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281.
Shannon E. Brown Jon S. Warland Eduardo A. Santos Claudia Wagner-Riddle Ralf Staebler Meaghan Wilton 《Boundary-Layer Meteorology》2013,147(1):83-102
Analytical Lagrangian equations capable of predicting concentration profiles from known source distributions offer the opportunity to calculate source/sink distributions through inverted forms of these equations. Inverse analytical Lagrangian equations provide a practical means of estimating source profiles using concentration and turbulence measurements. Uncertainty concerning estimates of the essentially immeasurable Lagrangian length scale ( ${\mathcal{L}}$ ), a key input, impedes the operational practicality of this method. The present study evaluates ${\mathcal{L}}$ within a corn canopy by using field measurements to constrain an analytical Lagrangian equation. Measurements of net CO2 flux, soil-to-atmosphere CO2 flux, and in-canopy profiles of CO2 concentration provided the information required to solve for ${\mathcal{L}}$ in a global optimization algorithm for 30-min time intervals. For days when the canopy was a strong CO2 sink, the optimization frequently located ${\mathcal{L}}$ profiles that follow a convex shape. A constrained optimization then fit the profile shape to a smooth sigmoidal equation. Inputting the optimized ${\mathcal{L}}$ profiles in the forward and inverse Lagrangian equations leads to strong correlations between measured and calculated concentrations and fluxes. Coefficients of the sigmoidal equation were specific to each 30-min period and did not scale with any measured variable. Plausible looking ${\mathcal{L}}$ profiles were associated with negative bulk Richardson number values. Once the canopy senesced, a simple eddy diffusivity profile sufficed to relate concentrations and sources in the analytical Lagrangian equations. 相似文献
282.
Impact‐related noncoaxial deformation in the Pułtusk H chondrite inferred from petrofabric analysis
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Agata Krzesińska Jérôme Gattacceca Jon M. Friedrich Pierre Rochette 《Meteoritics & planetary science》2015,50(3):401-417
Petrofabrics in chondrites have the potential to yield important information on the impact evolution of chondritic parent asteroids, but studies involving chondritic petrofabrics are scarce. We undertook an analysis of the Pu?tusk H chondrite regolith breccia. Measurements of anisotropy of magnetic susceptibility and quantitative tomographic examination of metal grains are presented here and the results are compared with petrographic observations. The major fabric elements are in Pu?tusk shear fractures cutting the light‐colored chondritic clasts as well as brittly and semibrittly deformed, cataclased fragments in dark matrix of regolith breccia. Cataclasis is accompanied by rotation of silicate grains and frictional melting. Fabric of metal grains in chondrite is well defined and coherently oriented over the breccia, both in the clasts and in the cataclastic matrix. Metal grains have prolate shapes and they are arranged into foliation plane and lineation direction, both of which are spatially related and kinematically compatible to shear‐dominated deformational features. We argue that the fabric of Pu?tusk was formed in response to impact‐related noncoaxial shear strain. Deformation promoted brittle cataclastic processes and shearing of silicates, and, simultaneously, allowed for ductile metal to develop foliation and lineation. We suggest that plastic flow is the most probable mechanism for the deformation of metal grains in the shear‐dominated strain field. The process led also to the formation of large metal nodules and bands in the dark matrix of breccia. 相似文献
283.
One of the major limitations of the classical ensemble Kalman filter (EnKF) is the assumption of a linear relationship between
the state vector and the observed data. Thus, the classical EnKF algorithm can suffer from poor performance when considering
highly non-linear and non-Gaussian likelihood models. In this paper, we have formulated the EnKF based on kernel-shrinkage
regression techniques. This approach makes it possible to handle highly non-linear likelihood models efficiently. Moreover,
a solution to the pre-image problem, essential in previously suggested EnKF schemes based on kernel methods, is not required.
Testing the suggested procedure on a simple, illustrative problem with a non-linear likelihood model, we were able to obtain
good results when the classical EnKF failed. 相似文献
284.
Randy L. Stotler Shaun K. Frape Humam Taha El Mugammar Craig Johnston Ian Judd-Henrey F. Edwin Harvey Robert Drimmie Jon Paul Jones 《Hydrogeology Journal》2011,19(1):101-115
The Waterloo Moraine is a stratigraphically complex system and is the major water supply to the cities of Kitchener and Waterloo in Ontario, Canada. Despite over 30?years of investigation, no attempt has been made to unify existing geochemical data into a single database. A composite view of the moraine geochemistry has been created using the available geochemical information, and a framework created for geochemical data synthesis of other similar flow systems. Regionally, fluid chemistry is highly heterogeneous, with large variations in both water type and total dissolved solids content. Locally, upper aquifer units are affected by nitrate and chloride from fertilizer and road salt. Typical upper-aquifer fluid chemistry is dominated by calcium, magnesium, and bicarbonate, a result of calcite and dolomite dissolution. Evidence also suggests that ion exchange and diffusion from tills and bedrock units accounts for some elevated sodium concentrations. Locally, hydraulic “windows??cross connect upper and lower aquifer units, which are typically separated by a clay till. Lower aquifer units are also affected by dedolomitization, mixing with bedrock water, and locally, upward diffusion of solutes from the bedrock aquifers. A map of areas where aquifer units are geochemically similar was constructed to highlight areas with potential hydraulic windows. 相似文献
285.
Daphne Cuvelier Pierre‐Marie Sarradin Jozée Sarrazin Ana Colaço Jon T. Copley Daniel Desbruyères Adrian G. Glover Ricardo Serrão Santos Paul A. Tyler 《Marine Ecology》2011,32(2):243-255
The Eiffel Tower edifice is situated in the Lucky Strike hydrothermal vent field at a mean depth of 1690 m on the Mid‐Atlantic Ridge (MAR). At this 11‐m‐high hydrothermal structure, different faunal assemblages, varying in visibly dominant species (mussels and shrimp), in mussel size and in density of mussel coverage, were sampled biologically and chemically. Temperature and sulphide (∑S) were measured on the different types of mussel‐based assemblages and on a shrimp‐dominated assemblage. Temperature was used as a proxy for calculating total concentrations of CH4. Based on the physico‐chemical measurements, two microhabitats were identified, corresponding to (i) a more variable habitat featuring the greatest fluctuations in environmental variables and (ii) a second, more stable, habitat. The highest temperature variability and the highest maximum recorded temperatures were found in the assemblages visibly inhabited by alvinocaridid shrimp and dense mussel beds of large Bathymodiolus azoricus, whereas the less variable habitats were inhabited by smaller‐sized mussels with increasing bare surface in between. Larger mussels appeared to consume more ∑S compared with smaller‐sized (<1 cm) individuals and thus had a greater influence on the local chemistry. In addition, the mussel size was shown to be significantly positively correlated to temperature and negatively to the richness of the associated macrofauna. The presence of microbial mats was not linked to specific environmental conditions, but had a negative effect on the presence and abundance of macro‐fauna, notably gastropods. Whereas some taxa or species are found in only one of the two microhabitats, others, such as polychaetes and Mirocaris shrimp, cross the different microhabitats. Temperature was proposed to be a more limiting factor in species distribution than ∑S. 相似文献
286.
Restoration of offshore marine habitats is a relatively new concept, with attempts in the European Union being largely instigated by requirements of various strategic directives. In this experiment, we investigate the practicality and effectiveness of gravel seeding, using a commercial aggregate dredging vessel, in order to recreate a gravel habitat. The experimental design consisted of a Treatment and Control site, both within an area of historic dredging characterised by an overburden of sand, and a gravel dominated Reference site. All sites were surveyed, using a combination of acoustic, camera and grab techniques, 2 months before, and then at 0, 12 and 22 months after the deposition of 4444 m3 of gravel dominated sediments within the Treatment site. Although financial and practical constraints limited replication of the Treatment to one area, and so precluded strong statistical conclusions, our results suggested that the technique was both practically feasible, and successful in terms of returning the physical and biological attributes at the Treatment site to a state more representative of gravelly substrata in the wider, un-impacted environment. 相似文献
287.
The Salmon industry in Norway includes three sectors, namely sea and river fishing for wild salmon, and salmon farming, or aquaculture. The three sectors provide different social, economic and cultural benefits to society, but also face many problems and challenges. They have different interests, practices, traditions and audiences, and are also administered by different authorities and regulated under varying management regimes and legislations. On the one hand, they complement each other in terms of product supply, employment creation and income; on the other hand, they face conflicts over management objectives and strategies. This paper provides an overview of the salmon sectors associated with their status, challenges and management regimes. It further analyzes their interests and conflicts over economic contribution and management. Finally, some potential solutions are suggested in an attempt to solve these conflicts. 相似文献
288.
Participation in the Indigenous visual arts sector provides one of few market opportunities for Indigenous Australians resident on remote Aboriginal lands. In this article we examine the economic factors that influence this market engagement as they relate to woodcarving in the Maningrida region of Arnhem Land. In particular, we look at the factors that affect participation, production and monetary returns using scan and focal sampling, resource accounting and sales data from the regional art centre. Artists were engaged in a range of activities of which art production was the prominent means of productive cash income generation. An artist's residence and also their language community were found to influence the amount of sculpture production undertaken, with artists residing on ‘country’ in the hinterland being more engaged in sculpture production than those living in the township of Maningrida. The annual income earned by an artist for carving was highly variable and a large proportion of woodcarvers also earned income from producing artwork in other media. Capital costs were relatively minor, with travel costs and labour the main input into carving production. Based on the average return for a single woodcarving, $160, we estimate the average hourly return to artists as between $12 and $14. Whilst this figure is relatively low and comparable to the Australian award wage for unskilled labour, the income earned from arts production makes an important contribution to people's livelihoods. 相似文献
289.
Michael W. Busch Steven J. Ostro Jon D. Giorgini Randy Rose Petr Pravec Stephen B. Broschart 《Icarus》2006,181(1):145-155
We estimate Asteroid 1992 SK's physical properties from delay-Doppler images and Doppler-only echo spectra obtained during March 22-27, 1999, at Goldstone and from optical lightcurves obtained during February-March 1999 at Ond?ejov Observatory. The images span only about 15° of sky motion and are not strong, but they place up to twenty 40 m by 160 m pixels on the asteroid and have complete rotational phase coverage. Our analysis establishes that the radar observations are confined to subradar latitudes between −20° and −40°. The echo spectra and optical lightcurves span ∼80° of sky motion, which provides important geometric leverage on the pole direction. The lightcurves are essential for accurate estimation of the asteroid's shape and spin state. We estimate the asteroid's period to be 7.3182±0.0003 h and its pole direction to be at ecliptic longitude, latitude=(99°±5°,−3°±5°). The asteroid is about 1.4 km in maximum extent and mildly asymmetric, with an elongation of about 1.5 and relatively subdued topography. The OC radar albedo is 0.11±0.02 and the SC/OC ratio is 0.34±0.05. The current orbital solution permits accurate identification of planetary close approaches during 826-2690. We use our model to predict salient characteristics of radar images and optical lightcurves obtainable during the asteroid's March 2006 approach. 相似文献
290.
Gordon T. Richards Scott M. Croom Scott F. Anderson Joss Bland-Hawthorn Brian J. Boyle Roberto De Propris Michael J. Drinkwater Xiaohui Fan James E. Gunn eljko Ivezi Sebastian Jester Jon Loveday Avery Meiksin Lance Miller Adam Myers Robert C. Nichol Phil J. Outram Kevin A. Pimbblet Isaac G. Roseboom Nic Ross Donald P. Schneider Tom Shanks Robert G. Sharp Chris Stoughton Michael A. Strauss Alexander S. Szalay Daniel E. Vanden Berk Donald G. York 《Monthly notices of the Royal Astronomical Society》2005,360(3):839-852