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181.
Rudolph Scherreiks Dan Bosence Marcelle BouDagher-Fadel Guillermo Meléndez Peter O. Baumgartner 《International Journal of Earth Sciences》2010,99(6):1317-1334
The Late Triassic and Jurassic platform and the oceanic complexes in Evvoia, Greece, share a complementary plate-tectonic
evolution. Shallow marine carbonate deposition responded to changing rates of subsidence and uplift, whilst the adjacent ocean
underwent spreading, and then convergence, collision and finally obduction over the platform complex. Late Triassic ocean
spreading correlated with platform subsidence and the formation of a long-persisting peritidal passive-margin platform. Incipient
drowning occurred from the Sinemurian to the late Middle Jurassic. This subsidence correlated with intra-oceanic subduction
and plate convergence that led to supra-subduction calc-alkaline magmatism and the formation of a primitive volcanic arc.
During the Middle Jurassic, plate collision caused arc uplift above the carbonate compensation depth (CCD) in the oceanic
realm, and related thrust-faulting, on the platform, led to sub-aerial exposures. Patch-reefs developed there during the Late
Oxfordian to Kimmeridgian. Advanced oceanic nappe-loading caused platform drowning below the CCD during the Tithonian, which
is documented by intercalations of reefal turbidites with non-carbonate radiolarites. Radiolarites and bypass-turbidites,
consisting of siliciclastic greywacke, terminate the platform succession beneath the emplaced oceanic nappe during late Tithonian
to Valanginian time. 相似文献
182.
Marcos García-Arias Luis Guillermo Corretgé Antonio Castro 《Mineralogy and Petrology》2010,99(3-4):153-164
Melting experiments on a gneissic protolith using the diamond trap technique produced an accumulation of crystals of biotite in the boundary of the diamond trap. Several hypotheses can be inferred to explain this feature, but textural evidence and calculations of the settling and drag velocities of the crystals suggest a model of extraction of melt due to a pressure gradient inside the capsule as the most likely origin of this biotite layer. This biotite layer and the trapped melt resemble the melanosome and leucosome, respectively, of stromatic metatexite migmatites. The melt extraction model developed is similar to the “filter pressing” model for migmatite formation. The diamond trap technique is a suitable method to develop migmatites experimentally. 相似文献
183.
Guillermo Gonzalez 《Monthly notices of the Royal Astronomical Society》1999,308(2):447-458
The chemical-dynamical properties of stars with giant planets are compared to those of a nearby star sample within the framework of a stellar orbital diffusion model. The stars-with-planets sample includes recently discovered extrasolar planets and the Sun. We find that the planet-bearing stars, 14 Her, ρ 1 Cnc and τ Boo, are much more metal-rich than stars of similar age and this cannot be easily explained by orbital diffusion. We also confirm previous claims that the motion of the Sun relative to the local standard of rest is very small compared to other G dwarfs of similar age, and we offer a possible explanation for this apparent anomaly. 相似文献
184.
George Wallerstein † Sean Matt† Guillermo Gonzalez† 《Monthly notices of the Royal Astronomical Society》2000,311(2):414-422
We have used echelle spectra of resolving power 35 000 to derive chemical abundances and the 12 C/13 C ratio in the 1.9-d carbon Cepheid RT TrA and the Cepheid U TrA, employed as a comparison star. We confirm that RT TrA is very metal-rich with [Fe/H]=+0.4. In addition, C and N are substantially in excess, and a small deficiency in O is present. We interpret these anomalies as resulting from the appearance on the stellar surface of material enriched in 12 C by the 3- α process, followed by CNO cycling to convert 12 C to 13 C and 14 N. In addition, some 16 O has been processed to 14 N. The partial processing of 16 O to 14 N indicates that substantial 17 O may be present. Proton capture seems to have enhanced 23 Na from the Ne isotopes. 相似文献
185.
Guillermo Aravena Fernando Villate Ibon Uriarte Arantza Iriarte Berta Ibez 《Estuarine, Coastal and Shelf Science》2009,83(4):621-628
The effect of environmental factors (river discharge, water temperature and dissolved oxygen saturation) on the abundance and distribution of Acartia populations and the interactions between their congenerics was evaluated by means of transfer function (TF) models in the estuary of Bilbao during the period 1998–2005. The recorded species were Acartia clausi, Acartia tonsa, Acartia margalefi and Acartia discaudata. Acartia clausi dominated in the entire euhaline region of this estuary until 2003 when it was displaced from the inner part by A. tonsa. This invasive species (A. tonsa) was found for the first time in 2001 and colonized successfully the inner (salinity 30) and intermediate (salinity 33) waters of this estuary since 2003. The TF models revealed an immediate and negative effect of A. tonsa on A. clausi in the intermediate salinity (33) waters, where these species showed the highest spatial overlap. The results indicate that environmental changes from 2003 influenced the abundance of Acartia species, being unfavourable for A. clausi. The decrease of A. clausi abundance in low salinity waters was related to a significant decrease of dissolved oxygen saturation levels, whereas the increase of temperature was linked to a significant increase of A. tonsa. Acartia margalefi and A. discaudata were scarce over the entire period, but they were found to be valuable indicators of hydrological changes, which were associated to climate factors. These two latter species increased in abundance and expanded their seasonal distribution, and in the case of A. margalefi also its spatial distribution, in 2002, coinciding with the period in the time-series when autumn–winter rainfall and summer temperatures were lowest, and dissolved oxygen saturation levels were highest. 相似文献
186.
Mayra C. Robles-Montes Guillermo Martínez-Flores Michael K. Faught Enrique H. Nava-Sánchez 《Geoarchaeology》2024,39(2):106-121
When the first Americans inhabited the area now known as Isla Espiritu Santo, around 12.5 and 6 ka, the sea level continuously rose. This resulted in the loss of the coastal territory and the retreat of the human population further inland. Part of the archaeological evidence of this period currently lies over the seafloor and under the seabed. Therefore, reconstructing paleoshorelines is a necessary first step toward submerged precontact archaeology and a broad understanding of the spatial context in which those human populations interacted and how the landscapes changed. Isla Espiritu Santo is of prehistoric importance as it contains numerous Paleocoastal tradition sites as early as ~12,400 Cal B.P. This research aims to reconstruct the changing shoreline positions as sea levels rose around Isla Espiritu Santo between 12.5 and 6.5 ka. We apply numerical modeling to map digital elevation models at 1 ka intervals by estimating the changes in the morphology of the seafloor according to the deposition rates and global sea-level curve. The results show the evolution of coastal morphology and paleoshoreline's position. Three primary geoforms are proposed: (1) coastal plains, (2) tombolo, and (3) a coastal lagoon–island barrier system. This also offers insights into the physical aspect of submerged prehistoric landscapes and the possible resource exploitation options of early societies. In this research, the reconstruction of submerged landscapes seeks to contribute to the long-term goal of locating submerged precontact sites. 相似文献