太行山南段沟谷杂木林的群落学特征及起源初探   总被引：1，自引：0，他引：1  

刘鸿雁 《地理科学》1995,15(2):188-195

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班公湖—怒江构造带西段三叠纪—侏罗纪构造—沉积演化   总被引：20，自引：2，他引：20  

王冠民  钟建华 《地质论评》2002,48(3):297-303

班公湖－怒江构造带西段在大地构造位置上处于特提斯构造域东端，横跨班公湖－怒江断裂带。三叠纪－株罗纪期间，其构造－沉积演化经历了大陆初始裂谷（T）、原洋裂谷（J1）、残余弧后盆地（J2－J3）阶段。初始裂谷阶段的拉张是呈南断北超的半地堑式由东向西进行的，逐渐形成地堑式原洋裂谷盆地。中晚侏罗世，南部新特提斯洋壳开始北各俯冲,产生的区域挤压应力使原洋裂谷逐渐封闭，裂谷盆地的小洋壳表现出以南向俯冲为主的双向式腑冲，同时伴生区域热沉降，盆地具残余弧后盆地的性质。该阶段,羌南地区发育碳酸盐岩为主的稳定陆缘沉积，冈度斯－念青唐古拉板片北部则形成广泛南超的近源碎屑沉积。  相似文献   

Assessing natural and cultural influence on soil in remnant tropical woodlands     

C Y Jim  Michael W H Chan 《Area》2004,36(1):6-18

Rural Hong Kong contains culturally protected enclaves of remnant woodlands that provide sanctuary for vegetation, wildlife and soil. This study focuses on the influence of natural and cultural factors on soil properties in woodlands with different human activities. At each of the nine selected sites, two pits were dug to collect soil samples for analysis of 24 physical and chemical properties. Analyses of variance between soil attributes and site factors suggest the prominence of woodland size, and important contribution of topography, aspect and parent material. Soil indicators of human impacts and the tenacity of woodland soil towards anthropogenic disturbance were demonstrated.  相似文献   

Upper-mantle reflectors: modelling of seismic wavefield characteristics and tectonic implications     

T. M. Hansen  N. Balling 《Geophysical Journal International》2004,157(2):664-682

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祁连山蛇绿岩型超镁铁岩铬铁矿床成矿的主要特征   总被引：4，自引：0，他引：4  

苟国朝  田培昭等 《甘肃地质》1993,2(1):35-45

祁连山造山带目前已发现不同规模的超镁铁岩体（群）1000余个,产有铬铁矿床（点）和矿化点80余处,这些岩体及其矿产主要产在北祁连优地斜增生地体边部的海沟带中,少数产在祁连中间地块的边部。岩体成因类型为蛇绿岩组合中的超镁铁质单元,铬铁矿的富集部位是地幔橄榄岩和堆积杂岩带底部的纯橄榄岩。岩石多为铝过饱和系列,岩体的平均化学成分接近于斜辉橄榄岩;Cr₂0₃的平均含量大于0.40％,Al₂0₃的平均含量近于或者大于1％。铬尖晶石的化学参数特征反映出低铁富镁的介质对形成富铬尖晶石是有利的。富铬岩体中Cr、Co、Ti、V的含量较高。  相似文献   

A possible explanation of photon emission from supernova remnants by jitter radiation     

T. Ogasawara  T. Yoshida  S. Yanagita  T. Kifune 《Astrophysics and Space Science》2007,309(1-4):401-405

We investigate a possibility that non-thermal X-ray emission in a supernova remnant(SNR) is produced by jitter radiation, which is the analogue of synchrotron radiation in small-scale random magnetic fields. We can fit the multi-wavelength data of SNRs RX J1713.7-3946 (G347.3-0.5) and RX J0852.0-4622 (G266.6-1.2) by constructing pure jitter and inverse Compton (IC) emission models. We find that the physical fit parameters of random magnetic fields take values of several tens of μG strength and of the order of ∼10⁷ cm correlation length. These properties of random magnetic fields in collisionless shock of SNRs are discussed.   相似文献   

Radio-silent isolated neutron stars as a new astronomical reality     

Patrizia A. Caraveo  Giovanni F. Bignami  Joachim E. Trümper 《Astronomy and Astrophysics Review》1996,7(3):209-216

Summary. As of today, seven X-ray sources have been tentatively identified as radio-quiet, isolated neutron stars. The family appears to be a rapidly growing one, although not all the objects have been identified with the same degree of certainty. The most convincing example of radio quiet pulsar is certainly Geminga, the neutron star nature of which, proposed in 1983 on the basis of its similarity with the Vela pulsar, has been firmly established with the discovery of its X and pulsation. Four more neutron star candidates, originally found in the Einstein data, have been confirmed by ROSAT, which has added to the list two more entries. All this is not the result of an unbiased search. The seven sources were not selected at random: four are inside supernova remnants, an obvious place to search for isolated neutron stars, while the remaining three were singled out because of some peculiarity. Intense -ray emission in the case of Geminga, very high X-ray counting rate for RXJ185635-3754, or being the brightest unidentified source in the Einstein medium sensitivity survey, MS 0317-6647. In spite of the limited number of objects and of the observational biases, these seven radio quiet neutron star candidates add valuable pieces of information to the observational panorama of known pulsars. Their properties, inferred from the X-ray emission, offer a coherent picture, pointing towards thermally emitting, cooling neutron stars. Received: April 1, 1996  相似文献   

Analytical Study of Supernova Remnant Non-Stationary Expansions     

X. Ribeyre  V. T. Tikhonchuk  S. Bouquet 《Astrophysics and Space Science》2005,298(1-2):75-80

We study analytically the Rayleigh–Taylor instability in expanding supernova gas shell. The instability appears at the inner shell surface accelerated by blowing pulsar wind. The most dangerous perturbations correspond to wavelengths comparable to the shell thickness. We analyze the fragility of the supernova remnant shell in function of the initial perturbation amplitude and the shell thickness.  相似文献   

大厚度自重湿陷性黄土湿陷变形特性水分入渗规律及地基处理方法研究   总被引：1，自引：0，他引：1  

黄雪峰  张广平  姚志华  张建华 《岩土力学》2011,32(Z2):100-108

为研究大厚度自重湿陷性黄土的湿陷变形特性、水分入渗规律以及地基处理合理方法等问题,选择典型大厚度自重湿陷性黄土场地,进行了布置沉降观测点和埋设水分计的浸水试验以及挤密桩、DDC（孔内深层强夯）桩地基处理试验。试验结果表明,在水分入渗过程中,深度22.5～25.0 m以上土体易发生湿陷,该深度以下土体则含水率增加缓慢,达不到湿陷起始含水率,不易发生湿陷,因此该深度考虑可作为现场湿陷性评价的临界深度,也可作为大厚度湿陷性黄土地区进行地基处理时可参考的地基处理下限深度。DDC桩间距为1.0～1.4 m时,无论从挤密系数还是湿陷系数都能满足规范要求;挤密桩15 m试验区域沉降量较小,但其剩余湿陷量任未满足要求,这也佐证了关于22.5～25.0 m深度难于发生湿陷的结论。试验成果可作为今后大厚度自重湿陷性黄土地区工程建设以及黄土规范进一步修订的参考。  相似文献   

昔格达断裂晚第四纪活动特征及强震复发周期     

卢海峰  姬志杰 《现代地质》2011,25(3)

利用冲沟、山脊等断错构造地貌的DEM影像资料和详实的野外踏勘,详细分析了昔格达断裂的晚第四纪活动特征。结果显示:断裂线两侧的河沟和山脊地貌呈"S"或反"Z"形或以多个首尾连接的"S"形雁列式斜列,断裂活动为左行左列式,断层上发育多个拉分盆地和断裂湖;该断裂最新活动时间晚于(12.83±1.09)ka,为全新世走滑活动断裂,倾滑分量不大,倾向总体西倾,且晚更新世以来的左旋走滑速率约为1.70 mm/a;依据断裂线地震遗迹及断裂活动特征,断裂强活动复发间隔大致为10~12 ka或更短。  相似文献