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71.
陶器资源——江西红土岩开发 总被引:4,自引:0,他引:4
依据江西红土岩物质组成特征及与宜兴紫砂土的相似性,对江西红土岩进行了较系统的陶器实验与研究。江西红土岩系的化学成分、矿物成分及工艺特征适合陶器要求。按其分布规律和物质组成特征可分成两类:酸性红土岩和碱性红土岩。在详细分析两类岩系工艺性质的基础上,对江西红土岩这一陶器资源进行了产品开发。 相似文献
72.
青藏高原东北部古喀斯特过程与环境 总被引:6,自引:0,他引:6
本文介绍了青藏高原东北部地区的古喀斯特现象,并对相关沉积进行了化学成、粘土矿物的X-射线衍射以及石英砂表面结构等气候代用指标的分析。分析结果一致,指示了温暖湿润的亚热带气候条件。重结晶方解石的裂变径迹测年结果表明,该地区古喀斯特发育于中中新世。 相似文献
73.
红层(盆)内外存在着工业金矿化现象,与红层(盆)有关的金矿化包括:次火山岩型、卡林型、穆龙套型、不整合脉型、风化壳型、热泉型以及砂金等众多类型。它们的形成过程及分布与红层(盆)关系密切。本文总结了与红层(盆)有关金矿化的成矿模式及找矿方向。 相似文献
74.
I. M. Korrat H. M. Hussein I. Marzouk E. M. Ibrahim R. Abdel-Fattah N. Hurukawa 《Acta Geophysica》2006,54(1):33-49
Seismicity in the northernmost part of the Red Sea has been studied using data from Hurghada Seismological Network in addition
to readings from the existing neighbouring networks. Relocated events in addition to data from national centers are used to
obtain a complete and true picture for the seismicity of the area. The spatial distribution of earthquakes defines three earthquake
zones in the Gulf of Aqaba and three zones at the entrance of the Gulf of Suez and southern tip of Sinai Peninsula. The thermal
activity and the triple junction nature control the activity in this area. The activity defines also an active trend extending
from the southern tip of Sinai Peninsula to the median zone of the Red Sea. The seismicity of this trend is probably related
to the active spreading zone associated with the opening of the Red Sea. The b-values are derived for the entrance areas of the two gulfs and for Gulf of Aqaba. Values of b are 1.35 for the triple junction region, 1.13 for the activity before the 22 November 1995 Gulf of Aqaba mainshock and 1.25
for the aftershocks of this event. 相似文献
75.
介绍了几内亚体育场岩土层结构和粘土的工程地质特征,将其与国内红粘土进行了比较,认为是属于基性岩风化而形成的红粘土,并探讨了该红粘土的形成过程。从元素迁移规律着手,分析了形成该地剖面上特殊的岩土层序的形成原因,从化学成份和分子结构着手分析了该粘土物理力学性质的形成原因。进而分析了几内亚红粘土工程地质评价中应注意的问题。 相似文献
76.
Geological analysis and FT dating of the large-scale right-lateral strike-slip movement of the Red River fault zone 总被引:1,自引:1,他引:1
XIANG HongFa WAN JingLin HAN ZhuJun GUO ShunMin ZHANG WanXia CHEN LiChun & DONG XingQuan Institute of Geology China Earthquake Administration Beijing China Earthquake Administration of Yunnan Province Kunming China 《中国科学D辑(英文版)》2007,50(3):331-342
Tectonically, the large-scale right-lateral strike-slip movement along the Red River fault zone is char-acterized at its late phase with the southeastward extension and deformation of the Northwestern Yunnan normal fault depression on its northern segment, and the dextral shear displacement on its central-southern segment. Research of the relations between stratum deformation and fault movement on the typical fault segments, such as Jianchuan, southeast Midu, Yuanjiang River, Yuanyang, etc. since the Miocene Epoch shows that there are two times dextral faulting dominated by normal shearing occurring along the Red River fault zone since the Miocene Epoch. The fission track dating (abbrevi-ated to FT dating, the same below) is conducted on apatite samples collected from the above fault segments and relating to these movements. Based on the measured single grain’s age and the con-fined track length, we choose the Laslet annealing model to retrieve the thermal history of the samples, and the results show that the fault zone experienced two times obvious shear displacement, one in 5.5 ± 1.5 MaBP and the other in 2.1± 0.8 MaBP. The central-southern segment sees two intensive uplifts of mountain mass in the Yuanjiang River-Yuanyang region at 3.6―3.8 MaBP and 1.6―2.3 MaBP, which correspond to the above-mentioned two dextral normal displacement events since the late Miocene Epoch. 相似文献
77.
门源盆地位于青藏高原东北缘北祁连山腹地,为狭长的新生代走滑拉分山间宽谷盆地。其中充填一厚约407~960 m、干旱气候条件下的河湖相沉积"红层",长期以来各项研究工作均未能于其中采获任何生物化石。因此,尽管各家均认同其属"第三纪"无疑,但仍对其确切时代存在着较大的争论,而对其时代的确定有助于正确认识门源盆地形成时的构造背景,具有较为重要的意义。通过区域地层对比、"红层"形成气候条件与南侧西宁盆地及北邻酒泉—张掖盆地古气候环境所作的对比,深入探讨认为其时代属中中新世,并初步分析了门源盆地形成的新构造运动大陆动力学机制背景。 相似文献
78.
We present the first diffraction-limited K-band image of the Red Rectangle with 76 mas resolution, an H-band image with 75 mas resolution, and an RG 715 filter image ( 800 nm wavelength) with 78 mas resolution (corresponding to 25 AU for a distance of 330 pc). The H and K images were reconstructed from 6 m telescope speckle data and the RG 715 image from 2.2 m telescope data using the speckle masking bispectrum method. At all wavelengths the images show a compact, highly symmetric bipolar nebula, suggesting a toroidal density distribution of the circumstellar material. No direct light from the central binary can be seen as it is obscured by a dust disk or circumbinary torus. Our first high-resolution H−K color image of the nebula shows a broad red plateau of H−K≈ 2m in the bright inner regions.The optical and near-infrared images and the available photometric continuum observations in a wide range of ultraviolet to centimeter wavelengths enabled us to model the Red Rectangle in detail using a two-dimensional radiative transfer code. Our model matches both the high-resolution images and the spectral energy distribution of this object very well, making the following picture much more certain. The central close binary system with a total luminosity of 3000 L is embedded in a very dense, compact circumbinary torus which has an average number density nH ≈5×1012 cm−3, an outer radius of the dense inner region of R≈30 AU (91 mas), and a ρ∝r−2 density distribution. The full opening angle of the bipolar outflow cavities in our model is 70°. By comparing the observed and theoretical images, we derived an inclination angle of the torus to the line of sight of 7°±1°.The radiative transfer calculations show that the dust properties in the Red Rectangle are spatially inhomogeneous. The modeling confirms that the idea of large grains in the long-lived disk around the Red Rectangle (Jura et al., 1997 [ApJ, 474, 741]) is quantitatively consistent with the observations. In our models, unusually large, approximately millimeter-sized grains dominate the emission of the compact, massive torus. Models with smaller average grain sizes can possibly be found in future studies, for instance, if it turns out that the radio spectrum is not mainly caused by continuum dust emission. Therefore, the large grains suggested by our models require further confirmation by both new observations and radiative transfer calculations. Assuming a dust-to-gas ratio ρd/ρg of 0.005, the dense torus mass is 0.25 M. The model gives a lower limit of 0.0018 M, for the mass of the large particles, which produce a gray extinction of A≈ 28m, towards the center. A much smaller mass of submicron-sized dust grains is presumably located in the polar outflow cavities, their conical surface layers, and in the outer low-density parts of the torus (where ρ∝r−4, in the region of 30 AUr 2000 AU corresponding to 0.′′09–6′′). 相似文献
79.
研究了盐度对黄鳍鲷SparuslatusHouttuyn、平鲷Rhabdosargussarba(Forskal)、黑鲷Sparusmacrocephalus(Basilewsky)和真鲷Pagrsomusmajor(TemmincketSchlegel)4种鲷鱼精子活力的影响。对南海区4种鲷鱼精子的适盐性及其活力进行了比较,黄鳍鲷、平鲷、黑鲷和真鲷精子激活所需的最低盐度分别为8、10、>8、>10;激活的最适盐度则分别为21、22、25、25,与之相应的精子活动(涡动)时间分别为14.7、17.7、17.2、18.0min;在高盐条件(盐度40左右)下,黄鳍鲷精子的适应性最强,精子活力最好,其次是黑鲷、真鲷的精子,平鲷精子对高盐条件的适应性最差。 相似文献
80.
Current plate motions across the Red Sea 总被引:3,自引:0,他引:3