利用高度角序列和水平角速率进行联合匹配的任意亮星识别算法。通过引入天体地平坐标计算程序,算法可正确辨别行星和恒星。本文分析了任意亮星高度角和水平角速率的观测误差和计算误差,以此给出了匹配阈值条件的设定依据,并在此基础上制定了有效的匹配策略。仿真计算及实际观测试验均表明,该算法具有100%的识别成功率,远优于现有算法。将此算法应用于任意亮星天文定向,定向结果的内符合精度达到2″,外部检核精度达到1.6″。采用多颗任意亮星进行定向,可有效减弱由测站位置误差引入的定向系统误差,提高绝对定向精度。本文提出的天文定向适用于多云及雾霾天气。  相似文献   

隐形碳关税:概念辨析与国际治理     

王谋 《气候变化研究进展》2020,16(2):243-250

碳关税是各国高度关注的贸易问题,因涉及各国经贸利益,南北国家在碳关税问题上分歧很大。任何有关碳关税的政策措施,都会引起发展中国家的强烈反对。因此,部分发达国家试图另辟蹊径,在国际贸易中通过增加生产标准、碳标签等技术要求,以比较隐蔽的方式实现执行碳关税的目的。文中将这些隐蔽的但能起到碳关税执行效果的政策措施归纳为隐形碳关税,并定义隐形碳关税是指那些虽然没有在边境环节征收碳关税,但与征收碳关税起到相同贸易壁垒作用的,对发展中国家出口产品和服务构成限制的政策和措施。隐形碳关税比较典型的表现形式包括生产标准、碳标签等措施。这些措施本身是政策中性的,并不构成隐形碳关税,但如果叠加了转移应对气候变化成本、限制发展中国家产业发展等目的,这些措施的性质便不再中性,而成为现实中的贸易壁垒。隐形碳关税的治理应该是国际气候治理进程的一个部分,《联合国气候变化框架公约》则应是隐形碳关税治理的主要国际平台。无论是在气候公约内还是气候公约外的治理机制,隐形碳关税的国际治理都应遵循气候公约的相关原则,尤其是共同但有区别责任原则,区别对待发达和发展中国家的责任和义务,充分发挥生产标准、碳标签等措施的积极环境效用,同时约束其不当使用,建立公平、互信、务实的国际合作模式,实现气候治理与经济发展的协同。  相似文献   

Kuramoto Model of Nonlinear Coupled Oscillators as a Way for Understanding Phase Synchronization: Application to Solar and Geomagnetic Indices     

Elena M. Blanter  Jean-Louis Le Mouël  Mikhail G. Shnirman  Vincent Courtillot 《Solar physics》2014,289(11):4309-4333

We apply a Kuramoto model of nonlinear coupled oscillators to the simulation of slow variations of the phase difference between sunspot number [R _I ] and geomagnetic indices [aa and ζ]. The Kuramoto model is described for the particular case of two oscillators connected by symmetric coupling with quasi-stationary behavior, and its properties are investigated. By solving an inverse problem, we reconstruct the evolution of the couplings between pairs of indices [R _I and aa, R _I and ζ, aa and ζ], and interpret these in terms of the physics of the solar dynamo. The de-correlation between R _I and geomagnetic indices found in Solar Cycle 20 by Le Mouël et al. (J. Geophys. Res. 117, A09103, 2012) is successfully reproduced by the Kuramoto model and corresponds to the alternation of the leading oscillator. Application of the Kuramoto model to the cross-correlations [C(R _I ,ζ) and C(aa,ζ)] for ζ-indices computed in eight geomagnetic stations shows the latitudinal dependence of the mean phase difference. We discuss these results in terms of the solar-wind contribution to local geomagnetic indices [ζ].  相似文献   

Surface gravitational field and topography changes induced by the Earth’s fluid core motions     

M.?Greff-LefftzEmail author  M. A.?Pais  J.-L. Le?Mou?l 《Journal of Geodesy》2004,78(6):386-392

Using a Love number formalism, the elastic deformations of the mantle and the mass redistribution gravitational potential within the Earth induced by the fluid pressure acting at the core–mantle boundary (CMB) are computed. This pressure field changes at a decadal time scale and may be estimated from observations of the surface magnetic field and its secular variation. First, using a spherical harmonic expansion, the poloidal and toroidal part of the fluid velocity field at the CMB for the last 40 years is computed, under the hypothesis of tangential geostrophy. Then the associated geostrophic pressure, whose order of magnitude is about 1000 Pa, is computed. The surface topography induced by this pressure field is computed using Love numbers, and is a few millimetres. The mass redistribution gravitational potential induced by these deformations and, in particular, the zonal components of the related surface gravitational potential perturbation (J₂, J₃ and J₄ coefficients), are calculated. Overall perturbations for the J₂ coefficient of about 10^–10, for J₃ of about 10^–11 and for J₄ are found of about 0.3×10^–11. Finally, these theoretical results are compared with recent observations of the decadal variation of J₂ from satellite laser ranging. Results concerning J₂ can be described as follows: first, they are one order of magnitude too small to explain the observed decadal variation of J₂ and, second, they show a significant linear trend over the last 40 years, whose rate of decrease amounts to 7% of the observed value.  相似文献