全文获取类型
收费全文 | 8186篇 |
免费 | 1361篇 |
国内免费 | 2063篇 |
专业分类
测绘学 | 815篇 |
大气科学 | 1659篇 |
地球物理 | 1699篇 |
地质学 | 3775篇 |
海洋学 | 1459篇 |
天文学 | 424篇 |
综合类 | 734篇 |
自然地理 | 1045篇 |
出版年
2024年 | 51篇 |
2023年 | 109篇 |
2022年 | 360篇 |
2021年 | 408篇 |
2020年 | 392篇 |
2019年 | 403篇 |
2018年 | 428篇 |
2017年 | 376篇 |
2016年 | 442篇 |
2015年 | 427篇 |
2014年 | 479篇 |
2013年 | 548篇 |
2012年 | 553篇 |
2011年 | 577篇 |
2010年 | 489篇 |
2009年 | 488篇 |
2008年 | 444篇 |
2007年 | 430篇 |
2006年 | 374篇 |
2005年 | 350篇 |
2004年 | 275篇 |
2003年 | 215篇 |
2002年 | 225篇 |
2001年 | 243篇 |
2000年 | 242篇 |
1999年 | 274篇 |
1998年 | 230篇 |
1997年 | 227篇 |
1996年 | 215篇 |
1995年 | 184篇 |
1994年 | 179篇 |
1993年 | 153篇 |
1992年 | 140篇 |
1991年 | 123篇 |
1990年 | 85篇 |
1989年 | 81篇 |
1988年 | 66篇 |
1987年 | 55篇 |
1986年 | 32篇 |
1985年 | 27篇 |
1984年 | 30篇 |
1983年 | 24篇 |
1982年 | 30篇 |
1981年 | 19篇 |
1980年 | 10篇 |
1979年 | 16篇 |
1977年 | 11篇 |
1976年 | 11篇 |
1975年 | 8篇 |
1973年 | 8篇 |
排序方式: 共有10000条查询结果,搜索用时 968 毫秒
141.
DMS (dimethylsulfide), a breakdown product of cellular solutes of many species of macroalgae andphytoplankton plays an important role in regulating global climate and counteracting partly the "greenhouse" effect.In this paper, the advance and prospects of DMS study are reviewed and discussed with respectto DMS sample storage, measurement and importance in regulating global climate and the acidity ofrain and aerosol. 相似文献
142.
On the basis of issues raised by observations of BL Lac objects and the qualitative jet model proposed by Bakeret al. in 1988, we have been led to consider the quantitative role of coherent, stimulated emission in jets and construct a new jet model of blazars in which a relativistic electron beam with an axial symmetric, power-law distribution is injected from the central engine into the jet plasma. We study quantitatively the synchrotron emission of the relativistic electron beams. Using the weak turbulent theory of plasma, we discuss the interaction between relativistic electron beams and jet plasma, and the roles of stimulated emission. The main results are:
- The synchrotron emission increases sensitively with the increase of the angle between the direction of the beam and the magnetic field. When the direction of the beam is vertical to the magnetic field, the synchrotron emission reaches its maximum, i.e. the emitted waves are beamed in the direction of the jet axis. We suggest that radio selected BL Lac objects belong to this extreme classification.
- The synchrotron emission of the relativistic beam increases rapidly with the increase of the Lorentz factor of the relativistic electron,γ, whenγ ≤ 22.5, then decreases rapidly with increase ofγ.
- The stimulated emission also increases with increasing Lorentz factorγ of the relativistic electrons whenγ ≤ 35 and then decreases with the increasingγ. The maximum stimulated emission and the maximum synchrotron emission occur at different frequencies. Stimulated emission is probably very important and reasonable flare mechanism in blazars.
- The rapid polarization position angle (PA) swings may arise from the interaction between the relativistic electron beam and the turbulent plasma.
143.
144.
西江主洼是珠江口盆地一个低勘探程度洼陷,油气差异聚集特征明显,但其机理不清。本文在断陷盆地油气成藏理论指导下,利用研究区地质、地球物理和地球化学等资料,开展了烃源岩、断盖组合、储集体系和运聚模式等方面的研究。结果表明,裂陷期沉降、沉积中心有序迁移,造成主力烃源岩自东向西由文四段迁移至文三段、文一+二段,控制东、西部油气差异分布。恩平组区域性泥岩发育且晚期断裂缺乏,导致油气纵向上更易聚集于下构造层;区域泥岩减薄尖灭或晚期断裂切开盖层的区域,上构造层有一定油气分布。"源-汇"类型从宏观上控制储层优劣,影响下构造层油气富集程度;"仓储"运移是控制上构造层油气规模聚集的主要模式。下构造层古近系应作为重点部署方向,东部围绕文四段、西部围绕文三段、文一+二段烃源岩构成的含油气系统展开;上构造层勘探需关注珠海组,在隆起周边寻找具备"仓储"运移模式的有利区带。 相似文献
145.
“4D”技术及其应用 总被引:13,自引:0,他引:13
介绍“4D”(即数字地面模型、数字正射影像、数字栅格地图和数字线划地图)系列产品的生产流程、关键技术、及其在耕地保护、防灾减灾救灾和城市规划等方面的应用方法。 相似文献
146.
Frederick A. Ochs III. Rebecca A. Lange 《Contributions to Mineralogy and Petrology》1997,129(2-3):155-165
The molar volumes of 19 hydrous albitic liquids (1.9 to 6.1 wt% H2Ototal) were determined at one bar and 505–765 K. These volume data were derived from density measurements on hydrous glasses at
298 K, followed by measurements of the thermal expansion of each glass from 298 K to its respective glass transition temperature.
The technique exploits the fact that the volume of a glass is equal to that of the corresponding liquid at the limiting fictive
temperature (T
f′), and that T
f′ can be approximated as the temperature near the onset of the rapid increase in thermal expansion that occurs in the glass
transition interval. The volume data of this study were combined with available volume data for anhydrous, Na2O-Al2O3-SiO2 liquids to derive the partial molar volume (±1) of the H2O component in an albitic melt at ∼565 K and one bar. To extend the determination of to higher temperatures and pressures, the molar volumes of the hydrous albitic liquids determined in this study were combined
with those measured by previous authors at 1023–1223 K and 480–840 MPa, leading to the following fitted values (±1) at 1673
K and one bar: (±0.46)×10−3 cm−3/mol-K, and dVˉ
H
2
O
total
/dP=−3.82 (±0.36)×10−4 cm3/mol-bar. The measured molar volumes of this study and those of previous authors can be recovered with a standard deviation
of 0.5%, which is within the respective experimental errors. There is a significant difference between the values for derived in this study as a function of temperature and pressure and those obtained from an existing polynomial, primarily
caused by the previous absence of accurate density measurements on anhydrous silicate liquids. The coefficients of thermal
expansion (=4.72×10−4/K) and isothermal compressibility (
T
=1.66×10−5/bar) for the H2O component at 1273 K and 100 MPa, indicate that H2Ototal is the single most expansive and compressible component in silicate liquids. For example, at 1473 K and 70 MPa (conditions
of a mid-ocean ridge crustal magma chamber), the presence of just 0.4 wt% H2O will decrease the density of a basaltic liquid by more than one percent. An equivalent decrease in melt density could be
achieved by increasing the temperature by 175 degrees or the decreasing pressure by 230 MPa. Therefore, even minor quantities
of dissolved water will have a marked effect on the dynamic properties of silicate liquids in the crustal environment.
Received: 20 August 1996 / Accepted: 15 March 1997 相似文献
147.
The nature of the solubility of water as [4H]Si defects in quartz, and their role in providing a source of molecular water on heating, is investigated. Existing ab inito energy calculations on the incorporation of water in quartz are used to show that energetically 4H for Si substitution is likely to constitute the most prevalent mode of water uptake on the atomic scale in quartz under equilibrium conditions, and that the planar defects previously observed by a number of different authors by electron microscopy in wet quartz are likely to be planar rafts of aggregated [4H]Si defects which are formed on supersaturation. These new conclusions call into question the previous identification of the planar defects as high pressure water clusters and require that their role in the production of molecular water in the context of recent theories of hydrolytic weakening be re-assessed. Accordingly the existing ab initio results have been used to establish the characteristics of the phase diagram for the system quartz-water in the temperature and pressure range of interest in hydrolytic weakening. Additional electron-optical experiments on wet quartz show that, on annealing at temperature in the electron microscope, similar planar defects develop in wet quartz by a diffusion process. In the context of existing theories of hydrolytic weakening it is now proposed that the conversion of [4H]Si defects to molecular water, where this is dictated by the equilibrium phase diagram, leads to a relatively large increase in volume and to the appearance of the bubbles of free water and the nucleation of associated prismatic dislocation loops of Burgers vector b=1/3 a $\langle 11\bar 20\rangle $ as previously observed. Ultimately the development of these loops leads to dislocation-induced plasticity. 相似文献
148.
Past studies of interplanetary magnetic sector boundaries have been based on the assumption that one can determine the field polarities by comparing the field directions with those of the nominal Parker spiral angles. Previous investigators have found evidence for decreases of B, the magnitude of the magnetic fieldB, and increases of , the angle betweenB and the ecliptic plane, at sector boundaries. Others have argued that the characteristic thickness of sector boundaries exceeds that of tangential discontinuities, making sector boundaries a separate class of structures.We use a simple technique for inferring the polarities of interplanetary magnetic fields based on the assumption thatE > 2 keV electrons are always flowing along the magnetic field away from the Sun. Electron data from the UC Berkeley experiment on the ISEE-3 spacecraft are used to examine periods around several apparent sector boundaries in 1978 and 1979. We compare properties of (a) boundaries with field polarity changes and (b) large-angle ( > 60°) directional discontinuities with no field polarity changes. We find no significant differences between the sector boundaries and the directional discontinuities in terms of associated decreases in B or of values of . These results suggest no significant difference between sector boundaries and directional discontinuities other than the change in field polarities. Within limited statistics we find that about half the polarity changes would not have been identified using a requirement that > 90° and that half of the > 120° discontinuities would have been misidentified as polarity changes. 相似文献
149.
Models for the motions of flare loops and ribbons 总被引:1,自引:0,他引:1
We have found a conformal mapping which is valid for any magnetic boundary condition at the photosphere and which can be used to determine the evolution of an open, two-dimensional magnetic field configuration as it relaxes to a closed one. Solutions obtained with this mapping are in quasi-static equilibrium, and they contain a vertical current sheet and have line-tied boundary conditions. As a specific example, we determine the solution for a boundary condition corresponding to a submerged, two-dimensional dipole below the photosphere. We assume that the outer edges of the hottest X-ray loops correspond to field lines mapping from the outer edges of the H ribbon to the lower tip of the current sheet where field lines reconnect at aY-type neutral line which rises with time. The cooler H loops are assumed to lie along the field lines mapping to the inner edges of the flare ribbons. With this correspondence between the plasma structures and the magnetic field we determine the shrinkage that field lines are observed to undergo as they are disconnected from the neutral line. During the early phase of the flare, we predict that shrinkage inferred from the height of the H and X-ray loops is close to 100% of the loop height. However, the shrinkage should rapidly decrease with time to values on the order of 20% by the late phase. We also predict that the shrinkage in very large loops obeys a universal scaling law which is independent of the boundary condition, provided that the field becomes self-similar (i.e., all field lines have the same shape) at large distances. Specifically, for any self-similar field containing aY-type neutral line, the observed shrinkage at large distances should decrease as (X/X
R)–2/3, where X is the ribbon width andX
Ris the ribbon separation. Finally, we discuss the relation between the electric field at the neutral line and the motions of the flare loops and ribbons. 相似文献
150.
Frederick W. Oliver 《Planetary and Space Science》1978,26(3):289-290
The Mossbauer spectra has been measured for the Leoville meteorite. Experimental results identify it as a type III carbonaceous meteorite. The spectrum shows the principle iron components to be olivine, magnetite, metallic iron, troilite and phyllosilicate material. 相似文献