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141.
Jeff Standish Dennis Geist Karen Harpp Mark D. Kurz 《Contributions to Mineralogy and Petrology》1998,133(1-2):136-148
Roca Redonda volcano is a mostly submarine shield volcano that rises nearly 3 km from the adjacent seafloor. Over twenty
lava flows and palagonite tuff are exposed in a 60 meter high oblong outcrop above sea level, and several other flows are
exposed in the shallow water surrounding the islet. Thick, slightly alkaline picritic flows form the base of the section.
Thinner picrites interbedded with sparsely porphyritic alkali-olivine basaltic pahoehoe toes characterize the upper section.
The subaerial section probably records the filling of a palagonite tuff cone with younger lavas. Numerous fumaroles that may
have a magmatic component are present in the shallow (<30 m) submarine zone and indicate that the volcano is probably still
active. Three lava types are exposed: the basal picrites with 19% > MgO > 14%, high-Mg basalts with MgO of about 9%, and low-Mg
basalts with MgO of about 6%. The Sr and Nd isotopic ratios of the three lava types are within analytical uncertainty. Olivine
compositions indicate that the picrites are basaltic liquids that have accumulated olivine whose composition is in equilibrium
with the host basaltic liquid. Apparently, basaltic magmas percolated through dunite and troctolite that had crystallized
from slightly older Roca Redonda basaltic magma. Lavas from Roca Redonda have enriched trace element contents and isotopic
ratios relative to nearby Wolf volcano, but they are quite similar to lavas from Cerro Azul and Ecuador volcanoes. The common
characteristic of these volcanoes is that they lie on the periphery of the archipelago and are in a stage of subaerial growth.
This suggests that Galápagos volcanoes may go through a juvenile alkaline stage before a mature tholeiitic stage, analogous
to the Loihi stage of Hawaiian volcanism. A low 3He/4He ratio in olivine from one of the picrites indicates a small contribution by the Galápagos mantle plume.
Received: 15 December 1997 / Accepted: 6 May 1998 相似文献
142.
The distribution of crystalline salt minerals in deposits in the McMurdo region of Antarctica has been examined to study the origin of these salts. Sulphate, chloride, sodium and calcium salts are most frequently encountered. Salts containing chloride and sodium ions become less common away from the coast. Sulphate salts are more regularly distributed but tend to be related isotopically to sea water sulphate. Salts containing magnesium ion tend to exist mainly on substrates composed of basic igneous rocks, whereas calcium and carbonate salts are present on all rock types in the region.These distributions show that salts of marine origin are regionally and quantitatively most important but that chemical weathering of mafic materials in rocks and soils is also significant. However, biological, volcanic and hydrothermal processes are or have been active contributing to salts in local areas, that include penguin rookeries and eastern Taylor Valley, the summit area of Erebus Volcano, and subsurface rocks, respectively. 相似文献
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144.
John B. Anderson Richard Wheeler Charles P. Dunning Sue Shepley Marion Fowke 《Environmental Geology》1978,2(2):67-78
A historical record of the effects of human development upon Lake Macatawa is established using geologic criteria. Significant
cultural events are recognized using the pollen record, particularly ambrosia/vesiculate pollen ratios, and occurrences of
detrital and chemical contaminants within the more recent sedimentary column. Detrital contaminants include such things as
cinder and ash from coal burning power plants and animal hair from early tanning operations. Trace metal contaminants, frequently
associated with specific industrial events, are particularly useful in establishing a modern sedimentary chronology.
The impact of human activity upon Lake Macatawa is measured using fossil diatoms. The advantage of this method of environmental
impact assessment is that it provides a historical perspective in which changes within an environment are related to its natural
conditions. 相似文献
145.
Self-diffusion of oxygen in a natural phlogopite mica (annite 4%) has been measured under hydrothermal conditions at 2000 bars pressure and from 500 to 800°C using water enriched in18O. Diffusional transport is dominantly parallel to the c crystallographic axis. A linear Arrhenius plot was obtained with a pre-exponential term = (1.03 ± 0.38) × 10?9cm2sec?1 a and an activation energy of 29 ± 2kcal/g-atom O. The difference in transport rate between oxygens in the OH groups and those in tetrahedral sites is small to non-existent unless the OH oxygens diffuse much more slowly than the other oxygens, which we consider unlikely. A typical phlogopite crystal, 0.2 mm thick by 1 mm across will lose radiogenic argon faster than it will exchange oxygen at temperatures above 435°C, but the reverse holds at lower temperatures if the diffusion mechanism can be extrapolated to temperatures below 500°C. Such a crystal will lose only 5% of its argon if held at 380°C for 1 m.y., but could exchange 27% of its oxygen in that time. The rate at which phlogopite will undergo deformation by diffusional creep does not appear to be controlled by oxygen diffusion. 相似文献
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147.
By the method of electron reflection, we have identified seven well-defined magnetized regions in the equatorial belt of the lunar far side sampled by the Apollo 16 Particles and Fields subsatellite. Most of these surface magnetic fields lie within one basin radius from the rim of a ringed impact basin, where thick deposits of basin ejecta are observed or inferred. The strongest of the seven magnetic features is linear, at least 250 km long, and radial to the Freundlich-Sharonov basin. The apparent correlation with basin ejecta suggests some form of impact origin for the observed permanently magnetized regions. 相似文献
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