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201.
Long-term performance of permeable reactive barriers using zero-valent iron: geochemical and microbiological effects 总被引:15,自引:0,他引:15
Geochemical and microbiological factors that control long-term performance of subsurface permeable reactive barriers were evaluated at the Elizabeth City, North Carolina, and the Denver Federal Center, Colorado, sites. These ground water treatment systems use zero-valent iron filings (Peerless Metal Powders Inc.) to intercept and remediate chlorinated hydrocarbon compounds at the Denver Federal Center (funnel-and-gate system) and overlapping plumes of hexavalent chromium and chlorinated hydrocarbons at Elizabeth City (continuous wall system). Zero-valent iron at both sites is a long-term sink for carbon, sulfur, calcium, silicon, nitrogen, and magnesium. After about four years of operation, the average rates of inorganic carbon (IC) and sulfur (S) accumulation are 0.09 and 0.02 kg/m2/year, respectively, at Elizabeth City where upgradient waters contain <400 mg/L of total dissolved solids (TDS). At the Denver Federal Center site, upgradient ground water contains 1000 to 1200 mg/L TDS and rates of IC and S accumulation are as high as 2.16 and 0.80 kg/m2/year, respectively. At both sites, consistent patterns of spatially variable mineral precipitation and microbial activity are observed. Mineral precipitates and microbial biomass accumulate the fastest near the upgradient aquifer-Fe0 interface. Maximum net reductions in porosity due to the accumulation of sulfur and inorganic carbon precipitates range from 0.032 at Elizabeth City to 0.062 at the Denver Federal Center (gate 2) after about four years. Although pore space has been lost due the accumulation of authigenic components, neither site shows evidence of pervasive pore clogging after four years of operation. 相似文献
202.
Hugues Leroux Guy Libourel Laurence Lemelle Franois Guyot 《Meteoritics & planetary science》2003,38(1):81-94
Abstract— An analytical transmission electron microscopy (ATEM) study was undertaken in order to better understand the formation conditions of dusty olivines (i.e., olivines containing abundant tiny inclusions of Fe‐Ni metal) in primitive meteorites. Dusty olivines from type I chondrules in the Bishunpur chondrite (LL3.1) and from synthetic samples obtained by reduction of San Carlos olivines were examined. In both natural and experimental samples, micron size metal blebs observed in the dusty region often show preferential alignments along crystallographic directions of the olivine grains, have low Ni contents (typically <2 wt%), and are frequently surrounded by a silica‐rich glass layer. These features suggest that dusty olivines are formed by a sub‐solidus reduction of initially fayalitic olivines according to the following reaction: Some volatilization of SiOgas may account for the apparent excess of metal relative to silica‐rich glass observed in both experimental and natural samples. Comparison with experimentally produced dusty olivines suggests that time scales of the order of minutes usually inferred for chondrule formation are also adequate for the formation of dusty olivines. These observations are in agreement with the hypothesis that at least part of the metal phase in chondrites originated from reduction during chondrule formation. 相似文献
203.
Raised Coral Terraces at Malakula, Vanuatu, Southwest Pacific, Indicate High Sea Level During Marine Isotope Stage 3 总被引:2,自引:0,他引:2
The occurrence of a series of raised coral reefs from the uplifted island of Malakula (Vanuatu, SW Pacific) provide an opportunity to examine sea-level fluctuations over at least the past 120,000 years. Thirteen fossil coral samples from Malakula were analyzed by the thermal ionization mass spectrometry (TIMS) U/Th dating technique, yielding information on sea levels during late marine isotope stage 3 and early stage 4. Our findings are in good agreement with sea-level estimates from raised coral terraces in Papua New Guinea and the recent sea-level reconstruction from the deep-sea sedimentary δ18O records. In particular, our coral data appear to confirm that sea levels at about 45,000–50,000 yr B.P. were only 30 to 60 m below the present level. Combined with other evidence of sea-level change, our data provide a strong case for much higher sea levels and therefore markedly reduced continental ice volume at 47,000 to 49,000 years ago. 相似文献
204.
This paper describes work undertaken to measure deformation of a pavement within the Newcastle University Rolling Load Facility (NUROLF). Precise three dimensional measurements of the pavement have been produced from stereo-imagery taken with diVerent cameras, using both analytical and digital photogrammetric instrumentation. The photogrammetric measurements, and those from the existing system consisting of an array of linear voltage displacement transducers, have been compared with measurements produced using a digital level. Encouraging results have been achieved and photogrammetry has been shown to be capable of producing a similar accuracy to the existing system. There are many advantages associated with a photogrammetric survey but attempts to establish a permanent, automated photogrammetric system for the rolling load facility at a reasonable cost have so far been unsuccessful. It is anticipated that, with the falling cost of high resolution digital sensors, such a system will soon be possible. 相似文献
205.
The common occurrence of olivine, clinopyroxene and plagioclase in natural basalts may suggest that crystallization of these
phases exerts important controls on the evolution of natural basalts at low pressure. In order to understand the effects of
such an assemblage on the evolution of basalt, an experimental study of the divariant assemblage 1+an+cpx+ol in the system
CMAS + FeO was undertaken at 1 bar and under very reducing conditions. Experiments have been performed along three isothernal
sections. Detailed electron microprobe data have been collected on all the coexisting phases. Combining these data with available
data in the system CMAS, the compositions of all the coexisting phases have been described as functions of temperature and
CaO content in the melt by applying a multiple linear regression method. This allows a quantitative characterization of the
divariant assemblage 1+an+epx+ol in the system CMAS + FeO, from 1275°C to 1160°C, with liquid compositions ranging from mg#=1
to mg#=0.28. Knowing the composition-temperature relationships, the basic T-X configuration of the assemblage 1+an+cpx+ol has been analysed, and mass balance calculations have been performed to examine
the FeO effect on different crystallization processes. Addition of FeO to the system CMAS transforms the thermal divide in
the assemblage 1+an+cpx+ol to a thermal ridge, and shifts the spine of the thermal ridge towards SiO2-poor compositions with decreasing temperature. This indicates that tholeiitic basalts can be relatively silica-poor, and
evolve towards slightly more silica-poor compositions. With increasing FeO content, pigeonite replaces ortheonstatite as a
crystallizing phase along the silica-rich boundary of the assemblage 1+an+cpx+ol. In some iron, and silica rich composition,
olivine possibly terminates its crystallization or even starts resorption prior to pigeonite precipitation; this suppresses
silica enrichment in the melt. Crystallization paths of the assemblage 1+an+cpx+ol are determined by the detailed T-X relations of the thermal ridge with the melt evolving away from the spine. The liquid evolution trend depends strongly on
the initial compositions. A tholeiitic liquid can follow a moderate silica enrichment path at the same very reducing condition
of there is a high modal proportion of olivine. ‘A Fenner mechanism therefore is at work at the same place as a Bowen mechanism’. 相似文献
206.
Guy P.F. Steed 《Geoforum》1978,9(1):35-47
Recent rapid changes in comparative advantage have led to serious stresses through market disruption of the industries of many developed countries. The paper views the global industrial geography of the clothing industries as a form of adaptive, purposeful system in which governments respond to stress through the negotiation of “voluntary” export restraints, reversion to “escape clauses” or safeguards offering protection, or the application of adjustment assistance. It contrasts the stresses and mechanisms of adjustment of the Netherlands, West Germany, Sweden, the United States and Japan. 相似文献
207.
Eucrites are extraterrestrial plagioclase-pigeonite basalts. Experimental studies suggest that they were produced by partial melting of an olivine (Fo65)-pigeonite (Wo5En65)-plagioclase (An94)-spinel-metal source region. Quantitative modeling of the evolution of REE abundances in the eucrites indicates that the main group of eucrites (e.g. Juvinas) may be produced by approximately 10% equilibrium partial melting of a source region with initial REE abundances which were chondritic relative and absolute. Other eucrites appear to represent greater (e.g. Sioux County—15%) or smaller (e.g. Stannern—4%) degrees of melting. Moore County and Serra de Magé appear to be cumulates of pyroxene and plagioclase produced by fractional crystallization of a Juvinas-like melt. Nuevo Laredo may represent a residual liquid after such fractional crystallization. Our calculations are consistent with the conclusion that the eucrites were derived from a single type of source region. The close correspondence of the age of the eucrites (? 4.6 AE) to the age of the solar system appears to preclude the possibility of extensive chemical differentiation of the eucrite parent body prior to the event which produced the eucritic melts. Thus our calculations have yielded not only the mode of the source region but, assuming homogeneous accretion, the mode and hence the bulk composition of the eucrite parent body as well. We are unable to estimate quantitatively the ratio of metal to olivine in the parent body. If no metal is present, the bulk composition (in oxide wt%) is Na2O—0.04, MgO—29.7, Al2O3—1.8, SiO2—39.0, CaO—1.2, FeO—28.3. If, in contrast, the parent body contained 30% metal, the bulk composition of the silicate portion of the eucrite parent body is Na2O—0.06, MgO—28.0, Al2O3—2.6, SiO2—41.3, CaO—1.9, FeO—26.3. Relative abundances of the meteorites suggest that the eucrite parent body is still intact. The solar system object most closely resembling the eucrites is asteroid 4 Vesta. Because Vesta is unique among the asteroids, we have license to conclude that it is the source of the eucrites and its bulk composition is close to the analyses given above. 相似文献
208.
The heating of cholestanol 2a with kaolinite (140°C, 16 hr) mainly leads to a mixture of steranes (40%) and sterenes (35%). The major compounds which are formed have been identified as 5α(H)- and 5β(H)-cholestanes, 4a and 4b, the diacholestenes, 5, the diacholestanes, 6, and the D-homodiacholestanes 7. With the exception of the latter, these compounds have all been observed previously in ancient sediments and crude oils. Several of these compounds are identical or bear structural similarities with those obtained from cholestanol at low temperature in acidic or superacidic conditions. The comparison with the results obtained using other minerals (montmorillonite, talc, alumina, polyphos-phate-treated montmorillonite) shows that the observed transformations are catalysed by superacid sites which are present in kaolinite and montmorillonite. 相似文献
209.
Shore-protection structures—largely groins and seawalls—have increased in number along the 300-km-long mainland Ohio shore
of Lake Erie from about 60 in 1876–77, to about 1,400 in the late 1930s, to about 3,600 in the mid 1970s. Recession rates,
on the other hand, have decreased from the early period (1876–1877 to the late 1930s) to the later period (late 1930s to 1973).
Forexample, the length of shore that receded at the intermediate rate (0.3 to 0.9 m/yr) decreased from 76 to 54 km and the
length of shore that receded at the lowest rate (less than 0.3 m/yr) increased from 151 to 171 km. Beach widths also have
decreased; the length of shore fronted by wide (greater than 15 m) beaches decreased from 64 km to 35 km between 1876–1877
and 1968. Furthermore, the length of shore without a beach increased from 84 km in 1876–1877 to 112 km in 1968. The decreases
in recession rates have been caused by the shore-protection structures, which have directly armored the shore from waves (seawalls)
or reduced the wave energy reaching the shore by trapping sand (groins). Moreoever, because the shore is a major source of
sand for the beaches, the decrease in recession has led to a reduced sand supply and narrower beaches. Ironically, by protecting
the shore, the structures apparently have more than compensated for the loss of the best natural form of shore protection,
beach sand. 相似文献
210.
The mathematical equivalence of several equations used to calculate the evolution of trace element abundances during equilibrium partial melting is demonstrated. 相似文献