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31.
Pierfrancesco Burrato Maria Eliana Poli Paola Vannoli Adriano Zanferrari Roberto Basili Fabrizio Galadini 《Tectonophysics》2008,453(1-4):157
We present an overview of the seismogenic sources of northeastern Italy and western Slovenia, included in the last version of the Database of Individual Seismogenic Sources (DISS 3.0.2) and a new definition of the geometry of the Montello Source that will be included in the next release of the database. The seismogenic sources included in DISS are active faults capable of generating Mw > 5.5 earthquakes. We describe the method and the data used for their identification and characterization, discuss some implications for the seismic hazard and underline controversial points and open issues.In the Veneto–Friuli area (NE Italy), destructive earthquakes up to Mw 6.6 are generated by thrust faulting along N-dipping structures of the Eastern Southalpine Chain. Thrusting along the mountain front responds to about 2 mm/a of regional convergence, and it is associated with growing anticlines, tilted and uplifted Quaternary palaeolandsurfaces and forced drainage anomalies. In western Slovenia, dextral strike–slip faulting along the NW–SE trending structures of the Idrija Fault System dominates the seismic release. Activity and style of faulting are defined by recent earthquakes (e.g. the Ms 5.7, 1998 Bovec–Krn Mt. and the Mw 5.2, 2004 Kobarid earthquakes), while the related recent morphotectonic imprint is still a debated matter.We reinterpreted a large set of tectonic data and developed a segmentation model for the outermost Eastern Southalpine Chain thrust front. We also proposed the association of the four major shocks of the 1976 Friuli earthquake sequence with individual segments of three major thrust fronts. Although several sub-parallel active strike–slip strands exist in western Slovenia, we were able to positively identify only two segments of the Idrija Fault System. A comparison of the regional GPS velocity with long-term geological slip-rates of the seismogenic sources included in DISS shows that from a quarter to half of the deformation is absorbed along the external alignment of thrust faults in Veneto and western Friuli. The partitioning of the deformation in western Slovenia among the different strike–slip strands could not be quantified. 相似文献
32.
We describe texture, mineralogy and whole-rock composition of cognate monzonite sub-volcanic clasts within debris flow deposits
related to the 5000 years catastrophic phreatomagmatic eruption probably linked to the Sciara del Fuoco sector collapse. The
debris flows are at the top of accretionary lapilli-rich ash deposits overlying potassic (KS, shoshonites) lavas of the Neostromboli
period. The monzonites are inferred to be crystallized in situ, at low P, at the side walls and/or roof margins of a shallow magma chamber and to be cogenetic with the KS Neostromboli
extrusives. They can be considered "ideal orthocumulates" since they approximately retain a bulk liquid composition and possibly
represent "slowly cooled equivalents" of their KS shoshonite host rock. The "closure temperature" of final solidification
of the monzonite lithic suite was estimated through ternary-feldspar geothermobarometry, plagioclase–K-feldspar and K-feldspar–biotite
equilibria and is in the range of 750–790 °C with a maximum –logfO2 around 15.1–15.3. The estimated pressure of crystallization is <0.5 kbar. Potassic lavas and dikes, previously emplaced during
the Neostromboli period, also resemble the monzonites in both major trace elements and mineral chemistry. The cogenetic relationship
between KS Neostromboli extrusives and the monzonite host-rock magma from which the sub-volcanic clasts were derived is clear
evidence that a shallow magma chamber existed between the caldera collapse of the Vancori period and the Sciara del Fuoco
sector collapse (i.e. between 13 000 and 5000 years). The monzonite clasts were derived from crystallization at very shallow
depth (ca. 1 km) and strongly support the hypothesis of violent decompression of the shallow magmatic plumbing system during
the Sciara del Fuoco sector collapse. Climax of the regressive landslide event, with maximum disruption of the chamber walls,
took place during emplacement of the debris flows, i.e. during the late stage of the Neostromboli phreatomagmatic eruption.
Received: 15 September 1996 / Accepted: 5 May 1997 相似文献
33.
34.
Antimo Angelino Alberto Incoronato Patrizia Sarno 《Studia Geophysica et Geodaetica》1996,40(3):217-224
Summary Mean magnetisation directions from 6 lava flows of questionable historical age have been determined. The results, which are
based upon very stringent linearity criteria during demagnetisation, point out erroneous dating and the corresponding lavas
can be ascribed to medieval activity of Mount Etna, as already suggested for some of the investigated flows, covering a time
interval of some centuries around AD 1000. The site mean direction of AD 1536 historically dated lava flow agrees with a previous
study (Tanguy et al., 1985), while the site mean directions of AD 1566 and AD 1169/812 differ significantly from those reported
earlier. Neither AD 812 nor AD 1169 dating is consistent with the site mean direction of the related flow being compatible
with an emplacement age possibly a few decades before AD 1000. The 3 lava flows historically dated AD 1595 exhibit different
within site mean directions indicating that they cannot be referred to coeval activity of the volcano; the site mean direction
of one of the flows is compatible with an emplacement occurring very close to AD 1000. The resulting SVC is significantly
shifted eastwards with respect to that of previous study (Tanguy et al., 1985). However, its older part nearly overlaps the
medieval Vesuvius SVC relocated to Etna. This indicates that the strict linearity analysis carried out during demagnetisation
has allowed to clearly define the characteristic magnetisations of the investigated lava flows. The adopted procedure is appropriate
for performing successful magnetic stratigraphy surveys in volcanic areas. 相似文献
35.
Giulio Bigazzi Aldo Del Moro Patrizia Macera 《Contributions to Mineralogy and Petrology》1986,94(1):46-53
A development of De Paolo's mathematical procedure (1981) for magmatic AFC (Assimilation-Fractional Crystallization) processes is discussed with respect to both trace element and Sr isotopic ratio behaviours during the genesis and evolution of Adamello batholith (northern Italy). Resolution of a two equation-system (one relative to 87Sr/86Sr ratio variation in a magma generated by an AFC process, the other to its trace element content variations) gives the F (mass of magma at time t/mass of initial magma) and D (bulk partition coefficient) values, by which one can deduce the r (rate of assimilation/rate of crystallization) value during each step of magmatic evolution. This quantitative approach suggests that: 1) there was a common precursor magma for all the Adamello granitoids, with a Mg-rich tholeiitic composition; 2) each intrusive unit appears to have been generated by different extents of AFC; 3) the trace element distribution in the magma seems essentially influenced by mineral fractionation, rather than by the composition of the assimilated crustal material. 相似文献
36.
Lucas J. Stal Patrizia Albertano Birgitta Bergman Klaus von Brckel John R. Gallon Paul K. Hayes Kaarina Sivonen Anthony E. Walsby 《Continental Shelf Research》2003,23(17-19):1695
The blooms of cyanobacteria that develop each summer in the Baltic Sea are composed of two functional groups, namely the small-sized picocyanobacteria (Synechococcus sp.) and the larger, colony-forming, filamentous N2-fixing cyanobacteria. The former encompassed both red (phycoerythrin-rich) and blue-green (phycocyanin-rich) species. The majority of the picocyanobacteria measured less than 1 μm and this size fraction comprised as much as 80% of the total cyanobacterial biomass and contributed as much as 50% of the total primary production of a cyanobacterial bloom. The picocyanobacteria are incapable of fixing N2, do not possess gas vesicles and are not toxic. However, a small filamentous Pseudanabaena sp. that could potentially fix N2 was isolated from the picocyanobacteria fraction. The larger cyanobacteria may form surface scums because they possess gas vesicles that make them buoyant. Although their biomass was less than the picocyanobacteria, they therefore form the more conspicuous and nuisance-forming part of the bloom. The larger cyanobacteria were composed mainly of three different species: Nodularia spumigena, Aphanizomenon flos-aquae and Anabaena sp. These all belong to the heterocystous, N2-fixing cyanobacteria. N. spumigena and A. flos-aquae were the dominant species; only N. spumigena was toxic. Although individual Nodularia filaments showed a range of different phenotypes, they all belong to one species as judged from 16S rDNA sequencing. Through determination of the genotypes of many individual Nodularia filaments, it was shown that this population was not clonal and that horizontal exchange of genetic information occurs. N. spumigena and A. flos-aquae were different with respect to their photosynthetic and N2-fixing potentials. Depending on prevailing environmental conditions, these differences would promote the proliferation of one species over the other and hence would determine overall the toxicity of a bloom. Daily integrals of photon irradiance rather than temperature determined the onset of bloom formation. During a bloom, the diazotrophic cyanobacteria fixed N2 at a rate that was 10–20% in excess of their own demand for N. Picocyanobacteria assimilated most of this excess N as shown by 15N incorporation. During bloom conditions, the diazotrophic cyanobacteria met about 50% of the N demand of the total cyanobacterial community. The picocyanobacteria were predominantly N-limited while the diazotrophic cyanobacteria were probably iron limited. These findings allow us to understand the formation of toxic cyanobacterial blooms and also to develop tools to predict bloom formation. 相似文献
37.
Nicola La Palombara Patrizia Caraveo Roberto Mignani Evanthia Hatziminaoglou Giovanni F. Bignami Mischa Schirmer 《Astrophysics and Space Science》2005,297(1-4):335-344
Most counterparts of the identified low-latitude γ-ray sources are isolated neutron stars (INSs). Since INSs are characterized by an extremely high value of f
X/f
opt, a systematic X-ray/optical coverage of the fields of unidentified low-latitude γ-ray sources is the best way to unveil INS
counterparts of unidentified sources. Since the low-latitude sources are heavily affected by the interstellar absorption in
both the X-ray and optical bands, we decided to apply the above strategy to two middle-latitude EGRET sources, which could belong to a local galactic population: 3EG J0616-3310 and 3EG J1249-8330. Here we report on the global
X-ray characterization of about 300 objects, on their candidate optical counterparts and on the preliminary results of their
identification. 相似文献
38.
Marina Manca Claudio Ramoni Patrizia Comoli 《Aquatic Sciences - Research Across Boundaries》2000,62(2):142-153
We reconstruct the impact of different environmental cues on Daphnia seasonal dynamics by means of an analysis of demographic and reproductive parameters, as well as of the size structure of the population. Data from 1996, indicative of the most recent productivity of the lake, with those from 1973, when the lake was meso-eutrophic, allow a discussion of the relevance of the observed changes for the structure of the pelagic food web of Lago Maggiore. Daphnia summer dynamics is mainly controlled by Bythotrephes longimanus. This is quite a different situation from that of the past, when Leptodora kindtii was the prevalent predatory cladocera. The size structure of Daphnia population revealed a depletion of small ovigerous females with increases in the predator. Our data allow a discussion of the idea, recently proposed, of Bythotrephes longimanus as a visual sit- and -wait predator. 相似文献
39.
40.
E. Virgilli F. Frontera P. Rosati E. Bonnini E. Buffagni C. Ferrari J. B. Stephen E. Caroli N. Auricchio A. Basili S. Silvestri 《Experimental Astronomy》2016,41(1-2):307-326
We report on results of observation of the focusing effect from the planes (220) of Gallium Arsenide (GaAs) crystals. We have compared the experimental results with the Monte Carlo simulations of the focusing capability of GaAs tiles performed with a dedicated ray-tracer. The GaAs tiles were bent using a lapping process developed at the cnr/imem - Parma (Italy) in the framework of the laue project, funded by ASI, dedicated to build a broad band Laue lens prototype for astrophysical applications in the hard X-/soft γ-ray energy range (80-600 keV). We present and discuss the results obtained from their characterization, mainly in terms of focusing capability. Bent crystals will significantly increase the signal to noise ratio of a telescope based on a Laue lens, consequently leading to an unprecedented enhancement of sensitivity with respect to the present non focusing instrumentation. 相似文献