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951.
李萍  李同录  王红  梁燕 《岩土力学》2013,34(Z2):184-189
我国黄土厚度大,黄土地区地下水位深,降雨量少,黄土多处于非饱和状态,土-水特征曲线是非饱和黄土应力状态、强度及渗透性研究的基础。以陇东高原马兰黄土为试验对象,采用张力计法测定原状土样的土-水特征曲线,采用三种理论模型对试验数据拟合,其中Gardner模型简单、参数少,但Fredlund & Xing模型拟合效果最好。基于已测得的土-水特征曲线,采用Childs & Collis-Geroge预测非饱和渗透系数的模型,计算得到非饱和黄土渗透系数与基质吸力或含水率的关系,发现黄土从饱和到非饱和,其渗透系数急剧降低,黄土非饱和渗透系数与基质吸力或体积含水率的关系均可用指数函数表示。本文对典型黄土土-水特征曲线的研究及渗透性的预测为黄土工程问题,如降雨入渗的边坡稳定性评价、非饱和地基湿陷变形计算等提供理论基础。  相似文献   
952.
以van Genuchten模型表述的土壤水分特征曲线为基础,推导出流域单点缺水量,并结合TOPMODEL模型中地形指数与地下水位关系,建立了反映地形和土壤特征共同影响的蓄水容量模型,通过统计方法从栅格尺度蓄水容量获得流域尺度蓄水容量曲线,取代传统新安江模型中率定的蓄水容量曲线。以淮河流域紫罗山子流域为例,分析地形特征与土壤类型对蓄水容量的影响;并与实测流量过程以及原新安江模型模拟的流量过程对比,表明模型能较好地模拟场次洪水过程。模型将蓄水容量曲线显式表述,减少了新安江模型参数,为无资料地区的水文模拟提供了分析方法。  相似文献   
953.
基于Laio土壤水分动态随机模型(Laio模型),利用2006-2010年5~9月土壤水分连续监测数据及日降水资料,分析科尔沁沙地固定沙丘和沙质草地生长季根系层土壤水分动态及其与降水格局的关系,研究点尺度土壤水分概率密度函数,并对Laio模型涉及的13个参数进行了敏感性分析。结果表明:① 研究区年降水的季节分配极不均匀,主要集中在4~10月的生长季,占全年降水量的93%;0~5 mm降水事件占全年降水事件的73%,但其降水量只占全年降水量的25%;降水间隔期以0~10 d为主,占全年无降水期的38%,其频数最高,占全年间隔期频数的87%。② 固定沙丘和沙质草地根系层厚度分别为0~100 cm和0~70 cm,沙质草地根系层土壤水分显著高于固定沙丘;两类沙地7月份的土壤水分都显著高于生长季其他月份。③ 两类沙地生长季根系层土壤水分均服从正态分布;通过Laio模型得到了两类沙地生长季根系层土壤水分概率密度函数p(s),其峰值及峰值出现的位置和峰的阔度均与观测结果很接近,说明Laio模型能对科尔沁沙地土壤水分概率密度函数进行较好的模拟。④ Laio模型涉及的13个参数中,对p(s)最为敏感的参数是降水频率λ、平均降水量α、最大蒸散量Emax、水分胁迫点s*和凋萎系数sw,主要影响p(s)曲线的峰值。  相似文献   
954.
物理海洋观测研究的进展与挑战   总被引:1,自引:0,他引:1  
从当今物理海洋所面临的若干前沿科学问题出发,重点探讨了物理海洋观测研究所面临的任务与挑战,包括大洋边界流系统、海洋湍流及跨等密度面混合以及海洋热含量和淡水平衡等.在已有的基础上,对我国在深海研究领域特别是物理海洋观测方面提出了几点针对性的建议.  相似文献   
955.
烷基酚是一类由酚类化合物烷基化后产生的化合物,与其他非烃化合物相比,更易溶于水.文章通过不同温度(25℃、45℃和65℃)、 不同盐水浓度(4000 mg/L、6000 mg/L和8000 mg/L)和不同原油类型(X37、X45和X61)的三组油水分配实验,研究了烷基酚在油水两相间的分配特征,确定了烷基酚分配系数的变...  相似文献   
956.
土壤水分是全球水循环的重要组成成分,对研究水分的空间分布、农作物长势和产量、气候变化、水资源时空特征等有着重要意义.利用Sentinel(哨兵)系列主动微波雷达卫星SAR(Sentinel-1)结合光学卫星(Sentinel-2)对格尔木中下游低矮植被覆盖下的地表土壤水分进行反演研究,探讨不同极化组合方式和水云模型前后...  相似文献   
957.
选择黄土丘陵沟壑区的羊圈沟流域,应用地理信息系统和野外采样技术,从小流域,坡面和单一土地利用类型三个尺度层次研究土地利用变化对流域土壤侵蚀,土壤养分和土壤水分的影响。结果发现:1996年比1984年该流域坡耕地减少43%,林地增加了42%,草地增加了5%,土壤侵蚀量减少了24%。  相似文献   
958.
The present observational status of the Sct stars, Dor stars and roAp stars is discussed. The Sct stars are the most intensively observed of the three groups, but it has become clear that there are severe problems in extracting asteroseismic information from them. Dozens of frequencies are observed, but hundreds of frequencies are predicted from the models; unique matches of observation and theory still elude us. The Sct stars are observationally complex – some recent `best case' campaigns are discussed. It is possible that substantial observational advances for Sct stars may need to await upcoming satellite missions. New Dor stars are beingdiscovered frequently, and new behaviour is being found for them. They constitutean observationally young field. Their pulsational frequency range is being expanded, their position in the HR diagram is becoming better known (but is yet to be fully constrained), and the possibility exists of hybrid Dor – Sct stars that have greatasteroseismic promise, although it is clear such stars are rare, if they do exist. It has been observationally challenging to extract more than a fewfrequencies for any Dor star so far. Exciting spectroscopic discoveries of new behaviour in roAp stars promise unprecedented information about the structure of the peculiar atmospheres ofthose stars – pulsation amplitude and phase in 3D, magnetic field structurein 3D, abundance stratification in 3D, realistic T- for the most peculiarstars – as well as entirely new information about the interaction of pulsation,rotation and magnetic fields. Recent theoretical work has led to new understandingof the previously inexplicable frequency spacing of HR 1217 with new Whole Earth Telescope observations supporting this theory. An `improved oblique pulsator model' has been developed in which the pulsationaxis is not the magnetic axis; this model has passed several observationaltests and new ones are being devised to examine it further.  相似文献   
959.
Better knowledge regarding internal soil moisture and piezometric responses in the process of rainfall-induced shallow slope failures is the key to an effective prediction of the landslide and/or debris flow initiation. To this end, internal soil moisture and piezometric response of 0.7-m-deep, 1.5-m-wide, 1.7-m-high, and 3.94-m-long semi-infinite sandy slopes rested on a bi-linear impermeable bedrock were explored using a chute test facility with artificial rainfall applications. The internal response time defined by the inflection point of the soil moisture and piezometric response curves obtained along the soil–bedrock interface were closely related to some critical failure states, such as the slope toe failure and extensive slope failures. It was also found that the response times obtained at the point of abrupt bedrock slope decrease can be used as indicators for the initiation of rainfall-induced shallow slope failures. An investigation of spatial distributions of soil water content, ω (or degrees of saturation, Sr), in the slope at critical failure states shows that the 0.2 m – below – surface zone remains unsaturated with Sr 40–60%, regardless of their distances from the toe and the rainfall intensity. Non-uniform distributions of ω (or Sr) along the soil–bedrock interface at critical failure states were always associated with near-saturation states (Sr 80–100%) around the point of bedrock slope change or around the transient ‘toe’ upstream of the slumped mass induced by the retrogressive failure of the slope. These observations suggest the important role of the interflow along the soil–bedrock interface and the high soil water content (or high porewater pressure) around the point of bedrock slope deflection in the rainfall-induced failure of sandy slopes consisting of shallow impermeable bedrocks. The present study proposes an ‘internal response time’ criterion to substantiate the prediction of rainfall-induced shallow slope failures. It is believed that the ‘internal response time’ reflects the overall characteristics of a slope under rainfall infiltration and can be as useful as the conventional meteorology-based threshold times. The ‘internal response time’ theory can be generalized via numerical modeling of slope hydrology, slope geology and slope stability in the future.  相似文献   
960.
Retrieval of the terrestrial moisture storage dataset from the Gravity Recovery and Climate Experiment (GRACE) satellite remote sensing system is possible when the catchment of interest is of large spatial scale. These dataset are of paramount importance for the estimation of the total storage deficit index (TSDI), which enables the characterization of a particular drought event from the perspective of the terrestrial moisture storage over that catchment. Incidentally, the GRACE gravity signal over the 13,000 km2 Upper Assiniboine River Basin on the drought-prone Canadian Prairie is so poor therefore making the computation of the total storage deficit index for this basin infeasible. Consequently, the estimation of the terrestrial moisture storage from other reliable sources becomes imperative in order to enable the computation of the TSDI over this basin.This study explores the utilization of the Variable Infiltration Capacity (VIC) model, a physically based, spatially distributed hydrologic model to simulate the total moisture storage over the Upper Assiniboine River Basin which was then employed in the estimation of the TSDI over this basin for subsequent characterization of the recent Prairie-wide drought. Interestingly, the temporal patterns in the computed TSDI from the VIC model reveal a strong resemblance with the same drought characterization undertaken over the larger adjacent Saskatchewan River Basin, which was accomplished utilizing terrestrial moisture storage from the GRACE-based approach. Additionally, these independent techniques employed in the characterization of the last Prairie drought over the two adjacently situated basins resulted in similar drought severity classification from the standpoint of the total moisture storage deficits over these basins. This study has therefore shown that in the computation of the total storage deficit index over small-scale catchments during anomalous climatic conditions that propagate extreme dryness through the terrestrial hydrologic systems, simulations of the total water storage from a structurally sound model such as the VIC model could be resourceful for the computation of the monthly total storage deficit index if no constraint is placed on the availability of accurate meteorological forcing.  相似文献   
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