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21.
Qie  Wenkun  Ma  Xueping  Xu  Honghe  Qiao  Li  Liang  Kun  Guo  Wen  Song  Junjun  Chen  Bo  Lu  Jianfeng 《中国科学:地球科学(英文版)》2019,62(1):112-134
The Global Boundary Stratotype Sections and Points(GSSPs) for the bases of all seven international Devonian stages have been formally defined and ratified by IUGS till 1996, and nowadays, the main tasks for Devonian stratigraphers include further subdivision of these standard stages, strictly constrained absolute ages for the boundaries, and precise neritic-pelagic and marine-terrestrial correlations using multidisciplinary stratigraphy methods. Establishment of high-resolution Devonian integrative stratigraphy framework and timescale of China would play an important role in improving regional and international correlation, facilitating the recognition of important stratigraphic levels in different paleogeographic settings, and understanding the evolution pattern of biota, paleoclimate and paleoenvironment during this critical interval. Based on well-studied bio-and chronostratigraphy of Devonian in South China and adjacent areas, in combination with recent achievements in carbon isotope stratigraphy, event stratigraphy and radioactive isotope ages, this paper briefly summarize the research history and current status of Devonian chronostratigraphy of China, and for the first time introduce Devonian integrative stratigraphy framework of China.Up to date, few studies have been conducted on the astronomical cyclostratigraphy and high-resolution radioactive isotope dating in Devonian of China, which should be our main focuses in the near future.  相似文献   
22.
阔克塔格西碱性岩体出露于库鲁克塔格地块东段,兴地断裂南0.5km,呈椭圆状岩株产出,出露面积约17.5km2。岩体北部和西北部侵入于古元古界兴地塔格群中亚群大理岩、片岩及片麻岩之中,南部和东南部分别侵入于中元古代黑云母石英正长岩和黑云母角闪二长岩中。岩体从边部至中心可分为霓石钠长岩、霓石角闪正长岩和角闪正长岩3个岩相带。岩体边部内接触带形成ERR-Nb-Ta-Zr中型矿床。岩体锆石U-Pb年龄(LA-ICP-MS方法)为(224±2)Ma。岩石主要矿物为微斜长石和条纹长石,暗色矿物主要为钠铁闪石,具有碱性岩典型的富碱、低硅的特点。此外,富集轻稀土元素,负Eu异常,富集Nb、Ta、Th及Hf等高场强元素,亏损Sr、P及Ti不相容元素。Hf同位素特征显示岩浆源于富集岩石圈地幔。地球动力学背景属造山后的板内演化阶段。  相似文献   
23.
A narrowband radio interferometer has been developed and used to locate the entire sources of VHF radiations from a negative cloud-to-ground (CG) lightning discharge which contains 19 strokes. This system uses five antennas to form an array consisting of short- and long-baselines along two or- thogonal directions. The system error which comes from frequency conversion is reduced by phase detection through direct high frequency amplifying. An interactive graphic analysis procedure is used to remove the fringe ambiguities which exist inherently in interferometry and to determine the direction of lightning radiation sources in two dimensions (azimuth and elevation) as a function of time at a time resolution of microsecond orders. With the developed system, the whole progression process in time and space of a lightning flash can be reconstructed. In this paper, combining the synchronous data of electric filed change and VHF radiation, the whole processes of an example negative CG flash have been studied in detail. It is found that the preliminary breakdown event of the CG flash started from negative charge region and exhibited firstly a downward pregression and then an upward propagation. There were very intense and continuous radiations during stepped leaders which became much stronger when the first return stroke began. In contrast, there were less and only discrete radiations during dart leaders. Stepped leader and dart leader may transform to each other depending on the state of the ionization of the path. The progression speed of initial stepped leaders was about 105 ms?1, while that was about 4.1×106 and 6.0×106 ms?1 for dart leaders and dart-stepped leaders, respectively. M events produced hook-shaped field changes accompanied by active burst of radiations at their begin- nings. Followed these active radiation processes, M events appeared to contact finally into conducting main discharge channels. The mean progression speed of M events was about 7×107 ms?1, greater than that of the dart leaders and dart-step leaders. K events and attempted leaders were essentially the same as dart leaders except that they could not reach the ground and initiate return strokes.  相似文献   
24.
The analyses of spatial and temporal characteristics of positive cloud-to-ground(CG)lightning for four mesoscaleconvective systems and two severe local convective systems in 1989 and 1990 show that positive CG flash rate usuallyhas two peak values.The major peak occurs during the developing stage of the storm and most of the positive CGflashes originate at the lower part of the storm.The minor occurs during the dissipative stage of the storm and most ofthe positive CG flashes originate at the upper part of the storm,especially in the region of the wind divergence in thestorm anvil.The positive CG flash rate is almost an order of magnitude larger in the developing stage than in thedissipative stage.The appearing time of the peak of negative CG flash rate is in accordance with that of the valley of pos-itive CG flash rate.The higher the intensity of the radar echo,the higher the positive CG flash rate.Most of the positive CG flashes oc-cur when the weak echo area is larger,and mostly originate in the region where the radar echo intensity is about 10dBzand in the back region of the moving storms.The spatial distribution of the positive CG flashes is much more dispersivethan that of the negative.The mesoscale analysis reveals a bipolar lightning pattern.The mean bipole--length reaches itsminimum during the mature stage of the storm and reaches the maximum during the developing stage of the storm.The vertical distribution of the charge density is calculated by a one-dimensional charging model.Then,we discussthe producing condition of the positive CG lightning and forming cause of charge structure mentioned above.  相似文献   
25.
北京与兰州地区的地闪特征   总被引:10,自引:8,他引:10  
郄秀书  郭昌明 《高原气象》1990,9(4):388-394
利用闪电定位系统(LLS)在兰州地区和北京地区探测到的共两万多个地闪资料,对两地的正、负地闪特征进行了对比。分析发现兰州地区的正闪比例是北京地区正闪比例的5倍多。北京地区的正闪平均强度近似为负闪的3倍,而兰州地区的正闪强度只有负闪的2.2倍。无论正闪还是负闪,两地的地闪强度均是稳定的正态分布,并且与雷暴本身的特征无关,从而可用DF强度来作雷暴临近的估计。两地的正、负地闪的回击数均按指数规律下降,不过北京地区的多次回击较兰州地区的多次回击要多。两地的闪电频数都在下午后期出现峰值,但北京地区的闪电频数最大值和最小值都较兰州地区早1小时出现。 通过试验找到了地闪定向仪显示数与闪电辐射电场和放电电流的关系,扩大了地闪定向仪的利用率。  相似文献   
26.
Super Typhoon Haiyan (1330), which occurred in 2013, is the most powerful typhoon during landfall in the meteorological record. In this study, the temporal and spatial distributions of lightning activity of Haiyan were analyzed by using the lightning data from the World Wide Lightning Location Network, typhoon intensity and position data from the China Meteorological Administration, and horizontal wind data from the ECMWF. Three distinct regions were identified in the spatial distribution of daily average lightning density, with the maxima in the inner core and the minima in the inner rainband. The lightning density in the intensifying stage of Haiyan was greater than that in its weakening stage. During the time when the typhoon intensity measured with maximum sustained wind speed was between 32.7 and 41.4 ms?1, the storm had the largest lightning density in the inner core, compared with other intensity stages. In contrast to earlier typhoon studies, the eyewall lightning burst out three times. The first two eyewall lightning outbreaks occurred during the period of rapid intensification and before the maximum intensity of the storm, suggesting that the eyewall lightning activity could be used to identify the change in tropical cyclone intensity. The flashes frequently occurred in the inner core, and in the outer rainbands with the black body temperature below 220 K. Combined with the ECMWF wind data, the influences of vertical wind shear (VWS) on the azimuthal distribution of flashes were also analyzed, showing that strong VWS produced downshear left asymmetry of lightning activity in the inner core and downshear right asymmetry in the rainbands.  相似文献   
27.
北京闪电综合探测网(BLNET):网络构成与初步定位结果   总被引:6,自引:5,他引:1  
北京闪电综合探测网(Beijing Lightning NETwork, 简称BLNET)由10个观测站组成, 每个子站主要由闪电快、慢电场变化测量仪(也称快、慢天线)和闪电甚高频(VHF)辐射探测仪构成, 实现了对闪电的多频段的综合观测。本文首先详细介绍了BLNET的网络构成, 然后利用蒙特卡罗法对网络的定位误差进行了理论分析, 模拟结果表明网络内部水平定位误差小于200 m, 网络外部100 km处水平定位误差小于3 km, 最后利用Chan氏算法和Levenberg-Marquardt算法相结合的方法, 对发生在2013年7月7日的一次雷暴过程分别进行了地闪和云闪定位, 将定位结果和对应时次的雷达回波进行比较, 发现地闪和云闪都出现在大于30 dBZ的雷达回波区, 表明了探测网络和定位方法的可靠性。  相似文献   
28.
张廷龙  郄秀书  袁铁 《大气科学》2008,32(5):1221-1228
利用2002年夏季在青海省大通县进行的雷暴及闪电综合观测实验中所获取的6站GPS同步闪电电场变化资料,对8月4日一次下部具有大范围正电荷区的典型性雷暴过程的雷电特征进行详细研究。利用点电荷模式对16次负地闪和2次正地闪所包含的共65次回击所中和电荷源进行的非线性最小二乘法拟合研究发现,负地闪所中和的负电荷距离地面的相对高度在3~5 km,而两次正地闪所中和的雷暴云电荷在5~6 km的高度,表明该雷暴云呈三极性电荷结构。负地闪单次回击所中和电荷量平均为1.48 C,而两次正地闪都为单次回击且中和的电荷量分别为1.37 C和2.68 C。  相似文献   
29.
In the summer of 2005, one negative lightning flash was artificially triggered in Shandong Province (117°48′ E, 37°42′N), middle latitude region of eastern China. The flash included 10 return strokes, and the geometric mean value of the current peak was 11.9 kA (the average value was 12.6 kA) with a maximum of 21.0 kA and a minimum of 6.6 kA, similar to the subsequent return strokes in natural lightning. The geometric mean value of half peak width was 39 μs (the average value was 40 μs), which was much larger than the usual result. Based on the Diendorfer and Uman (DU) model, the return-stroke current waveforms and charge distribution along the lightning channel are discussed. The simulated current waveforms, being divided into breakdown and corona current components, are in agreement with the optical measurements when the two different discharge time constants are properly chosen.  相似文献   
30.
Lightning and Doppler radar observations of a squall line system   总被引:2,自引:0,他引:2  
A typical squall line with damaging wind and hailstones occurred on 28 April 2006 in Shandong Province, middle eastern China, and caused great economic loss. The characteristics of cloud-to-ground lightning (CG) in the squall line were studied in detail by combining the data from the ground-based CG location network, two Doppler radars and the Lightning Imaging Sensor on the TRMM satellite. Results show that positive CG flashes accounted for 54.7% of the total CG flashes. During the initial developing stage, the CG flash rate was lower than 0.5fl min− 1 and most of the CG flashes were positive. It increased significantly, up to 4.5fl min− 1, along with the rapid development of the squall line, and the percentage of positive CG was more than 75% during this period. The CG flash rate began to decrease but the percentage of negative CG flash increased gradually and exceeded that of positive CG during the mature and dissipating stages. Positive CG flashes tended to occur on the right flank and negative ones on the left flank. Strong wind at the surface occurred in or near the regions with dense positive CG flashes. Almost all positive CG flashes occurred near the strong radar echo regions, in the front parts of the squall line. However, the negative CG flashes almost exclusively occurred in the regions with weak and uniform radar echoes. The total flash rate in the storm was very high, up to 136fl min− 1, and its ratio of intracloud flashes (IC) to CG flashes was 35:1. Dense positive CG flashes corresponded to updraft regions, they did not occur in the core of the updraft, but just behind and close to the main updraft instead. The rear inflow jet, between 3 and 6 km, played an important role in the formation of the bow echo and very strong wind at surface. The CG distribution features in the squall line were obviously different from that of an ordinary MCS. The charge structure could be roughly described as an inverted charge structure.  相似文献   
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