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931.
In the Lachlan Fold Belt of southeastern Australia, major orogenic gold and porphyry gold–copper deposits formed simultaneously
within distinct tectonic settings during a very short time interval at ca. 440 Ma. The driving mechanism that controlled the
temporal coincidence of these deposits remains largely unexplained. A review of contemporaneous metallogenic, tectonic, magmatic
and sedimentological events in central and eastern Australia reveals that a change in subduction dynamics along the Australian
sector of the Early Palaeozoic circum–Gondwana mega-subduction system could have influenced lithospheric stress conditions
far inboard of the subduction margin. The magnitude of ore formation and the spatial extent of related events are proposed
in this paper to have been controlled by the interplay of mantle processes and lithospheric changes that followed slab break-off
along a portion of the mega-subduction system surrounding Gondwana at that time. Slab break-off after subduction lock-up caused
mantle upwelling that, in turn, provided an instantaneous heat supply for magmatic and hydrothermal events. Coincident reorganisation
of lithospheric stress conditions far inboard of the proto-Pacific margin of Australia controlled reactivation of deep-lithospheric
fault structures. These fault systems provided a pathway for fluids and heat fuelled by mantle upwelling into the upper lithosphere
and caused the deposition of ~440 Ma gold deposits in the Lachlan Fold Belt, as well as a range of metallogenic, tectonic
and sedimentary changes elsewhere in central and eastern Australia. 相似文献
932.
Tsung-Ren Peng Chung-Ho Wang Tein-Chang Lai Frank Shu-Ken Ho 《Environmental Geology》2007,52(8):1617-1629
Over a 1-year period, 343 samples, including precipitation, creek, pond, and groundwater, were collected from June 2003 to
May 2004. Analyses were performed for stable oxygen and hydrogen isotope compositions. Selected samples were also analyzed
for tritium. The goal was to identify possible hydrologic factors contributing to a severe landslide in the Li-Shan area,
central Taiwan. The isotope characteristics indicate that groundwater from Fu-Shou-Shan farm located up-slope from the landslide
area is a major source for slope groundwater, in addition to precipitation. The groundwater is mainly recharged by pond water
at Fu-Shou-Shan farm. According to the calculation of a two-end member equation with δ
18O, the contribution of farm groundwater to slope groundwater is significantly higher than that of precipitation, up to a factor
of five. The estimated drainage efficiency of the existing system is only 23%. Draining off the slope groundwater in the up-slope
region to decrease farm groundwater flow into the slope area is a feasible strategy to effectively reduce the risk of landslide. 相似文献
933.
Anja Zander Detlev Degering Frank Preusser Haino Uwe Kasper Helmut Brückner 《Quaternary Geochronology》2007,2(1-4):123-128
Shallow marine and intertidal shell rich sediments from the low coastal plain of Dubai were dated by optically stimulated luminescence. Combined high-resolution gamma spectrometry and ICP–MS analyses revealed significant disequilibria in the 238U decay series. Time dependent dose rates were modelled for two scenarios including a closed system and an open system with linear U and Ra uptake. OSL ages that were calculated using the linear uptake model are in good agreement with archaeological evidence and radiocarbon datings on shells and wood. The presented results illustrate that luminescence-dating techniques are suitable to set up a chronostratigraphic frame for calcareous coastal environments if an appropriate model is applied to consider the influence of radioactive disequilibria and time dependent dose rates. A comprehensive radionuclide analysis of the sediments is thought necessary to perform geochemically supported dose rate simulations. 相似文献
934.
Selection and ranking of ground motion models for seismic hazard analysis in the Pyrenees 总被引:1,自引:0,他引:1
Stéphane Drouet Frank Scherbaum Fabrice Cotton Annie Souriau 《Journal of Seismology》2007,11(1):87-100
The issue addressed in this paper is the objective selection of appropriate ground motion models for seismic hazard assessment
in the Pyrenees. The method of Scherbaum et al. (2004a) is applied in order to rank eight published ground motion models relevant to intraplate or to low deformation rate contexts.
This method is based on a transparent and data-driven process which quantifies the model fit and also measures how well the
underlying model assumptions are met. The method is applied to 15 accelerometric records obtained in the Pyrenees for events
of local magnitude between 4.8 and 5.1, corresponding to moment magnitudes ranging from 3.7 to 3.9. Only stations at rock
sites are considered. A total of 720 spectral amplitudes are used to rank the selected ground motion models. Some control
parameters of these models, such as magnitude and distance definitions, may vary from one model to the other. It is thus important
to correct the selected models for their difference with respect to the magnitude and distance definitions used for the Pyrenean
data. Our analysis shows that, with these corrections, some of the ground motion models successfully fit the data. These are
the Lussou et al. (2001) and the Berge-Thierry et al. (2003) models. According to the selected ground motion models, a possible scenario of a magnitude 6 event is proposed; it predicts
response spectra accelerations of 0.08–0.1 g at 1 Hz at a hypocentral distance of 10 km. 相似文献
935.
Thomas D. Frank 《The Professional geographer》1985,37(1):36-46
Relationships between Landsat reflectance indexes that extract the individual component contributions of vegetation and the soil background and the composition of a semiarid grassland-shrub environment are examined. The results indicate that two reflectance indexes, the Transformed Vegetation Index (TVI) and the ratio of Landsat MSS6/MSS5, exhibit the highest correlation with vegetation density. The ratio of MSS6/MSS4, the ratio of MSS5/MSS4, and the MSS6 soil background reflectance component (Rgg6) emerge as the best indexes to discriminate between semiarid landscape units. The relationships between reflectance and land cover composition suggest that Landsat reflectance may be useful to monitor temporal and spatial changes in the condition of semiarid vegetation. 相似文献
936.
A.T.Y. Lui C.-I. Meng L.A. Frank K.L. Ackerson S.-I. Akasofu 《Planetary and Space Science》1981,29(8):837-842
The temperature and density of the plasma in the Earth's distant plasma sheet at the downstream distances of about 20–25 Re are examined during a high geomagnetic disturbance period. It is shown that the plasma sheet cools when magnetospheric substorm expansion is indicated by the AE index. During cooling, the plasma sheet temperature, T, and the number density, N, are related by (adiabatic process) in some instances, while by T ∝ N?1 (isobaric process) in other cases. The total plasma and magnetic pressure decreases when and increases when T ∝ N?1. Observation also indicates that the dawn-dusk component of plasma flow is frequently large and comparable to the sunward-tailward flow component near the central plasma sheet during substorms. 相似文献
937.
A highly anisotropic packet of solar electron intensities was observed on 6 April 1971 with a sensitive electrostatic analyzer array on the Earth-orbiting satellite IMP-6. The anisotropies of intensities at electron energies of several keV were factors 10 favoring the expected direction of the interplanetary magnetic lines of force from the Sun. The directional, differential intensities of solar electrons were determined over the energy range 1–40 keV and peak intensities were 102 cm–2 s–1 sr–1 eV–1 at 2–6 keV. This anisotropic packet of solar electrons was detected at the sattelite for a period of 4200 s and was soon followed by isotropic intensities for a relatively prolonged period. This impulsive emission was associated with the onsets of an optical flare, soft X-ray emission and a radio noise storm at centimeter wavelengths on the western limb of the Sun. Simultaneous measurements of a type III radio noise burst at kilometric wavelengths with a plasma wave instrument on the same satellite showed that the onsets for detectable noise levels ranged from 500 s at 178 kHz to 2700 s at 31.1 kHz. The corresponding drift rate requires a speed of 0.15c for the exciting particles if the emission is at the electron plasma frequency. The corresponding electron energy of 6 keV is in excellent agreement with the above direct observations of the anisotropic electron packet. Further supporting evidence that several-keV solar electrons in the anisotropic packet are associated with the emission of type III radio noise beyond 50R
is provided by their time-of-arrival at Earth and the relative durations of the radio noise and the solar electron packet. Electron intensities at E 45 keV and the isotropic intensities of lower-energy solar electrons are relatively uncorrelated with the measurements of type III radio noise at these low frequencies. The implications of these observations relative to those at higher frequencies, and heliocentric radial distances 50R
, include apparent deceleration of the exciting electron beam with increasing heliocentric radial distance.Research supported in part by the National Aeronautics and Space Administration under contracts NAS5-11039 and NAS5-11074 and grant NGL16-001-002 and by the Office of Naval Research under contract N000-14-68-A-0196-0003. 相似文献
938.
Residual intensity fluctuation measurements within the wings of the 5183.6 Mgi b1 line, obtained from two, high-resolution, high-dispersion, Sacramento Peak Observatory spectrograms, have been subtracted from intensity fluctuations in the adjacent continuum in order to isolate fluctuations associated exclusively with line formation. The useable spectral range for studying these lineformation fluctuations is restricted to wavelengths between 1040 and 7170 km because the subtraction increases the relative importance of noise and large-scale photographic variations across the spectrograms could not be completely removed. Power and cross-power (coherence and phase) spectra proved to be valuable diagnostic tools in isolating line-formation fluctuations.Over this spectral range, the line-formation fluctuations are characterized by flat power spectra as compared to those for continuum fluctuations, appreciable fluctuation rms relative to that for continuum fluctuations, and the necessity to multiply the wing fluctuations by a factor 0.95 min 1.00 to most effectively isolate these fluctuations (Figures 3 and 4). That continuum fluctuations are modified in shape but otherwise not drastically changed in the line wings explains the flat spectrum. The relative rms's vary from 0.34 in the inner wing to 0.22 in the outer. The range of possible values for
min results from uncertainties in the photographic density-residual intensity calibration. 相似文献
939.
Sebastian Wagner Martin Widmann Julie Jones Torsten Haberzettl Andreas Lücke Christoph Mayr Christian Ohlendorf Frank Schäbitz Bernd Zolitschka 《Climate Dynamics》2007,29(4):333-355
This study investigates the atmospheric circulation in transient climate simulations with a coupled atmosphere–ocean general
circulation model (GCM) for the mid-Holocene (MH) period 7–4.5 ka BP driven with combinations of orbital, solar and greenhouse
gas forcings. The focus is on southern South America. Statistical downscaling models are derived from observational data and
applied to the simulations to estimate precipitation in south-eastern Patagonia during the MH. These estimates are compared
with lake level estimates for Laguna Potrok Aike (LPA) from sediments. Relative to pre-industrial conditions (i.e. 1550–1850),
which show extraordinarily high lake levels, the proxy-based reconstructed lake levels during the MH are lower. The downscaled
simulated circulation differences indicate higher LPA precipitation during the MH from March to August, higher annual means,
and reduced precipitation from September to February. Thus the reconstructed lower LPA lake levels can not be explained solely
by the simulated precipitation changes. Possible reasons for this discrepancy are discussed. Based on proxy data from southern
South America hypotheses have also been proposed on the latitudinal position of the southern hemispheric westerlies (SHWs).
In agreement with some of these hypotheses our simulations show an increased seasonal cycle of the latitudinal position of
the SHWs during the MH, which can be explained by the orbital forcing. The simulations also show stronger SHWs over southern
Patagonia during austral summer and weaker SHWs during winter. The downscaling model associates weaker SHWs with increased
precipitation in the LPA region. However, this relationship is only moderate, and therefore the downscaling model does not
support the assumption of a strong link between mean SHWs and precipitation over south-eastern Patagonia, which is the basis
of many proxy-based hypotheses about the SHWs. 相似文献
940.
Frank Drewnick Johannes Schneider Silke S. Hings Nele Hock Kevin Noone Admir Targino Silke Weimer Stephan Borrmann 《Journal of Atmospheric Chemistry》2007,56(1):1-20
The Aerodyne aerosol mass spectrometer (Q-AMS) was coupled with a counterflow virtual impactor (CVI) for the first time to measure cloud droplet residuals of warm tropospheric clouds on Mt. Åreskutan in central Sweden in July 2003. Operating the CVI in different operational modes generated mass concentration and species-resolved mass distribution data for non-refractory species of the ambient, interstitial, and residual aerosol. The ambient aerosol measurements revealed that the aerosol at the site was mainly influenced by long-range transport and regional photochemical generation of nitrate and organic aerosol components. Four different major air masses were identified for the time interval of the experiment. While two air masses that approached the site from northeastern Europe via Finland showed very similar aerosol composition, the other two air masses from polar regions and the British Islands had a significantly different composition. During cloud events the larger aerosol particles were found to be activated into cloud droplets. On a mass basis the activation cut-off diameter was approximately 150 nm for nitrate and organics dominated particles and 200 nm for sulfate dominated particles. Generally nitrate and organics were found to be activated into cloud droplets with higher efficiency than sulfate. While a significant fraction of the nitrate in ambient particles was organic nitrates or nitrogen-containing organic species, the nitrate found in the cloud droplet residuals was mainly ammonium nitrate. After passage of clouds the ambient aerosol size distribution had shifted to smaller particle sizes due to the predominantly activation of larger aerosol particles without a significant change in the relative composition of the ambient aerosol. 相似文献