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501.
The structural role played by masonry infills on RC building performances after the 2011 Lorca,Spain, earthquake 总被引:3,自引:3,他引:0
Flavia De Luca Gerardo M. Verderame Fernando Gómez-Martínez Agustín Pérez-García 《Bulletin of Earthquake Engineering》2014,12(5):1999-2026
On May 11, 2011 an earthquake of magnitude 5.1 ( \(M_{w}\) ) struck Murcia region causing nine casualties and damage to buildings and infrastructures. Even if the main characteristics of the event would classify it as a moderate earthquake, the maximum Peak Ground Acceleration (PGA) registered (equal to 0.37 g) exceeded significantly local code provisions in terms of hazard at the site. This high PGA was a result of directivity effects in the near source region. An overview of earthquake characteristics and damage observed is provided. Notwithstanding the lack of proper structural design characterizing building stock in the area, most of the losses were caused by non-structural damage. According to in field observations, it emerges that masonry infills provided additional, “not designed”, strength to reinforced concrete (RC) buildings. Observed damage data, collected after the earthquake, are shown and compared to the results of a simplified approach for nonstructural damage assessment of RC infilled structures (FAST vulnerability approach). The latter comparison provided a fair accordance between observed data and analytical results. 相似文献
502.
503.
Alessandro Patruno Luca Zampieri 《Monthly notices of the Royal Astronomical Society》2008,386(1):543-552
We present evolutionary tracks of binary systems with high-mass companion stars and stellar-through-intermediate mass black holes (BHs). Using Eggleton's stellar evolution code, we compute the luminosity produced by accretion from the donor during its entire evolution. We compute also the evolution of the optical luminosity and colours of the binary system taking the disc contribution and irradiation effects into account. The calculations presented here can be used to constrain the properties of the donor stars in ultraluminous X-ray sources by comparing their position on the Hertzsprung–Russell or colour–magnitude diagrams with the evolutionary tracks of massive BH binaries. This approach may actually provide interesting clues also on the properties of the binary system itself, including the BH mass. We found that, on the basis of their position on the colour–magnitude diagram, some of the candidate counterparts considered can be ruled out and more stringent constraints can be applied to the donor masses. 相似文献
504.
We prove the existence of infinitely many periodic solutions, with larger and larger minimal period, accumulating onto elliptic
invariant tori for (an “outer solar-system” model of) the planar (N + 1)-body problem.
相似文献
505.
GPS measurements were collected within the framework of the VLNDEF (Victoria Land Network for DEFormation control) project, which was started in 1999 with the aim of detecting crustal deformation in Northern Victoria Land (Antarctica). The network was established in 1999 and is composed of one permanent station (TNB1), which has been observing since 1998, and 28 periodically surveyed control points. Three complete campaigns and some partial surveying of the network have been carried out to date.Data processing and analysis have been performed using an undifferenced approach for the network position within the ITRF. A double-differences-based strategy has been applied for movement detection. The data processing and analysis of results have been carried out for all available data, both periodically acquired and long time series.GPS measurements collected between December 1999 and February 2006 indicate a mean “absolute” motion of the region of ve = 11.3 mm/yr and vn = − 11.1 mm/yr and rock uplift rates of vu = 2.8 mm/yr. These values are consistent with Antarctic plate motion and the general postglacial rebound models of the region. The relative motions within VLNDEF are small and only few points show velocities greater than the confidence levels. 相似文献
506.
Antonio Emolo Matteo Picozzi Gaetano Festa Claudio Martino Simona Colombelli Alessandro Caruso Luca Elia Aldo Zollo Piero Brondi Nicola Miranda 《Bulletin of Earthquake Engineering》2016,14(9):2513-2529
We present the results of a feasibility study of an earthquake early warning system (EEWS) for the Campania region (southern Italy) using schools as specific targets. The study considered the seismogenic zones as sources of potential earthquakes for the area, the Italian accelerometric network as the recording network for seismic event occurrence, and the performances of the software platform PRESTo Plus for data analysis and processing. We analyze the distribution of lead-times for all possible threatening seismic sources for each municipality in the region under study by extracting the lead-time value corresponding to the 5th, 10th and 25th percentiles of the distributions. We discuss the results for the 5th percentile in order to analyze the worst-case scenario: in the case of a single site, the lead-time is expected to be larger than this value in the 95 % of the cases. Since the population distribution in Campania is uneven and most of the people live nearby the coast, whilst the most destructive earthquakes occur along the Apennine chain, we can conclude that an efficient EEWS can allow most of the schools in the area to undertake some mitigating actions. The testing of the EEWS was carried out in the high school ITIS ‘E. Majorana’, located at Somma Vesuviana, about 80 km from the seismogenic Irpinia region. For this purpose, the Sentinel, an actuator made up of low-cost hardware (i.e., Arduino®), was developed in close cooperation with students and teachers of the school to receive alert messages from the PRESTo Plus platform and warn the school users in case of a seismic event. The EEWS and the Sentinel were successfully tested during some blind drills performed during normal school activities. 相似文献
507.
508.
The ShakeMap software automatically generates maps of the peak ground motion parameters (shakemaps) and of instrumental intensity
soon after an earthquake. Recorded data are fundamental to obtaining accurate results. In case observations are not available,
ShakeMap relies on ground motion predictive equations, but due to unmodelled site conditions or finite fault effects, large
uncertainties may appear, mainly in the near-source area where damage is relevant. In this paper, we aim to account for source
effects in ShakeMap by computing synthetics to be used for integrating observations and ground motion predictive equations
when near-source data are not available. To be effective, the computation of synthetics, as well as of the finite fault, should
be done in near real time. Therefore, we computed rapid synthetic seismograms, by a stochastic approach, including the main
fault features that were obtained through inversion of regional and teleseismic data. The rapidity of calculation is linked
to a number of assumptions, and simplifications that need testing before the procedure can run in automatic mode. To assess
the performance of our procedure, we performed a retrospective validation analysis considered as case study of the M
w = 6.3 earthquake, which occurred in central Italy on April 6, 2009. In that case, the first shakemaps, generated a few minutes
after the earthquake, suffered large uncertainties on ground motion estimates in an area closer to the epicenter due to the
lack of near-field data. To verify our approach, we recomputed shakemaps for the L’Aquila earthquake, integrating data available
soon after the earthquake at different elapse times with synthetics, and we compared our shaking map with the final shakemap,
obtained when all the data were available. Our analysis evidences that (1) when near-source data are missing, the integration
of real data with synthetics reduces discrepancies between computed and actual ground shaking maps, mainly in the near-field
zone where the damage is relevant and (2) the approach that we adopted is promising in trying to reduce such discrepancies
and could be easily implemented in ShakeMap, but some a priori calibration is necessary before running in an automatic mode. 相似文献
509.
510.
This study analyses large wood (LW) storage and the associated effects on channel morphology and flow hydraulics in three third‐order mountain basins (drainage area 9–12 km2) covered in old‐growth Nothofagus forests, ranging from the temperate warm Chilean Andean Cordillera to the sub‐Antarctic Tierra del Fuego (Argentina). Amount, characteristics and dimensions of large wood (>10 cm diameter, >1 m long) were recorded, as well as their effects on stream morphology, hydraulics and sediment storage. Results show that major differences in LW abundance exist even between adjacent basins, as a result of different disturbance histories and basin dissection. Massive LW volumes (i.e. >1000 m3 ha?1) can be reached in basins disturbed by fires followed by mass movements and debris flows. Potential energy dissipation resulting from wood dams is about a quarter of the total elevation drop in two streams, with a gross sediment volume stored behind wood dams of around 1000 m3 km?1, which appears to be of the same order as the annual sediment yield. Finally, the presence of wood dams may increase flow resistance by up to one order of magnitude. Copyright © 2007 John Wiley & Sons, Ltd. 相似文献