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941.
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945.
Basalts dredged from the south wall of a fracture zone transecting the southern Mid-Atlantic Ridge (SMAR) at 54° S are unusual in that they include a suite of highly olivine phyric basalts, sampled along with more normal sparsely plagioclase phyric basalts, and a highly plagioclase phyric basalt. Four basalt types (olivine phyric, sparsely plagioclase phyric, evolved sparsely plagioclase phyric and highly plagioclase phyric) are readily distinguished on the basis of petrography, mineralogy and bulk composition. They range from primitive to evolved, with the olivine phyric basalts having elevated MgO (up to 15.5%) and the plagioclase phyric basalt having elevated Al2O3 (19.3%) and CaO (13.1%) contents. Compositional variations are extremely consistant, with the olivine phyric basalts and the sparsely plagioclase phyric basalts defining coherent linear trends. On the basis of the ratios and covariation of the incompatible trace elements Zr, Nb, Y and Ba, distinct parental magmas for each basalt type are required. An investigation of Fe-Mg and Mg-Ni distribution coefficients between olivine and magma indicates that olivines from the olivine phyric basalts are on average too forsteritic and too Ni poor to have crystallized in a magma corresponding to the host bulk rock composition. This implies that these basalts are enriched in xenocrystic olivine. Olivines from the other basalt types are mostly of equilibrium composition, although there are some exceptions. Petrogenetic models for the formation of the different basalt types are quantitatively evaluated in terms of fractional crystallization/crystal accumulation processes. These indicate that (1) the olivine phyric basalts are the products of olivine and minor Cr-spinel accumulation and do not represent analogues of primary magma, or a liquid fractionation trend; (2) that the sparsely plagioclase phyric basalts were formed by polybaric fractional crystallization of olivine, plagioclase and clinopyroxene; and (3) that the evolved sparsely plagioclase phyric basalts are not readily related to one another. The single highly plagioclase phyric basalt is unrelated to the other basalt types and is cumulus enriched in plagioclase.The different basalt types are unrelated to one another and document the presence of at least four distinct magma types erupted in close proximity at this ridge/transform intersection on the southern end of the Mid-Atlantic Ridge. 相似文献
946.
Constant M.G. van den Berg 《Geochimica et cosmochimica acta》1984,48(12):2613-2617
The stability constants, , for borate complexes with the ions of Cu, Pb, Cd and Zn are determined in this work by DPASV in 0.7 M KNO3 at metal concentrations of 10?7 M. The acidity constants of the Cu2+ ion are determined by DPASV in the same conditions. The following values for log () have been obtained: CuB: 3.48, CuB2: 6.13, PbB: 2.20, PbB2: 4.41, ZnB: 0.9, ZnB2: 3.32, CdB: 1.42, and CdB2: 2.7, while the values for the acidity constants of Cu are and . At the low concentration of boron in 35%. S sea-water complexes with borate represent only about 0.2% Cu, 0.03% Pb, 0.02% Zn and 0.003% Cd. 相似文献
947.
In 1982 we carried out a shallow-penetration, high-resolution seismic profiling study on the shelf of the southern Argolid, Peloponnesos, Greece, to identify and map the shores of the late Pleistocene and Holocene, and to establish their coastal environments. Portable equipment and a local boat were used. The lowest glacial shore occurs at ?115 to ?118 m, within the range of global values. The subsequent rise across the distinct old land surface left behind many shore features (scaps, beaches and beach ridges, channels and lagoons) now buried under a few meters of post-transgressive deposits. These features cluster at a small number of depths below present sea level, suggesting that the rise of the sea, usually too fast to leave an imprint, was episodically interrupted by brief stillstands or even temporary reversals of climatic or tectonic origin. The clusters can be roughly dated with reference to a global sea-level-rise curve; after 6000 yr B.P. sparse archaeological data establish a local curve. The seismic profiling technique, convenient and not costly, holds promise for the identification of postglacial shores elsewhere prior to sampling for dating. It has wide application for environmental reconstructions of vanished coastal zones as a basis for prehistoric resource assessments. These applications are illustrated with examples from this study. 相似文献
948.
949.
Univ. Doz. Dr. Dirk van Husen 《International Journal of Earth Sciences》1984,73(1):433-445
Zusammenfassung Während der Sedimentation der Rosenbacher Kohleschichten (W.Klaus 1956, Untersarmat) spielten die Karawanken als Liefergebiet der Sedimente kaum eine Rolle. Wie aus der Verbreitung dieser Sedimente im Bereich des Karawankenkörpers zu erkennen ist, wurden zumindest seine nördlichen Teile damit bedeckt. Im Hangenden dieser, aus gut gerollten, tonig sandigen Kiesen (mit hohem Quarzanteil) gebildeten Rosenbacher Kohleschichten treten dann die ersten deutlichen Einschüttungen aus den Karawanken auf. Diese deuten auf eine beginnende Heraushebung hin. Ihre Geröllzusammensetzung zeigt an, daß am Beginn dieser Entwicklung noch ein deutlicher Gerölltransport aus dem Bereich der Periadriatischen Naht über den Nordstamm der Karawanken stattfand.Die fortschreitende Heraushebung unterbrach diese Transportwege und führte zum Lösen großer Schollen von Wettersteinkalk, die nach Norden abglitten. Begünstigt wurde dieser Vorgang durch die Unterlagerung des Wettersteinkalkes durch mächtige Raibler Schiefer, die als Gleitmittel dienten.Die abgeglittenen Schollen (Tafeln bis zu 100–150 m Mächtigkeit und Längserstreckungen bis 2000 m) wurden dann in die grobklastischen Sedimente des Vorlandes konkordant eingelagert. Beide Vorgänge, Lösen und Abgleiten ins Vorland dieser Tafeln deuten auf eine rasche Hebung des Karawankenkörpers hin.Die weitere Hebung brachte dann nur noch sehr grobe Karbonatkiese, die die hangenden Anteile des grobklastischen Jungtertiärs (Bärental Konglomerat) bilden.In der weiteren Folge wurden diese Sedimente noch vom Karawankenkörper über eine kurze Strecke überschoben und auch in die fortschreitende Hebung (Ostteile) miteinbezogen.
During the sedimentation of the Rosenbacher Kohleschichten (W.Klaus 1956, Untersarmat) the Karawanken were not so important for yielding sediments. As to be seen by the distribution of these sediments in the Karawanken area, at least its northern parts were covered by them. The top layers of the Rosenbacher Kohleschichten, consisting of clayey, sandy, well shaped gravels (with a high percentage of quartz) show first strong embankments from the Karawanken indicating a beginning uplift. Their gravel composition assigns that at the beginning of this development there was yet a transport northward from the area of the Periadriatische Naht through the Nordstamm of the Karawanken on many places.The proceeding uplift interrupted some of these spillways and lead to a discharge of large plates of Wettersteinkalk which glided northward. This procedure was favored by the thick Raibler Schiefer underlying the Wettersteinkalk and working as a lubricant.The down-glided plates (to 100–200 m thickness and a width up to 2000 m) were then embedded concordantly in the coarse clastic sediments of the forelands. Both, discharge and gliding of the plates point to a quick uplift of the Karawanken during Obersarmat.The further uplift yielded only very coarse carbonate gravels forming the top layers of the coarse clastic Young Tertiary (Bärental Konglomerat).Henceforth these sediments were overthrust by the Karawankenbody over a short distance and included in the advancing uplift (Eastern parts).
Résumé Pendant la sédimentation des Rosenbacher Kohleschichten (W. Klaus 1956, Sarmatien inférieur) les Karawanken ne jouaient pas un grand rôle dans l'apport de sédiments. Tout au moins les sédiments couvraient-ils les pentes nord des Karawanken. Le toit des Rosenbacher Kohleschichten (formées par les graviers sableux et argileux, bien roulés, avec quartz abondant) montrent les premiers remblaiements provenant des Karawanken. Ceuxci indiquent le commencement du soulèvement des Karawanken. La composition des galets indiquent que, au commencement de ce développement, il y avait encore un transport bien marqué de galets depuis la suture périadriatique par dessus le rameau septentrional des Karawanken. Le soulèvement progressif interrompit cette voie de transport et conduisit à la séparation des grands blocaux du Wettersteinkalk, qui glissèrent vers le Nord. Ce processus était favorisé par la présence d'une puissante couche de Schistes de Raibler en-dessous du Wettersteinkalk, agissant comme lubrifiant.Puis les blocaux entraînés (des plaques de 100 à 200 m. d'épaisseur, jusqu'à 2000 m. de long), venaient s'intercaler en concordance dans les sédiments clastiques grossiers de l'avant-pays. Les deux phénomènes, séparation et glissement de ces plaques dans l'avantpays, indiquent un soulèvement rapide des Karawanken. Le soulèvement ultérieur ne délivra que de gros cailloux carbonatiques qui forment la partie supérieure du Miocène clastique (Bärentalkonglomerat).Dans la suite, ces sédiments furent chevauchés sur une courte distance par les Karawanken et impliqués aussi dans le soulèvement encore en cours (partie orientale).
(W. Klaus, 1956, Untersarmat) , , . , . , , . . , . , . , . ( 100– 150 2000 ) . , , . - , ( ). .相似文献
950.
L. van Driel-Gesztelyi A. Hofmann P. Démoulin B. Schmieder G. Csepura 《Solar physics》1994,149(2):309-330
Through coordinated observations made during the Max'91 campaign in June 1989 in Potsdam (magnetograms), Debrecen (white light and H), and Meudon (MSDP), we follow the evolution of the sunspot group in active region NOAA 5555 for 6 days. The topology of the coronal magnetic field is investigated by using a method based on the concept of separatrices - applied previously (Mandriniet al., 1991) to a magnetic region slightly distorted by field-aligned currents. The present active region differs by having significant magnetic shear. We find that the H flare kernels and the main photospheric electric current cells are located close to the intersection of the separatrices with the chromosphere, in a linear force-free field configuration adapted to the observed shear. Sunspot motions, strong currents, isolated polarities, or intersecting separatrices are not in themselves sufficient to produce a flare. A combination of them all is required. This supports the idea that flares are due to magnetic reconnection, when flux tubes with field-aligned currents move towards the separatrix locations. 相似文献