全文获取类型
收费全文 | 1607篇 |
免费 | 76篇 |
国内免费 | 29篇 |
专业分类
测绘学 | 39篇 |
大气科学 | 176篇 |
地球物理 | 359篇 |
地质学 | 598篇 |
海洋学 | 131篇 |
天文学 | 248篇 |
综合类 | 4篇 |
自然地理 | 157篇 |
出版年
2023年 | 5篇 |
2022年 | 9篇 |
2021年 | 30篇 |
2020年 | 33篇 |
2019年 | 21篇 |
2018年 | 48篇 |
2017年 | 41篇 |
2016年 | 74篇 |
2015年 | 45篇 |
2014年 | 65篇 |
2013年 | 111篇 |
2012年 | 54篇 |
2011年 | 98篇 |
2010年 | 83篇 |
2009年 | 91篇 |
2008年 | 90篇 |
2007年 | 93篇 |
2006年 | 93篇 |
2005年 | 61篇 |
2004年 | 62篇 |
2003年 | 47篇 |
2002年 | 47篇 |
2001年 | 39篇 |
2000年 | 31篇 |
1999年 | 36篇 |
1998年 | 23篇 |
1997年 | 19篇 |
1996年 | 19篇 |
1995年 | 16篇 |
1994年 | 12篇 |
1993年 | 16篇 |
1992年 | 7篇 |
1991年 | 17篇 |
1990年 | 15篇 |
1989年 | 15篇 |
1987年 | 13篇 |
1986年 | 17篇 |
1985年 | 8篇 |
1984年 | 5篇 |
1983年 | 14篇 |
1982年 | 12篇 |
1981年 | 14篇 |
1980年 | 12篇 |
1979年 | 6篇 |
1978年 | 6篇 |
1977年 | 6篇 |
1976年 | 6篇 |
1975年 | 4篇 |
1974年 | 7篇 |
1973年 | 5篇 |
排序方式: 共有1712条查询结果,搜索用时 15 毫秒
131.
Pranab K. Roy Chowdhury Jeanette E. Weaver Eric M. Weber Dalton Lunga St. Thomas M. LeDoux Amy N. Rose 《International Journal of Digital Earth》2020,13(1):119-135
ABSTRACTUrban areas presently consume around 75% of global primary energy supply, which is expected to significantly increase in the future due to urban growth. Having sustainable, universal energy access is a pressing challenge for most parts of the globe. Understanding urban energy consumption patterns may help to address the challenges to urban sustainability and energy security. However, urban energy analyses are severely limited by the lack of urban energy data. Such datasets are virtually non-existent for the developing countries. As per current projections, most of the new urban growth is bound to occur in these data-starved regions. Hence, there is an urgent need of research methods for monitoring and quantifying urban energy utilization patterns. Here, we apply a data-driven approach to characterize urban settlements based on their formality, which is then used to assess intra-urban urban energy consumption in Johannesburg, South Africa; Sana’a, Yemen; and Ndola, Zambia. Electricity is the fastest growing energy fuel. By analyzing the relationship between the settlement types and the corresponding nighttime light emission, a proxy of electricity consumption, we assess the differential electricity consumption patterns. Our study presents a simple and scalable solution to fill the present data void to understand intra-city electricity consumption patterns. 相似文献
132.
Eric M. Jones 《Icarus》1981,46(3):328-336
Monte Carlo calculations of the expansion of space-faring civilizations are presented for a wide range of values of the population growth coefficient (α) and emigration coefficient (γ). Even for the very low values proposed by Newman and Sagan (α = 10?4per year; γ = 10?8per year) the migration wavefront expands at 1.4 × 10?5 pc per year. Even with this low expansion velocity, such a civilization would fill the Galaxy in about 109 years. Filling times of the order of 60 million years seem probable. The wavefront velocity is approximated by , where is the average radial distance traveled, the average distance traveled, and υs the ship speed. This approximation was derived by Newman. 相似文献
133.
Eric Bosset 《Aquatic Sciences - Research Across Boundaries》1976,38(2):69-70
Sans résumé
Insp. cant. eaux VD 相似文献
134.
In an attempt to reduce the threat of global warming, it has been proposed that the rise of atmospheric carbon dioxide concentrations be reduced by the ocean disposal of CO2 from the flue gases of fossil fuel-fired power plants. The release of large amounts of CO2 into mid or deep ocean waters will result in large plumes of acidified seawater with pH values ranging from 6 to 8. In an effort to determine whether these CO2-induced pH changes have any effect on marine nitrification processes, surficial (euphotic zone) and deep (aphotic zone) seawater samples were sparged with CO2 for varying time durations to achieve a specified pH reduction, and the rate of microbial ammonia oxidation was measured spectrophotometrically as a function of pH using an inhibitor technique. For both seawater samples taken from either the euphotic or aphotic zone, the nitrification rates dropped drastically with decreasing pH. Relative to nitrification rates in the original seawater at pH 8, nitrification rates were reduced by ca. 50% at pH 7 and more than 90% at pH 6.5. Nitrification was essentially completely inhibited at pH 6. These findings suggest that the disposal of CO2 into mid or deep oceans will most likely result in a drastic reduction of ammonia oxidation rates within the pH plume and the concomitant accumulation of ammonia instead of nitrate. It is unlikely that ammonia will reach the high concentration levels at which marine aquatic organisms are known to be negatively affected. However, if the ammonia-rich seawater from inside the pH plume is upwelled into the euphotic zone, it is likely that changes in phytoplankton abundance and community structure will occur. Finally, the large-scale inhibition of nitrification and the subsequent reduction of nitrite and nitrate concentrations could also result in a decrease of denitrification rates which, in turn, could lead to the buildup of nitrogen and unpredictable eutrophication phenomena. Clearly, more research on the environmental effects of ocean disposal of CO2 is needed to determine whether the potential costs related to marine ecosystem disturbance and disruption can be justified in terms of the perceived benefits that may be achieved by temporarily delaying global warming. 相似文献
135.
136.
Eric Gutierrez 《Geoforum》2007,38(5):886-900
Meeting Millennium Development Goals on water and sanitation services in developing countries are fraught with difficulties, as can be seen most clearly from the experiences of Malawi and Zambia, two of the world’s poorest countries that have committed to meeting these goals. The challenges are not only technical, requiring programmatic or engineering solutions, but are also and most importantly political, because solutions will most often cause a rearrangement of the peculiar forms of power relations that have emerged within institutional and political environments of the two countries. The challenges include weak state support for water and sanitation provision, unreliable and contested indicators of coverage, poor sectoral co-ordination, and fragmented donor efforts. This field note examines these challenges in greater detail to cast new light as well as draw attention to possible solutions that can be implemented. 相似文献
137.
The Zagros fold-and-thrust belt of SW-Iran is among the youngest continental collision zones on Earth. Collision is thought to have occurred in the late Oligocene–early Miocene, followed by continental shortening. The High Zagros Belt (HZB) presents a Neogene imbricate structure that has affected the thick sedimentary cover of the former Arabian continental passive margin. The HZB of interior Fars marks the innermost part of SE-Zagros, trending NW–SE, that is characterised by higher elevation, lack of seismicity, and no evident active crustal shortening with respect to the outer (SW) parts. This study examines the brittle structures that developed during the mountain building process to decipher the history of polyphase deformation and variations in compressive tectonic fields since the onset of collision. Analytic inversion techniques enabled us to determine and separate different brittle tectonic regimes in terms of stress tensors. Various strike–slip, compressional, and tensional stress regimes are thus identified with different stress fields. Brittle tectonic analyses were carried out to reconstruct possible geometrical relationships between different structures and to establish relative chronologies of corresponding stress fields, considering the folding process. Results indicate that in the studied area, the main fold and thrust structure developed in a general compressional stress regime with an average N032° direction of σ1 stress axis during the Miocene. Strike–slip structures were generated under three successive strike–slip stress regimes with different σ1 directions in the early Miocene (N053°), late Miocene–early Pliocene (N026°), and post-Pliocene (N002°), evolving from pre-fold to post-fold faulting. Tensional structures also developed as a function of the evolving stress regimes. Our reconstruction of stress fields suggests an anticlockwise reorientation of the horizontal σ1 axis since the onset of collision and a significant change in vertical stress from σ3 to σ2 since the late stage of folding and thrusting. A late right-lateral reactivation was also observed on some pre-existing belt-parallel brittle structures, especially along the reverse fault systems, consistent with the recent N–S plate convergence. However, this feature was not reflected by large structures in the HZB of interior Fars. The results should not be extrapolated to the entire Zagros belt, where the deformation front has propagated from inner to outer zones during the younger events. 相似文献
138.
Effects of mesoscale sea-surface temperature fronts on the marine atmospheric boundary layer 总被引:1,自引:0,他引:1
Eric D. Skyllingstad Dean Vickers Larry Mahrt Roger Samelson 《Boundary-Layer Meteorology》2007,123(2):219-237
A numerical modelling study is presented focusing on the effects of mesoscale sea-surface temperature (SST) variability on
surface fluxes and the marine atmospheric boundary-layer structure. A basic scenario is examined having two regions of SST
anomaly with alternating warm/cold or cold/warm water regions. Conditions upstream from the anomaly region have SST values
equal to the ambient atmosphere temperature, creating an upstream neutrally stratified boundary layer. Downstream from the
anomaly region the SST is also set to the ambient atmosphere value. When the warm anomaly is upstream from the cold anomaly,
the downstream boundary layer exhibits a more complex structure because of convective forcing and mixed layer deepening upstream
from the cold anomaly. An internal boundary layer forms over the cold anomaly in this case, generating two distinct layers
over the downstream region. When the cold anomaly is upstream from the warm anomaly, mixing over the warm anomaly quickly
destroys the shallow cold layer, yielding a more uniform downstream boundary-layer vertical structure compared with the warm-to-
cold case. Analysis of the momentum budget indicates that turbulent momentum flux divergence dominates the velocity field
tendency, with pressure forcing accounting for only about 20% of the changes in momentum. Parameterization of surface fluxes
and boundary-layer structure at these scales would be very difficult because of their dependence on subgrid-scale SST spatial
order. Simulations of similar flow over smaller scale fronts (<5 km) suggest that small-scale SST variability might be parameterized
in mesoscale models by relating the effective heat flux to the strength of the SST variance. 相似文献
139.
Neil S. Mancktelow Djordje Grujic Eric L. Johnson 《Contributions to Mineralogy and Petrology》1998,131(1):71-85
A backscattered and secondary electron SEM study of the grain boundary microstructure in quartz mylonites sampled along the length of the retrograde Simplon Fault Zone established three characteristic components. (1) Fine isolated pores (≤?1?μm diameter) are scattered across two-grain interfaces, preferentially concentrated on surfaces in extension. Pores are uncommon on three-grain junctions and there is no evidence for fluid interconnectivity along three- and four-grain junctions. The fine porosity may develop by accumulation of original, mainly intragranular fluid inclusions to the grain boundary during deformation and recrystallization and by cavitation of grain boundaries during grain boundary sliding. Dynamic cavitation implies that the “ductile” mylonitic deformation is at least locally dilatant and therefore pressure sensitive. (2) Large “vug”-like pores (up to mm-scale) extend along multi-grain boundaries. Observed in all samples, they are most common in the higher initial temperature, coarse-grained samples with a microstructure dominated by grain boundary migration recrystallization. Grains bordering this connected porosity develop perfect crystal faces, undecorated by fine pores or pits. The irregular “lobate” optical microstructure of many migrating grain boundaries actually consists of a series of straight crystal faces. The coarse porosity is probably due to accumulation during dynamic recrystallization of (CO2-rich ?) fluid with a high wetting angle against quartz. (3) In one sample, interconnected sinuous ridges, ≤?0.2?μm high, are observed to follow three- and four-grain junctions and disjoint into more isolated worms and spheroidal globules. On two-grain interfaces, these are transitional to more branching vein-like or convoluted brain-like forms. The brain-like and globular forms have been observed, with varying frequency, through the range of samples, with the globules attaining sizes of up to 60?μm. Vein structures have also been observed on intragranular fractures. These topologies do not match across adjoining surfaces and must have developed into free space. The ridge-vein-brain-spheroid structure is distinctly different to that previously observed on experimentally healed microcracks and its origin is not unequivocally established. They could represent unstable meniscus necking of a thin grain-boundary phase of low viscosity, developed due to quasi-adiabatic shear and/or local stress-induced dilatancy during microcracking. 相似文献
140.
Eric G. Blackman 《Monthly notices of the Royal Astronomical Society》1998,299(4):L48-L52
The α turbulent viscosity formalism for accretion discs must be interpreted as a mean field theory, modelling a steady state only on spatial or time-scales greater than those of the turbulence. The extent of the scale separation determines the relative precision error (RPE) of the predicted luminosity L ν . Turbulence and the use of α implies that (1) field line stretching gives a magnetic pressure α2 /6 of the total pressure generally, and a one-to-one relation between α and the pressure ratio for thin discs, and (2) large turbulent scales in advection-dominated accretion flows (ADAFs) predict a lower L ν precision than thin discs for a given observation duration and central mass. The allowed variability (or RPE) at frequency ν increases with the size of the contributing region. For X-ray binary ADAFs, the RPE ∼ 5 per cent at R ≤ 1000 Schwarzchild radii ( R s ) for averages over 1000 s. However, current data for galaxies like NGC 4258 and M87 give RPEs in L ν of 50–100 per cent even at R ≤ 100 R S . More data are required, but systematic deviations from ADAF predictions are more significant than random deviations, and may constrain properties of the turbulence, the accretion mode, the assumption of a steady state or the accretion rate. 相似文献