全文获取类型
收费全文 | 3835篇 |
免费 | 945篇 |
国内免费 | 441篇 |
专业分类
测绘学 | 1134篇 |
大气科学 | 53篇 |
地球物理 | 619篇 |
地质学 | 2350篇 |
海洋学 | 489篇 |
天文学 | 66篇 |
综合类 | 334篇 |
自然地理 | 176篇 |
出版年
2024年 | 5篇 |
2023年 | 53篇 |
2022年 | 188篇 |
2021年 | 286篇 |
2020年 | 239篇 |
2019年 | 204篇 |
2018年 | 104篇 |
2017年 | 168篇 |
2016年 | 149篇 |
2015年 | 185篇 |
2014年 | 331篇 |
2013年 | 220篇 |
2012年 | 285篇 |
2011年 | 275篇 |
2010年 | 196篇 |
2009年 | 201篇 |
2008年 | 224篇 |
2007年 | 262篇 |
2006年 | 233篇 |
2005年 | 173篇 |
2004年 | 180篇 |
2003年 | 168篇 |
2002年 | 134篇 |
2001年 | 94篇 |
2000年 | 94篇 |
1999年 | 90篇 |
1998年 | 75篇 |
1997年 | 79篇 |
1996年 | 79篇 |
1995年 | 64篇 |
1994年 | 38篇 |
1993年 | 29篇 |
1992年 | 25篇 |
1991年 | 16篇 |
1990年 | 18篇 |
1989年 | 17篇 |
1988年 | 8篇 |
1987年 | 9篇 |
1986年 | 7篇 |
1985年 | 3篇 |
1984年 | 4篇 |
1983年 | 2篇 |
1982年 | 2篇 |
1980年 | 1篇 |
1978年 | 3篇 |
1954年 | 1篇 |
排序方式: 共有5221条查询结果,搜索用时 500 毫秒
51.
中国数字地质调查系统的基本构架
及其核心技术的实现 总被引:6,自引:0,他引:6
数字地质调查系统是贯穿整个地质矿产资源调查全过程的软件,涵盖地质矿产调查、矿产资源勘查、矿体模拟、品住估计、资源量估算、矿山开采系统优化等内容。考虑数字地质调查系统的应用技术层面,从数据“层”模型、数据流“池”技术、不同阶段数据模型继承技术、数据互操作技术等几个方面讨论了核心技术及其实现,通过基于无缝一体化技术的数据采集、管理、综合处理与成果表达,在实体或矿块的矿床建模技术与品住估计、储量估算等方面展现了全地质调查过程的数字化,不但为地质人员应用高新技术降低了门坎,而且极大地提高了研究精度和效率,丰富了成果的表现形式和服务形式。随着数字地质调查系统的完善和应用水平的提高,数字地质调查系统将成为中国地质调查的主流软件体系。 相似文献
52.
传统的三角高程水准测量由于受地形起伏的限制,外业工作量大,施测精度和工作效率不高。本文采用全站仪对传统的三角高程水准测量方法进行了改进,并论述了全站仪三角高程测量方法的原理和实际作业方法。 相似文献
53.
D. Rouan N. Epchtein M. De Muizon F. Lacombe P. Puget D. Tiphene F. Boulanger X. Desert G. Guyot L. D'Hendecourt J -M. Lamarre A. Leger F. Pajot J -L. Puget E. Caux M. Giard G. Serra C. Cesarsky L. Vigroux A. Omont 《Astrophysics and Space Science》1994,217(1-2):41-44
Proposed to both the French and the European Space Agency as one possible small mission, SPICE is a project for a dedicated small satellite for a near-IR spectroscopic all-sky survey. The instrument would cover the spectral range 1.8 - 3.6µm, possibly extended to 1.8 - 7µm, at a resolution of 100, with pixels of 1 arc-min. The excellent sensitivity (0.02 MJy sr-1) results from: i) the quasi-zero level of background due to the efficient passive cooling of the whole experiment; ii) the use of large format arrays; iii) the non-stop observing mode (drift-scanning). The spectral domain, complementing the one of ISO, partially opaque from the ground, is specially rich in spectral features tracing stars and all components of the Interstellar Medium (molecular, atomic and ionized gas, dust). With a cooling below 80 K of the focal instrument, then it becomes possible to consider doubling the spectral domain and to cover the whole 1.8 - 7µm range. 相似文献
54.
丰台—野鸡坨断裂为唐山地区主要断裂之一,西侧为鸦鸿桥凹陷,东侧为唐山凸起,断裂两侧第四系厚度之差巨大。本文依据该断层两侧钻孔对其第四纪以来活动性进行初步的探讨。通过对丰台—野鸡坨断裂上下两盘PZK14和PZK20孔磁性地层学研究,并结合钻孔岩石地层,及浅部光释光和14C测年结果,建立第四纪地层格架。结果表明:两孔底部“泥包砾”为新近纪沉积;PZK14孔下更新统底界埋深为387 m,中更新统底界埋深为114 m,上更新统底界埋深为71 m,全新统底界埋深为6 m;PZK20孔下更新统底界埋深为155 m,中更新统底界埋深为73 m,上更新统底界为36 m,无全新世地层。丰台—野鸡坨断裂活动在早更新世时表现为逐渐增强的特点,活动速率由早期的5.4 cm/ka增加到13.9 cm/ka。中更新世断裂活动基本处于停滞状态,活动速率为1.0 cm/ka。晚更新世以后,断裂重新活动,且更加剧烈,活动速率达到了54.5 cm/ka。 相似文献
55.
雄安新区内地热资源丰富,区内有牛驼镇地热田、容城地热田和高阳地热田,地热资源开发利用较早,但是对其深部热源机制仍未形成统一观点。为了研究雄安新区内地热田深部热源机制,在新区及外围进行了深反射地震和长周期大地电磁探测,对取得的同剖面的深反射地震和大地电磁数据进行处理和综合解释,探明了研究区从地表至莫霍面范围内地质构造和电性结构。下地壳结构在深反射地震剖面与大地电磁剖面上有很好的对应关系。电阻率低值区对应着在深反射地震剖面上存在一系列反射同相轴,且同相轴可以延续到莫霍面,电阻率高值区对应着在深反射地震剖面上无明显连续反射同相轴,尤其是在莫霍面之上呈现地震反射近似"空白区"。结合区域地热资料构建了研究区深部地热地质模型,对新区内深部地热机制进行了解释。该模型为"二元"生热模型,其热源包含两个部分,深部地幔热源和地壳放射性元素衰变生热。放射性元素衰变生热占地表热流的接近30%,而幔源热流在地表热流中的占比可达约70%。在牛驼镇下方,莫霍面以上,由于地幔热物质上涌造成下地壳上隆,幔源岩浆底侵作用于下地壳形成了局部热异常,该热异常具有低速高导的地球物理特征,认为是牛驼镇地热田和容城地热田的深部热源;以区域断裂为热通道,大地热流由深部向上传导、扩散到牛驼镇凸起和容城凸起顶部,对碳酸盐岩储水层进行加热,形成地热储层;上覆新近系沉积地层是良好的热盖层。 相似文献
56.
57.
58.
The feasibility of using the more sophisticated weighted least-squares (WLS) model, as opposed to the traditional ordinary least-squares (OLS), in linear regressions of BHT data to estimate the static formation temperatures (SFT) was investigated. The most commonly used analytical methods (line-source; spherical and radial heat flow; and cylindrical heat source) were applied. Error propagation equations were derived to calculate errors in the time function of each method. These errors were combined with the BHT measurement errors to compute weighting factors for applying the WLS. Intercept uncertainties were estimated for all regressions using sets of synthetic and actual borehole logs taken from geothermal and oil applications. SFT computed with the spherical and radial heat flow method were generally greater than those from the other two methods. 相似文献
59.
The distribution of radiogenic heat production as a function of depth in the Sierra Nevada Batholith, California 总被引:4,自引:0,他引:4
Geochemical analyses and geobarometric determinations have been combined to create a depth vs. radiogenic heat production database for the Sierra Nevada batholith, California. This database shows that mean heat production values first increase, then decrease, with increasing depth. Heat production is 2 μW/m3 within the 3-km-thick volcanic pile at the top of the batholith, below which it increases to an average value of 3.5 μW/m3 at 5.5 km depth, then decreases to 0.5–1 μW/m3 at 15 km depth and remains at these values through the entire crust below 15 km. Below the crust, from depths of 40–125 km, the batholith's root and mantle wedge that coevolved beneath the batholith appears to have an average radiogenic heat production rate of 0.14 μW/m3. This is higher than the rates from most published xenolith studies, but reasonable given the presence of crustal components in the arc root assemblages. The pattern of radiogenic heat production interpreted from the depth vs. heat production database is not consistent with the downward-decreasing exponential distribution predicted from modeling of surface heat flow data. The interpreted distribution predicts a reasonable range of geothermal gradients and shows that essentially all of the present day surface heat flow from the Sierra Nevada could be generated within the 35 km thick crust. This requires a very low heat flux from the mantle, which is consistent with a model of cessation of Sierran magmatism during Laramide flat-slab subduction, followed by conductive cooling of the upper mantle for 70 m.y. The heat production variation with depth is principally due to large variations in uranium and thorium concentration; potassium is less variable in concentration within the Sierran crust, and produces relatively little of the heat in high heat production rocks. Because silica content is relatively constant through the upper 30 km of the Sierran batholith, while U, Th, and K concentrations are highly variable, radiogenic heat production does not vary directly with silica content. 相似文献
60.
Study of geothermal water intrusion due to groundwater exploitation in the Puebla Valley aquifer system, Mexico 总被引:1,自引:1,他引:1
E. Leticia Flores-Márquez Gabriel Jiménez-Suárez Raymundo G. Martínez-Serrano René E. Chávez Daniel Silva Pérez 《Hydrogeology Journal》2006,14(7):1216-1230
Significant intrusion of geothermal water into fresh groundwater takes place in the Puebla Valley aquifer system, Mexico. The decline in the potentiometric surface due to the overexploitation of the groundwater induces this intrusion. This hydrological system comprises three aquifers located in Plio-Quaternary volcanic sediments and Mesozoic calcareous rocks. The hydraulic balance of the aquifer shows that the annual output exceeds the natural inputs by 12 million m3. Between 1973 and 2002, a drop in the potentiometric surface, with an 80 m cone of depression, was identified in a 5-km-wide area located southwest of the city of Puebla. Chemical analyses performed on water samples since 1990 have shown an increase in total dissolved solids (TDS) of more than 500 mg/L, coinciding with the region showing a cone of depression in the potentiometric surface. A three-dimensional flow and transport model, based on the hydrogeological and geophysical studies, was computed by using the MODFLOW and MT3D software. This model reproduces the evolution of the aquifer system during the last 30 years and predicts for 2010 an additional drawdown in the potentiometric surface of 15 m, and an increase in the geothermal water intrusion. 相似文献