全文获取类型
收费全文 | 729篇 |
免费 | 37篇 |
国内免费 | 9篇 |
专业分类
测绘学 | 21篇 |
大气科学 | 44篇 |
地球物理 | 212篇 |
地质学 | 289篇 |
海洋学 | 82篇 |
天文学 | 89篇 |
综合类 | 1篇 |
自然地理 | 37篇 |
出版年
2023年 | 3篇 |
2022年 | 16篇 |
2021年 | 20篇 |
2020年 | 32篇 |
2019年 | 21篇 |
2018年 | 38篇 |
2017年 | 30篇 |
2016年 | 42篇 |
2015年 | 23篇 |
2014年 | 39篇 |
2013年 | 56篇 |
2012年 | 33篇 |
2011年 | 47篇 |
2010年 | 47篇 |
2009年 | 53篇 |
2008年 | 43篇 |
2007年 | 27篇 |
2006年 | 30篇 |
2005年 | 23篇 |
2004年 | 26篇 |
2003年 | 13篇 |
2002年 | 14篇 |
2001年 | 10篇 |
2000年 | 6篇 |
1999年 | 9篇 |
1998年 | 8篇 |
1996年 | 7篇 |
1995年 | 2篇 |
1994年 | 6篇 |
1993年 | 2篇 |
1992年 | 5篇 |
1991年 | 3篇 |
1990年 | 5篇 |
1989年 | 4篇 |
1988年 | 3篇 |
1987年 | 1篇 |
1986年 | 1篇 |
1985年 | 1篇 |
1984年 | 1篇 |
1983年 | 1篇 |
1981年 | 2篇 |
1980年 | 1篇 |
1979年 | 2篇 |
1978年 | 4篇 |
1977年 | 2篇 |
1976年 | 2篇 |
1975年 | 1篇 |
1974年 | 5篇 |
1973年 | 2篇 |
1970年 | 1篇 |
排序方式: 共有775条查询结果,搜索用时 31 毫秒
251.
Willem Viveen Jorge Sanjurjo-Sanchez Ana Goy-Diz Antonie Veldkamp Jeroen M. Schoorl 《Quaternary Research》2014
A 15-m-thick, fluvial sedimentary record of the NW Iberian lower Miño River was studied. Grain-size analyses were performed and twelve samples were dated using optically stimulated luminescence dating techniques, documenting a 1300-yr-old reconstructed fluvial record that does not match with known climate fluctuations in the area, but is linked instead to the construction of a series of ancient fishing weirs (pesqueiras). The sedimentation phases are in agreement with known episodes of increased population density, which suggests active use of the pesqueiras. A number of sedimentation hiatuses in the fluvial record point towards damage to the pesqueiras during large-scale flooding in the Miño River basin, and a sudden drop in population probably due to the arrival of the plague in the 13th century AD. The oldest sedimentation phases started just after 700 AD, and we infer that the first pesqueiras were constructed around this time. This timing coincides with the transition of the NW Iberian landscape towards a more intensively used agricultural landscape, as evidenced from other geo-archeological investigations. The results demonstrate that the pesqueiras are several hundreds of years older than known from historical records, but not so old as to date back to the Roman occupation. 相似文献
252.
Hardage Kyle Street Joseph Herrera-Silveira Jorge A. Oberle Ferdinand K. J. Paytan Adina 《Journal of Paleolimnology》2022,67(2):131-162
Journal of Paleolimnology - Epikarst estuary response to hydroclimate change remains poorly understood, despite the well-studied link between climate and karst groundwater aquifers. The influence... 相似文献
253.
254.
Eugenio Aragón Lucio Pinotti Fernando D’Eramo Antonio Castro Osvaldo Rabbia Jorge Coniglio Manuel Demartis Irene Hernando Claudia E.Cavarozzi Yolanda E.Aguilera 《地学前缘(英文版)》2013,4(4):377-388
The collision of a divergent ocean ridge may evolve into two end cases:in the continuity of ocean-floor subduction.or in the detachment of the subducted plate.The northern Patagonia active plate margin has the unique situation that in Cenozoic time it has been subjected to two divergent ridge collisions,each one representing one of the end members.The Neogene Antarctica-Nazca divergent ridge collision evolved as a continuous ocean-floor subduction system,promoting a magmatic hiatus at the arc axis,the obduction of part of the ridge ocean-floor in the fore-arc.and basaltic volcanism in the back-arc.In contrast,the Paleogene Farallon-Aluk divergent ridge collision evolved into a transform margin,with the detachment and sinking of the Aluk plate and the development of a large slab window.As in the previous case,this collision promoted a magmatic hiatus at the arc axis,but the tectono-magmatic scenario changed to postorogenic synextensional volcanism that spread to the former fore-arc(basalt,andesite,rhyolite) and former back-arc(bimodal ignimbrite flare-up,basalt).Geochemistry of this slab window synextensional volcanism shows more MORB-like basalts towards the former fore-arc,and MORB-OIB-like basalts towards the former back-arc.Instead,an isolated undeformable crustal block in the former back-arc,with an "epeirogenic" response to the slab window and extensional regime,was covered by OIB-type basalts after uplift.Major elements show that slab window basalts reach TiCh values up to 3 wt%,as compared with the top value of 1.5 wt%of arc magmas.Besides,the MgO with respect to(FeOt + Al2O3) ratio helps to distinguish slab window magma changes from the former fore-arc to the former back-arc and also with respect to the "epeirogenic" block.Higher contents of HFS elements such as Nb and Ta also help to distinguish this slab window from arc magmas and also,to distinguish slab window magma changes from the former fore-arc to the former back-arc and "epeirogenic" block settings.The isotope compositions of slab window magmatism show a disparate coeval array from MORB to crustal sources,interpreted as a consequence of the lack of protracted storage and homogenization due to the extensional setting. 相似文献
255.
Jorge L. Pousa Enrique E. D’Onofrio Mónica M. E. Fiore Eduardo E. Kruse 《Environmental Earth Sciences》2013,68(8):2325-2335
The Argentine shore of the Rio de la Plata estuary and its southwards adjacent maritime front are normally affected by extratropical positive and negative storm surges that affect human activities seriously. Positive surges can raise the water level in the estuary by more than 3 m over the predicted tide; thus, flooding the coastal plain where over 13 million people live and causing extensive property damage. Sometimes, there has been loss of life too. Although less populated than the coastal plain, the maritime front has many important tourist resorts and also undergoes severe beach erosion processes and loss of property owing to positive surges. Negative surges are particularly troublesome in the Rio de la Plata because they critically affect navigation safety and drinking water supply by lowering the predicted water level in an amount that sometimes reached more than 4 m. A remarkable point is that the same storm event can simultaneously give rise to a positive surge on the maritime front and a negative one in the Rio de la Plata. The environmental impacts of positive storm surges are strongly aggravated by human intervention. At the same time, sea level rise due to global climatic change has also its influence. 相似文献
256.
Teresita Betancur Carlos Palacio Jorge Ignacio Gaviria María Rueda 《Environmental Earth Sciences》2013,70(1):315-328
Interaction between vulnerability and contaminating charge was used in order to determine the groundwater contamination danger. The result of danger being adapted to the scale of impact on human or animal health and ecosystems is known as “risk”. Index and overlapping methodologies such as EPNNA, DRASTIC, SINTACS, GOD AVI, and Ekv were used and compared to evaluate vulnerability. Contaminating charge to the subsoil, which is generated from specific human activity, has four characteristics: kind of contaminant, means of disposal, intensity, and duration. Interaction among these characteristics obtains a Contaminating Charge Index. In the Bajo Cauca Antioqueño region, over 150,000 inhabitants require ground water for meeting their basic needs at home, for cattle breeding activities, and for irrigation. For this region, an assessment of the groundwater contamination of the free aquifer, as well as an estimation of its impact and the danger this contamination may pose to ecosystems or communities has been performed. Analysis of the interaction between vulnerability and threat allows for the creation of danger and risk maps. 相似文献
257.
Wytler Cordeiro dos Santos 《Astrophysics and Space Science》2011,331(1):295-307
The Laser Interferometer Space Antenna (LISA) mission will use advanced technologies to achieve its science goals: the direct
detection of gravitational waves, the observation of signals from compact (small and dense) stars as they spiral into black
holes, the study of the role of massive black holes in galaxy evolution, the search for gravitational wave emission from the
early Universe. The gravitational red-shift, the advance of the perihelion of Mercury, deflection of light and the time delay
of radar signals are the classical tests in the first order of General Relativity (GR). However, LISA can possibly test Einstein’s
theories in the second order and perhaps, it will show some particular feature of non-linearity of gravitational interaction.
In the present work we are seeking a method to construct theoretical templates that limit in the first order the tensorial
structure of some metric fields, thus the non-linear terms are given by exponential functions of gravitational strength. The
Newtonian limit obtained here, in the first order, is equivalent to GR. 相似文献
258.
E. Aprile K. Arisaka F. Arneodo A. Askin L. Baudis A. Behrens K. Bokeloh E. Brown J.M.R. Cardoso B. Choi D. Cline S. Fattori A.D. Ferella K.L. Giboni A. Kish C.W. Lam J. Lamblin R.F. Lang K.E. Lim J.A.M. Lopes T. Marrodán Undagoitia Y. Mei A.J. Melgarejo Fernandez K. Ni U. Oberlack S.E.A. Orrigo E. Pantic G. Plante A.C.C. Ribeiro R. Santorelli J.M.F. dos Santos M. Schumann P. Shagin A. Teymourian D. Thers E. Tziaferi H. Wang C. Weinheimer M. LaubensteinS. Nisi 《Astroparticle Physics》2011,35(2):43-49
Results of the extensive radioactivity screening campaign to identify materials for the construction of XENON100 are reported. This dark matter search experiment is operated underground at Laboratori Nazionali del Gran Sasso (LNGS), Italy. Several ultra sensitive High Purity Germanium detectors (HPGe) have been used for gamma ray spectrometry. Mass spectrometry has been applied for a few low mass plastic samples. Detailed tables with the radioactive contaminations of all screened samples are presented, together with the implications for XENON100. 相似文献
259.
Edmond Giraud Jorge Melnick Hernan Quintana Fernando Selman Ignacio Toledo Paula Zelaya 《中国天文和天体物理学报》2011,11(3)
We present galactic spectroscopic data from a pencil beam of 10.75×7.5 centered on the X-ray cluster RXJ0054.0-2823 at z=0.29.We study the spectral evolution of galaxies from z=1 down to the cluster redshift in a magnitude-limited sample at R≤23,for which the statistical properties of the sample are well understood.We divide emission-line galaxies into star-forming galaxies,Low Ionization Nuclear Emission line Regions(LINERs) ,and Seyferts by using emission-line ratios of[OII],Hβ,and[OIII],and derive stella... 相似文献
260.
M. E. Zucolotto L. L. Antonello M. E. Varela R. B. Scorzelli Isabel P. Ludka P. Munayco E. dos Santos 《Earth, Moon, and Planets》2012,108(2):139-150
The new Brazilian chondrite, Lavras do Sul, was found in 1985 at Lavras do Sul, Rio Grande do Sul State-Brazil (33°30′48″S; 53°54′65″W). It consists of a single mass weighing about 1 kg, covered by a black fusion crust with grayish interior. Four polished thin sections were prepared from a slice weighing 67 g on deposit at the Museu Nacional/UFRJ. It consists mostly of chondrules and chondrule fragments dispersed in a recrystallized matrix. Most chondrules are poorly defined and range in size from 300 to 2,000 μm, although some of them show distinct outlines, particularly when viewed under cross-polarized transmitted and reflected light. The texture of chondrules varies from non-porphyritic (e.g., barred-olivine, radial-pyroxene) to porphyritic ones (e.g., granular olivine as well as olivine-pyroxene). The meteorite contains mainly olivine (Fa24.9), low-Ca pyroxene (Fs22.6) and metal phases, with minor amounts of plagioclase, chromite and magnetite. Mössbauer Spectroscopy studies indicate that the metal phase is kamacite, tetrataenite and antitaenite. Veins of secondary iddingsite crosscut the thin section and some ferromagnesian silicates. The chemical composition indicates that Lavras do Sul is a member of the low iron L chondrite group. The poorly delineated chondritic texture with few well-defined chondrules, the occurrence of rare clinopyroxene and plagioclase (and maskelynite) with apparent diameters ranging from 5 to 123 μm led us to classify Lavras do Sul as an equilibrated petrologic type 5. The shock features of some minerals suggest a shock stage S3, and the presence of a small amount of secondary minerals such as iddingsite and goethite, a degree of weathering W1. The meteorite name was approved by the Nomenclature Committee (Nom Com) of the Meteoritical Society (Meteoritic Bulletin Nº99). 相似文献