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411.
412.
Josef Horálek Tomá? Fischer Alena Bou?ková Petr Jedli?ka 《Studia Geophysica et Geodaetica》2000,44(2):1-5
Foreword
FOREWORD 相似文献413.
Kerstin?DrostEmail author Ulf?Linnemann Neal?McNaughton Old?ich?Fatka Petr?Kraft Michael?Gehmlich Christian?Tonk Jaroslav?Marek 《International Journal of Earth Sciences》2004,93(5):742-757
The Teplá-Barrandian unit (TBU) of the Bohemian Massif was a part of the Avalonian-Cadomian belt at the northern margin of Gondwana during Neoproterozoic and Early Cambrian times. New detrital zircon ages and geochemical compositions of Late Neoproterozoic siliciclastic sediments confirm a deposition of the volcano-sedimentary successions of the TBU in a back-arc basin. A change in the geotectonic regime from convergence to transtension was completed by the time of the Precambrian-Cambrian boundary. The accumulation of around 2,500 m Lower Cambrian continental siliciclastics in a Basin-and-Range-type setting was accompanied by magmatism, which shows within-plate features in a few cases, but is predominantly derived from anatectic melts displaying the inherited island arc signature of their Cadomian source rocks. The geochemistry of clastic sediments suggests a deposition in a rift or strike-slip-related basin, respectively. A marine transgression during Middle Cambrian times indicates markedly thinned crust after the Cadomian orogeny. Upper Cambrian magmatism is represented by 1,500 m of subaerial andesites and rhyolites demonstrating several geochemical characteristics of an intra-plate setting. Zircons from a rhyolite give a U-Pb-SHRIMP age of 499±4 Ma. The Cambrian sedimentary and magmatic succession of the TBU records the beginning of an important rifting event at the northern margin of Gondwana.
相似文献
Kerstin DrostEmail: |
414.
415.
Magnetic fabric variations in Mesozoic black shales, Northern Siberia, Russia: Possible paleomagnetic implications 总被引:1,自引:0,他引:1
Martin Chadima Petr Pruner Stanislav lechta Tom Grygar Ann M. Hirt 《Tectonophysics》2006,418(1-2):145
A 28-m-long section situated on the coast of the Arctic Ocean, Russia (74°N, 113°E) was extensively sampled primarily for the purpose of magnetostratigraphic investigations across the Jurassic/Cretaceous boundary. The section consists predominantly of marine black shales with abundant siderite concretions and several distinct siderite cemented layers. Low-field magnetic susceptibility (k) ranges from 8 × 10− 5 to 2 × 10− 3 SI and is predominantly controlled by the paramagnetic minerals, i.e. iron-bearing chlorites, micas, and siderite. The siderite-bearing samples possess the highest magnetic susceptibility, usually one order of magnitude higher than the neighboring rock. The intensity of the natural remanent magnetization (M0) varies between 1 × 10− 5 and 6 × 10− 3 A/m. Several samples possessing extremely high values of M0 were found. There is no apparent correlation between the high k and high M0 values; on the contrary, the samples with relatively high M0 values possess average magnetic susceptibility and vice versa. According to the low-field anisotropy of magnetic susceptibility (AMS), three different groups of samples can be distinguished. In the siderite-bearing samples (i), an inverse magnetic fabric is observed, i.e., the maximum and minimum principal susceptibility directions are interchanged and the magnetic fabric has a distinctly prolate shape. Triaxial-fabric samples (ii), showing an intermediate magnetic fabric, are always characterized by high M0 values. It seems probable that the magnetic fabric is controlled by the preferred orientation of paramagnetic phyllosilicates, e.g., chlorite and mica, and by some ferromagnetic mineral with anomalous orientation in relation to the bedding plane. Oblate-fabric samples (iii) are characterized by a bedding-controlled magnetic fabric, and by moderate magnetic susceptibility and M0 values. The magnetic fabric is controlled by the preferred orientation of phyllosilicate minerals and, to a minor extent, by a ferrimagnetic fraction, most probably detrital magnetite. Considering the magnetic fabric together with paleomagnetic component analyses, the siderite-bearing, and the high-NRM samples (about 15% of samples) were excluded from further magnetostratigraphic research. 相似文献
416.
Jaromír Janský Vladimír Plicka Helene Lyon-Caen Oldřich Novotný 《Journal of Seismology》2007,11(2):199-204
We determine the velocities in an upper crustal model, composed of three homogeneous layers, for one subregion of the western
part of the Gulf of Corinth, NE of the town of Aigion, Greece. We have used local events that occurred there in the year 2001
and were recorded by the Corinth Rift Laboratory Network. Weighted P and S arrival time residuals are minimized using the Neighbourhood Algorithm of Sambridge (1999), combined with the grid search
for source locations. The resolution of the inversion is tested by delete-one jackknifing. The model obtained is compared
with some other models derived or applied to the subregion. A fast velocity increase between depths of 5 and 7 km is confirmed
as the major structural element. 相似文献
417.
Cyclic variations of the mean semi-annual intensities I
of the coronal green line 530.3 nm are compared with the mean semi-annual variations of the Wolf numbers W during the period of 1943–1999 (activity cycles 18–23). The values of I
in the equatorial zone proved to correlate much better with the Wolf numbers in a following cycle than in a given one (the correlation coefficient r is 0.86 and 0.755, respectively). Such increase of the correlation coefficient with a shift by one cycle differs in different phases of the cycle, being the largest at the ascending branch. The regularities revealed make it possible to predict the behaviour of W in the following cycle on the basis of intensities of the coronal green line in the preceding cycle. We predict the maximum semi-annual W in cycle 23 to be 110–122 and the epoch of minimum between cycles 23 and 24 to take place at 2006–2007. A slow increase of I
in the current cycle 23 permits us to forecast a low-Wolf-number cycle 24 with the maximum W50 at 2010–2011. A scheme is proposed on the permanent transformation of the coronal magnetic fields of different scales explaining the found phenomenon. 相似文献
418.
The scientific and operational aims of the Czech-made Hard X-Ray Spectrometer (HXRS) launched onboard the U.S. Department
of Energy Multispectral Thermal Imager satellite (MTI), on 12 March 2000 are discussed. The principal operating characteristics
of the instrument such as the temporal resolution, energy band selection, spectral sensitivity, and the in-flight calibration
procedure are described as well as the technical details of the spectrometer including detectors, shielding (against charged
particles) and electronic design. The MTI host satellite and its orbit are briefly described. Recent observations by the 3 GHz
Ondřejov radiometer are compared with HXRS data to demonstrate one example of the HXRS data utilization: the temporal relation
between hard X-rays and radio emission. These results show relatively long time delays (2–14 s) of the GHz broadband radio
pulses relative to the hard X-ray emission peaks. Access to the HXRS data base via the Internet is provided. 相似文献
419.
420.
Marek Wolf Petr Harmanec Josip Kleczek Pavel Mayer 《Astrophysics and Space Science》1987,134(1):205-208
Geographical, seasonal, and day-to-day variations in the vertical distributions of atmospheric density and temperature must be considered in the design and operation of reentry vehicles. This work is part of a continuing effort to compile, analyze, and present information on the distribution of the atmospheric temperature in a form suitable for use in the design and operation of aerospace vehicles. We have used temperature data obtained from rockets which are mostly based on the datasonde system throughout the decade 1969–1978. Profiles and the individual arrays of coefficients of correlation of the temperature at 20 km with temperature at higher altitudes up to 60 km are shown for each season for locations in the low, middle, and high latitudes. 相似文献