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11.
土地利用变化对喀纳斯自然保护区生态系统服务价值的影响 总被引:2,自引:0,他引:2
应用喀纳斯自然保护区1980,2005年两个时期的LandsatTM影像解译数据,采用Costanza生态系统服务价值计算公式,参照中国单位面积生态服务价值系统,确定了喀纳斯自然保护区生态系统单位面积生态服务价值系数,分析了保护区土地利用变化对其生态系统服务价值的影响.结果表明,保护区林地面积在减少,草地,水域、建设用地面积有所增加;研究期内生态系统服务价值从26.79亿元减少到26.02亿元,天然有林地和高覆盖度草地的减少是生态服务价值降低的主要原因;保持土壤、维持生物多样性、气候调节等各单项功能服务价值均呈现不同程度的减少,说明保护区生态环境不断趋向恶化. 相似文献
12.
Plagioclase zoning as an indicator of magma processes at Bezymianny Volcano,Kamchatka 总被引:6,自引:1,他引:5
Vasily D. Shcherbakov Pavel Yu. Plechov Pavel E. Izbekov Jill S. Shipman 《Contributions to Mineralogy and Petrology》2011,162(1):83-99
Back-scattered electron (BSE)-derived zoning patterns of plagioclase phenocrysts are used to identify magma processes at Bezymianny
Volcano, Kamchatka, based on the 2000–2007 sequence of eruptive products. The erupted magmas are two-pyroxene andesites, which
last equilibrated at ~915°C temperature, 77–87 MPa pressure, and a water content of ~1.4 wt%. Textural and compositional zoning
of individual plagioclase phenocrysts typically includes a repeated core-to-rim sequence of oscillatory zoning (An50–60) truncated by a dissolution surface followed by an abrupt increase in An content (up to An85), which then gradually decreases rimward. This zoning pattern is interpreted to be the result of frequent replenishments
of the magma chamber which cause both thermal and chemical interaction between resident and recharge magmas. The outermost
70- to 150-μm-wide zoning patterns of plagioclase phenocrysts are composed of dissolution surface with a subsequent increase
in An and Fe contents. Zoning patterns of the rims exhibit correlation among plagioclase phenocrysts within one eruption.
Rims are interpreted as a result of crystallization of a batch of magma in the conduit after recharge event. 相似文献
13.
综合利用卡姆斯特煤田钻孔测井、野外露头及古生物化石等资料,应用经典层序地层学基本理论和方法,对卡姆斯特煤田八道湾组进行了层序地层划分,共识别出SQ1和SQ2两个三级层序,并根据地层叠置样式、沉积旋回特征细分为6个体系域。通过沉积基础图件、沉积环境的分析明确了研究区八道湾组沉积演化主要受古地形起伏、古气候条件等古地理因素的综合影响。确定研究区内目的层段主要在高位和低位时期聚煤,湖侵时期不利于聚煤。通过详细研究卡姆斯特煤田八道湾组的沉积环境和聚煤特征,为今后寻找和开发卡姆斯特地区煤炭资源提供地质依据。 相似文献
14.
On the accuracy of the bathymetry-generated gravitational field quantities for a depth-dependent seawater density distribution 总被引:1,自引:0,他引:1
In geophysical studies investigating the lithosphere structure, the gravitational field generated by the ocean density contrast
(i.e., bathymetry-generated gravitational field) represents a significant amount of the signal to be modelled and subsequently
removed from the Earth’s gravity field. The ocean density contrast is typically calculated as the difference between the mean
density values of the Earth’s crust and seawater. The approximation of the actual seawater density distribution by its mean
value yields relative errors up to about 2% in computed quantities of the gravitational field. To reduce these errors, a more
realistic model of the seawater density distribution is utilized based on the analysis of existing oceanographic data of salinity,
temperature, and pressure (depth). We study the accuracy of the bathymetry-generated gravitational field quantities formulated
for a depth-dependent model of the seawater density distribution. This density distribution approximates the seawater density
variations due to an increasing pressure with depth, whereas smaller lateral density variations caused by salinity, temperature,
and other oceanographic factors are not taken into consideration. The error analysis reveals that the approximation of the
seawater density by the depth-dependent density model reduces the maximum errors to less than 0.6%. The corresponding depth-averaged
errors are below 0.1%. The depth-dependent seawater density model is further facilitated in expressions for computing the
bathymetry-generated gravitational field quantities by means of the spherical bathymetric (ocean bottom depth) functions.
The numerical realization reveals large differences in the results obtained with and without consideration of the depth-dependent
seawater density distribution. The maxima of absolute differences reach 201 m2/s2 and 16.5 mGal in computed values of the potential and attraction, respectively. The application of the depth-dependent seawater
density model thus significantly improves the accuracy in the forward modelling of the bathymetric gravitational field quantities. 相似文献
15.
通过对克孜尔水库跨断层形变特征进行分析,结果显示:①垂直形变每年3~4月、10~11月分别为峰、谷值时间;水平形变每年6~7月、1月分别为峰、谷值时间.②垂直变形的峰-谷时间间隔在1997年之前多为5~8个月,1998年后多为1~3个月;谷-峰值时间间隔在1997年前多为4~7个月,1998年后多在8~11个月.水平形... 相似文献
16.
基于博斯腾湖1955—2012年湖水位变化资料,利用树木年轮法分析了博斯腾湖年和月水位变化与湖滨柽柳(Tamarix ramosissina)年轮生长关系,利用敏感度指数得出博斯腾湖滨柽柳年轮生长的敏感水位范围。结果表明:(1)1955—2012年博斯腾湖年平均水位经历了3个明显变化阶段,即1955—1987年下降至最低,1987—2002年上升至最高。受向下游生态输水影响,2002—2012年博斯腾湖水位快速下降。输水对博斯腾湖月平均水位和季节性水位变化有影响。(2)博斯腾湖滨柽柳年轮指数与当年的湖水位变化和前1年的湖水位变化均显著相关(p0.05)。柽柳年轮指数与前1年10月至当年4月各个月份的湖水位表现出显著相关(p0.05)。柽柳年轮指数与前1年冬季湖水位相关显著(p0.05),与当年春季3—4月月平均湖水位相关性显著,与当年夏季和秋季湖水位的相关性不显著。(3)博斯腾湖滨柽柳年轮生长对月湖水位变化响应比较敏感。当湖水位在1045.3m时,柽柳年轮指数灵敏度指数(Sk)存在最低值;当湖水位在1 046.3m时,Sk出现最高值。 相似文献
17.
18.
钻井液的类型与性能对于提高极地冰层取心钻进的效率与保证钻孔稳定性具有重要的影响。在分析铠装电动机械钻具工作原理与钻井液循环方式的基础上,较为详细地分析了升降钻具的速度与钻井液粘度与密度之间的关系;分析了现有钻井液类型和所存在的问题;以二元脂肪酸二醇酯、低分子量饱和脂肪酸酯与甲基硅油的试验测试数据为基础,确定了可用于极地冰层取心钻进的钻井液类型及其性能要求。 相似文献
19.
20.
High entry speed (>25 km s?1) and low density (<2500 kg m?3) are the two factors that lower the chance of a meteoroid to drop meteorites. The 26 g carbonaceous (CM2) meteorite Maribo recovered in Denmark in 2009 was delivered by a bright bolide observed by several instruments across northern and central Europe. By reanalyzing the available data, we confirmed the previously reported high entry speed of (28.3 ± 0.3) km s?1 and trajectory with slope of 31° to the horizontal. In order to understand how such a fragile material survived, we applied three different models of meteoroid atmospheric fragmentation to the detailed bolide light curve obtained by radiometers located in Czech Republic. The Maribo meteoroid was found to be quite inhomogeneous with different parts fragmenting at different dynamic pressures. While 30–40% of the (2000 ± 1000) kg entry mass was destroyed already at 0.02 MPa, another 25–40%, according to different models, survived without fragmentation up to the relatively large dynamic pressures of 3–5 MPa. These pressures are only slightly lower than the measured tensile strengths of hydrated carbonaceous chondrite (CC) meteorites and are comparable with usual atmospheric fragmentation pressures of ordinary chondritic (OC) meteoroids. While internal cracks weaken OC meteoroids in comparison with meteorites, this effect seems to be absent in CC, enabling meteorite delivery even at high speeds, though in the form of only small fragments. 相似文献