大别山低级变质岩的构造背景     

徐树桐  吴维平  陆益群 《地质通报》2010,29(6):795-810

大别山南北两侧的浅变质岩是碰撞造山以前洋壳俯冲造山阶段的重要组成部分。木兰山片岩或张八岭群是俯冲的洋壳;苏家河群、信阳群和佛子岭群是由洋壳俯冲形成的海沟沉积,并因俯冲过程中的前进变形而形成增生楔;杨山煤系和梅山群是石炭纪弧前盆地沉积,并因俯冲过程中的前进变形而被增生楔逆掩。宿松群是扬子大陆被动边缘沉积,不是俯冲造山带的成员。因洋壳俯冲形成的弧和弧后盆地可能已被新生界沉积物掩盖。高压-超高压变质带是碰撞造山后期从深部折返的外来体。高压-超高压变质带正好处于洋壳和增生楔之间,破坏了早期洋壳俯冲造山带的完整性,使得洋壳俯冲造山阶段的特征被破坏,因而不易辨别。俯冲造山阶段应为奥陶纪到泥盆纪,碰撞造山阶段应从二叠纪开始。  相似文献   

伴有OH 1720 MHz脉泽发射的混合形态超新星遗迹的X射线特征研究     

俞志尧 《天文学报》2005,46(2):145-150

在银河系中，超新星遗迹的射电巡视揭示了19个伴有OH1720MHz脉泽发射的超新星遗迹．在从超新星遗迹膨胀到分子云的激波波面的后面产生了这一类不寻常的脉泽源．这个模型的重要点是从超新星遗迹来的X射线促使产生OH分子．研究伴有OH1720MHz脉泽发射的混合形态超新星遗迹的X射线特征是很重要的．研究了这19个伴有OH1720MHz脉泽发射的混合形态超新星遗迹的X射线特征．得到了这些源的X射线物理参数之间的一些相关关系和反相关关系．X射线电离率ζ与θ、D、r、r^2等物理量均不相关，而与Lx之间存在着正相关关系．另外超新星遗迹的X射线光度与相伴的OH1720MHz脉泽的最弱的束流量密度之间存在着紧密的正相关关系．这些都说明从超新星遗迹来的X射线发射足够在激波波阵面后面分解水分子并产生OH1720MHz脉泽．  相似文献   

Numerical simulation of the sudden rainstorm associated with the remnants of Typhoon Meranti (2010)     

周玲丽  杜惠良  翟国庆  王东海 《大气科学进展》2013,30(5):1353-1372

The Advanced Research Weather Forecasting (ARW) model was used to simulate the sudden heavy rainstorm associated with the remnants of Typhoon Meranti in September 2010. The results showed that the heavy rainfall was produced when the remnant clouds redeveloped suddenly, and the redevelopment was caused by rapid growth of micro/mesoscale convective systems (MCSs). As cold air intruded into the warm remnant clouds, the atmosphere became convectively unstable and frontogenesis happened due to strong wind shear between weak northerly flow and strong southwesterly flow in the lower levels. Under frontogenesis-forcing and warm-air advection stimulation in updrafts, vertical convection developed intensely inside the remnant clouds, with MCSs forming and maturing along the front. The genesis and development of MCSs was due to the great progress vertical vorticity made. The moist isentropic surface became slantwise as atmospheric baroclinity intensified when cold air intruded, which reduced the convective instability of the air.Meanwhile, vertical wind shear increased because the north cold air caused the wind direction to turn from south to north with height. In accordance with slantwise vorticity development (SVD), vertical vorticity would develop vigorously and contribute greatly to MCSs. Buoyancy, the pressure gradient, and the lifting of cold air were collectively the source of kinetic energy for rainfall. The low-level southwesterly jet from the western margin of the Western Pacific Subtropical High transported water and heat to remnant clouds. Energy bursts and continuous water vapor transportation played a major role in producing intense rainfall in a very short period of time.  相似文献   

Forearc serpentinite mélange from the Hongseong suture, South Korea   总被引：1，自引：0，他引：1  

Sung Won Kim  M. Santosh  Nari Park  Sanghoon Kwon 《Gondwana Research》2011,20(4):852-864

The signature of a prolonged subduction–accretion history from Paleozoic to Early Mesozoic is preserved within the dismembered serpentinite mélanges within the Hongseong suture. Here we present major and trace element data from the mafic fragments/blocks within the Baekdong serpentinite mélange revealing their arc-like tholeiite affinity within a suprasubduction zone tectonic setting. Chromian spinel compositions from the Baekdong hydrated mantle peridotite (serpentinite) are characterized by high Cr# (0.53–0.67) and Fe²⁺/Fe³⁺ ratio, medium Mg# (0.42–0.55), and Al₂O₃ contents (17–25 wt.%) indicating a forearc tectonic environment for the hydrated mantle peridotite. The estimated melting degree (> 17.6%) and FeO/MgO of the parental melt (0.9–1.3) are consistent with that of forearc magmas. SHRIMP zircon U–Pb ages from a high-grade mafic rock and an anorthosite from the study area give protolith ages of ~ 310 Ma and ~ 228 Ma, respectively. Zircons from an associated orthogneiss block within the mélange yield a Neoproterozoic crystallization age of ~ 748 Ma. These results, together with the recent SHRIMP zircon ages from other dismembered serpentinite mélanges within the Wolhyeonri complex, suggest that Paleozoic to Early Mesozoic subduction and subsequent collision events led to the exhumation of the hydrated forearc mantle peridotites from a metasomatized mantle wedge. The Hongseong region preserves important clues to a long-lived subduction system related to global events associated with the final amalgamation of the Pangaea supercontinent.  相似文献   

A study of the X-ray characteristics of mixed-morphology supernova remnants with 1720 MHz OH maser emission     

Zhi-yao Yu   《Chinese Astronomy and Astrophysics》2005,29(4):380-385

Radio surveys of supernova remnants (SNRs) in the Galaxy have discovered 19 SNRs which are accompanied by the OH maser emission at 1720 MHz. This unusual maser is thought to be produced behind a shock front when a SNR expands into a molecular cloud. An important ingredient of this model is that the X-ray emission from the remnant enhances the production of OH molecules. In this sense, to study the characteristics of the mixed-morphology SNRs accompanied by the OH maser emission at 1720 MHz is important. By studying the X-ray characteristics of the mixed-morphology SNRs accompanied by the 1720 MHz OH maser emission, it is found that the ionization rate of X-ray is not correlated with the physical parameters , D, r, r² and so on, but is correlated with the X-ray luminosity L_x. Meanwhile, L_x is closely correlated with the beam flux density of the weakest feature of the accompanying 1720 MHz OH maser emission. These mean that the X-ray emission from SNRs is sufficient to dissociate the water molecules behind a shock front and to produce the 1720 MHz OH masers.  相似文献   

Molecular Gas Distribution around the Supernova Remnant G40.5-0.5     

Ji Yang  Jie-Long Zhang  Zhi-Yong Cai  Deng-Rong Lu  You-Heng Tan Purple Mountain Observatory  Chinese Academy of Sciences  Nanjing  Key Laboratory of Particle Astrophysics  Institute of High-Energy Physics  Chinese Academy of Sciences  Beijing National Astronomical Observatories  Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2006,6(2):210-216

The distribution of dense molecular gas around the supernova remnant G40.5-0.5 has been investigated by radio spectroscopic observations in the CO (J = 1-0) transition. The molecular gas is found to extend over the entire region of G40.5-0.5. A molecular shell, with a diameter of - 26', coincides with the ionized gas as revealed by the cm-radio observations. This coincidence, along with the velocity discontinuity following the shell, provides direct evidence for interaction between the ionized gas and the dense molecular gas. No clear evidence for cosmic-ray acceleration can be identified from this SNR as previously suggested, due to positional uncertainty in relating the SNR shell defined by CO to the EGRET gamma-ray sources, GRO J1904 06, from the gamma-ray observations.  相似文献   

卫星遥感影像有理函数模型优化方法     

张永军  王蕾  鲁一慧 《测绘学报》2011,40(6):756-761

针对高分辨率遥感影像有理函数模型（RFM）在实际应用中存在过度参数化和定位精度不高的问题,提出基于离差阵和消去变换及残余系统误差补偿的高分辨率遥感影像RFM优化方法。试验结果表明,经过参数筛选后的RFM参数均为无偏估计值,拟合精度可以达到全部参数用于拟合时的精度,而且模型病态性基本消除,模型稳定性更高;残余系统误差补偿方法可以有效消除RFM拟合严格成像模型的残余误差,达到与严格成像模型一致的对地定位精度。  相似文献   

山东灵山岛晚中生代滑塌沉积层的发现及区域构造意义初探   总被引：6，自引：0，他引：6  

吕洪波  王俊  张海春 《地质学报》2011,85(6)

灵山岛位于青岛胶南市东南黄海近岸海域中,为中国北方第一高岛,构造上属于苏鲁造山带,但岛上很多重要的地质现象尚未在地质文献中披露过。本文作者对灵山岛进行了初步地质考察,在被看做早白垩世莱阳期的地层中发现远源浊积岩及其内部大量的滑塌沉积层,孢粉鉴定初步结果显示该地层的时代很可能为侏罗纪。滑塌构造以同沉积滑塌褶皱为主,而在滑塌体内部还发现有很多同沉积变形构造,如:同沉积布丁构造、同沉积拉伸线理、同沉积双重构造等。同沉积滑塌褶皱体的排列方向揭示了其物源来自南东方向,韵律层中弱粒序层单元颗粒为细砂到粉砂,反映出远源浊积岩的特征。根据滑塌体运移方向判断盆地的古地理特征为东南侧水体变浅而西北侧水体变深。滑塌沉积发育时,盆地为介于扬子板块和华北板块之间的残余洋盆。发育于砂质单元中的早期平面X剪节理指示了该套浊积岩在褶皱之前受到了SE—NW向的动态挤压,而后期的不对称褶皱构造记录了扬子板块自南东向北西侧的华北板块俯冲的历史。灵山岛中生代滑塌沉积层的发现不仅揭示了中国东部存在着晚中生代海相沉积,更为扬子板块与华北板块在郯庐断裂以东碰撞缝合的演化历史研究提供了珍贵的实际材料。  相似文献   

鄂尔多斯盆地延安地区奥陶系风化壳古地貌恢复   总被引：3，自引：0，他引：3  

王高平  王震亮  赵雪娇  李彦婧  王念喜  任来义  曹红霞 《沉积学报》2013,31(4):563-570

鄂尔多斯盆地东南部延安地区奥陶系马家沟组顶部发育风化壳岩溶储层,因古地貌代表了地层沉积和成岩作用的背景,因而在储层的形成和演化过程中具有重要意义。在区域构造背景和地层展布的基础上,综合利用残余厚度法和印模法,并结合铝土岩厚度分布和古沟槽识别结果,准确恢复出延安地区奥陶系风化壳古地貌分布格局。结果显示,延安地区西南部表现为古岩溶高地,中部大部分地区表现为古岩溶斜坡,东部属岩溶斜坡与岩溶盆地之间的过渡带。古地貌格局和古沟槽的分布影响了储层的形成、发育和天然气的富集。延安地区岩溶古高地、靠近侵蚀古沟槽的斜坡位置含气性较好,可能与大气水淋滤等因素导致的储层发育程度、物性好坏、不整合面之上盖层的封盖性等因素有关。  相似文献   

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陈品馨  章传银  黄昆学 《大地测量与地球动力学》2010,30(2):120-124

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