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291.
We use a dynamic finite-difference model to simulate martian landslides in the Valles Marineris canyon system and Olympus Mons aureole using three different modal rheologies: frictional, Bingham, and power law. The frictional and Bingham modes are applied individually. Fluidized rheology is treated as a combination of frictional and power-law modes; general fluidization can include pore pressure contributions, whereas acoustic fluidization does not. We find that general fluidization most often produces slides that best match landslide geometry in the Valles Marineris. This implies that some amount of supporting liquid or gas was present in the material during failure. The profile of the Olympus Mons aureole is not well matched by any landslide model, suggesting an alternative genesis. In contrast, acoustic fluidization produces the best match for a lunar slide, a result anticipated for dry crust with no overlying atmosphere. The presence of pressurized fluid during Valles Marineris landsliding may be due to liquid water beneath a thin cryosphere (<1-2 km) or flash sublimation of CO2. 相似文献
292.
Chris Blake Michael B. Pracy Warrick J. Couch Kenji Bekki Ian Lewis Karl Glazebrook Ivan K. Baldry Carlton M. Baugh Joss Bland-Hawthorn Terry Bridges Russell Cannon Shaun Cole Matthew Colless Chris Collins Gavin Dalton Roberto De Propris Simon P. Driver George Efstathiou Richard S. Ellis Carlos S. Frenk Carole Jackson Ofer Lahav Stuart Lumsden Steve Maddox Darren Madgwick Peder Norberg John A. Peacock Bruce A. Peterson Will Sutherland Keith Taylor 《Monthly notices of the Royal Astronomical Society》2004,355(3):713-727
293.
294.
Anisotropy of magnetic susceptibility and structural geology of the ca. 1.45 Ga Karlshamn pluton (southern Sweden) are used
to study its emplacement and structural evolution. The Karlshamn pluton is one of the largest metaluminous A-type granitoid
intrusions in southern Sweden. It is a multiphase body made up of two suites that differ in composition but which have similar
crystallization ages. The magmatic foliation, ductile shear zones and granite–pegmatite filled fractures were mapped as well
as the metamorphic foliation and extension lineation in the metamorphic host rocks. The anisotropy of magnetic susceptibility
was used to map the magnetite petrofabric of the pluton, providing a larger data set for both the magmatic foliations and
lineations, which could not be mapped in the field. The fabrics within the pluton are continuous with the metamorphic fabrics
in the country rocks. Both the pluton and the country rock fabrics were folded during ENE–WSW compression, while the pluton
was still a magma mush. The stress field orientation during cooling of the pluton is determined on the basis of magmatic,
ductile and brittle structures in the Karlshamn pluton that formed successively as the pluton cooled. The compressional event
is referred to as the Danopolonian orogeny and therefore the Karlshamn granitoids, and other plutons of similar composition
and age in central and southern Sweden, on the Danish Island of Bornholm, and in Lithuania, may be considered as syntectonic
intrusions and not as anorogenic, as was previously thought. 相似文献
295.
Port surveys are being conducted in Australia, New Zealand and around the world to confirm the presence or absence of particular marine pests. The most critical aspect of these surveys is their sensitivity-the probability that they will correctly identify a species as present if indeed it is present. This is not, however, adequately addressed in the relevant national and international standards. Simple calculations show that the sensitivity of port survey methods is closely related to their encounter rate-the average number of target individuals expected to be detected by the method. The encounter rate (which reflects any difference in relative pest density), divided by the cost of the method, provides one way to compare the cost-effectiveness of different survey methods. The most cost-effective survey method is site- and species-specific but, in general, will involve sampling from the habitat with the highest expected population of target individuals. A case study of Perna viridis in Trinity Inlet, Cairns, demonstrates that plankton trawls processed with gene probes provide the same level of sensitivity for a fraction of the cost associated with the next best available method-snorkel transects in bad visibility (secchi depth=0.72 m). Visibility and the adult/larvae ratio, however, are critical to these arguments. If visibility were good (secchi depth=10 m), the two approaches would be comparable. Diver deployed quadrats were at least three orders of magnitude less cost-effective in this case study. It is very important that environmental managers and scientists perform sensitivity calculations before embarking on port surveys to ensure the highest level of sensitivity is achieved for any given budget. 相似文献
296.
Keith Harries 《Geoforum》2006,37(3):404-416
A salient characteristic of the geography of crime in the US is the presence of extremely sharp geographic variations. These variations may be significant indicators of local environmental inequalities and may have implications for fear of crime and crime contagion, and may also be indicators of potential or actual neighborhood instability. Such micro-level variations are not generally apparent on small scale maps of urban crime. Previously, micro-level analysis of this gradient phenomenon has been inhibited by the confluence of large volumes of data over large areas, a plethora of possible boundaries that might be used for the purpose of data aggregation, and practical difficulties in the identification of gradients in the context of small units of analysis. The present study attempts to identify steep crime gradients and to characterize the physical and social circumstances under which they occur. Analysis was based on 97,880 geocodable incidents reported in 2000 in Baltimore County, Maryland. Crime densities were calculated for 5324 census blocks that experienced at least one crime incident. A steep gradient for the purpose of this research was the juxtaposition of blocks in the highest and lowest quintiles in terms of crime density. Using residential and commercial land uses as a filter, some 259 blocks satisfied the gradient criterion. Further analysis linked these blocks to their parent block groups for the purpose of identifying their social attributes. In addition, six clusters of blocks were investigated in the field. A typology of adjacencies identified six categories. 相似文献
297.
Will J. Percival Carlton M. Baugh Joss Bland-Hawthorn Terry Bridges Russell Cannon Shaun Cole Matthew Colless Chris Collins Warrick Couch Gavin Dalton Roberto De Propris Simon P. Driver George Efstathiou Richard S. Ellis Carlos S. Frenk Karl Glazebrook Carole Jackson Ofer Lahav Ian Lewis Stuart Lumsden Steve Maddox Stephen Moody Peder Norberg John A. Peacock Bruce A. Peterson Will Sutherland Keith Taylor 《Monthly notices of the Royal Astronomical Society》2001,327(4):1297-1306
The 2dF Galaxy Redshift Survey has now measured in excess of 160 000 galaxy redshifts. This paper presents the power spectrum of the galaxy distribution, calculated using a direct Fourier transform based technique. We argue that, within the k -space region , the shape of this spectrum should be close to that of the linear density perturbations convolved with the window function of the survey. This window function and its convolving effect on the power spectrum estimate are analysed in detail. By convolving model spectra, we are able to fit the power-spectrum data and provide a measure of the matter content of the Universe. Our results show that models containing baryon oscillations are mildly preferred over featureless power spectra. Analysis of the data yields 68 per cent confidence limits on the total matter density times the Hubble parameter , and the baryon fraction , assuming scale-invariant primordial fluctuations. 相似文献
298.
Keith Taylor 《Astrophysics and Space Science》1974,26(2):327-336
A fast new deconvolution technique has been developed which employs a complex iterative scheme in order to deconvolve severely broadened noisy data. A great many computer-simulated experiments have been made using the iterative scheme in order to test its reliability and stability in many different situations. It is found to be extremely reliable in the reclaiming of partially resolved multi-featured spectra and can be used with any type of instrumental profile. Deconvolution of single Gaussian features are achieved in 5% noise conditions, where the instrumental profile is 5 times broader than the spectral features to be reclaimed. 相似文献
299.
We present infrared (20 μm) observations of Saturn's rings for a solar elevation angle of 10° and phase angle of 6°. Scans across the rings yield information about the cooling of particles during eclipse and the subsequent heating along their orbits. All three rings exhibit significant cooling during eclipse, as well as a 20-μm brightness asymmetry between east and west ansae, the largest asymmetry occuring in the C ring (the brightest ring). The eclipse cooling is a simple and adequate explanation for 20-μm brightness asymmetries between the ansae of Saturn's rings. The relatively large C ring asymmetry is thought to be primarily due to the short travel time of the particles in that ring from eclipse exit to east ansa. We compare the B ring data to the theoretical models of H.H. Aumann and H.H. Kieffer (1973, Astrophys. J.186, 305–311) in order to set constraints on the average particle size and thermal inertia. The rather rapid heating after exit from eclipse points to low-conductivity-particle surfaces, similar to the water frost surfaces of Galilean satellites. If the surface conductivity is indeed low, one cannot determine an upper limit for the particle size through such infrared observations, since only the uppermost millimeters experience a thermal response during eclipse. However, based on these infrared data alone, it is clear that particles of radius equal to a few millimeters or less cannot occupy a significant fraction of the ring surface area, because-regardless of thermal inertia-their thermal response is much faster than observed. 相似文献
300.
Keith J. Tinkler 《Mathematical Geology》1971,3(4):335-355
A quantitative analysis was made of the spatial arrangement of 149explosion craters in the western rift of Uganda. A variety of methods demonstrate that the spatial pattern of the craters reveals significant structural patterns that have guided volcanism to the surface. It is shown that the east-west elements in the field affected location, and the main rift fault is resolved into two main components. Tentatively, a possible dextral transform fault is identified that affected the relative location of the two main zones of activity. Grouping techniques demonstrate that crater groups obey an exponential rank-size rule and allow a mapping of the craters into energy classes that reveals a concentric pattern of energy in the field. The effect of the topography on energy levels and crater size show that only topography greater than 11,000ft could have prevented all eruptive activity, but the smaller energies and craters are sensitive to height differences on the order of the height of the rift wall, about 1000ft. Total energy in each crater class size is roughly constant, and the field energy could create one or two single craters comparable in size to small central volcanoes. 相似文献