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81.
Résumé L'activité magmatique ophiolitique du géosynclinal alpin (diabases, gabbros, serpentines, etc.) a été suivie par une activité à caractère volcanique moins bien connue. En effet, les appareils correspondant à cette activité ont complètement disparu; nous devons nous contenter pour tous renseignements de l'étude des fragments de roches contenus dans des grauwackes tertiaires appartenant au Flysch (grès de Taveyanne, grès d'AItdorf pro parte, grès du Champsaur).La détermination de la nature originelle des laves est, en outre, rendue difficile par le fait, découvert récemment, que ces grauwackes ont subi un métamorphisme régional les plaçant dans le faciès à zéolites; on peut raisonnablement admettre qu'il s'agissait d'andésites basaltiques.L'áge des épanchements est encore indéterminé, il doit être compris entre le Crétacé supérieur et la fin de l'Eocène. L'hypothèse la plus plausible consiste à admettre que les volcans, aujourd'hui complètement érodés se trouvaient dans la partie la plus interne du domaine pennique. Toutefois au moment du dépôt des grès de Taveyanne, les coulées ne se trouvaient plus dans leur position initiale, elles avaient glissé vers l'avant-pays sous forme d'une nappe.Il est très probable que cette activité volcanique post-ophiolitique n'est pas restreinte au segment franco-suisse des Alpes occidentales mais que des formations analogues aux grès de Taveyanne se retrouvent ailleurs, notamment en Sicile et dans les Apennins.
The magmatic activity which gave birth to the ophiolites (diabases, gabbros, serpentinites) of the alpine geosyncline was followed by subaerial volcanism. This volcanic activity is not well known as the volcanoes were completely destroyed by erosion. Our only source of information is to be found in fragments of volcanic rocks which are part of Tertiary Flysch graywackes (Taveyanne sandstones, part of the Altorf sandstones, Champsaur sandstones).The determination of the initial composition of the lavas is further complicated by metasomatic transformations; it has been recently shown that the Taveyanne graywackes were submitted to a light regional metamorphism corresponding to the zeolitic facies ofCoombs. However, it seems that these lavas were originally basaltic andesites.The age of this volcanism is not precisely known, it cannot be later than Upper Eocene as the time of deposition of the Taveyanne sandstones is Uppermost Eocene-Lower Oligocene; it is probably post-Cenomanian. It is likely that the volcanoes were located in the southern part of the Penninic zone; however at the time of deposition of the graywackes the volcanic flows had already left their initial location, gliding toward the Foreland as part of a Nappe.Very probably, remnants of this post-ophiolitic volcanism are not restricted to the French-Swiss segment of the Western Alps, but will be found elsewhere, particularly in the Apennine Mountains and in Sicily.
Zusammenfassung Die magmatische Tätigkeit, die Ophiolithe (Diabase, Gabbros, Serpentinite) der alpinen Geosynklinale entstehen ließ, wurde von subärischem Vulkanismus abgelöst. Diese Vulkantätigkeit ist wenig bekannt, da die Vulkane durch Erosion völlig zerstört wurden. Unsere einzige Informationsquelle findet sich in vulkanischen Gesteinsfragmenten, die Bestandteile der Tertiär-Flysch-Grauwacken sind.Die Bestimmung der ursprünglichen Zusammensetzung der Laven wird weiter durch metasomatische Umwandlungen erschwert. Kürzlich wurde gezeigt, daß die Taveyanne-Grauwacken einem regionalen Metamorphismus ausgesetzt waren, welcher der zeolithischen Fazies von Coombs entspricht. Es scheint jedoch, daß diese Laven ursprünglich basaltische Andésite waren.Das Alter dieses Vulkanismus ist nicht genau bekannt; es kann aber nicht später sein als das Obere Eozän, da die Ablagerungszeit der Taveyanne-Sandsteine Oberstes Eozän—Unteres Oligozän ist. Wahrscheinlich lagen die Vulkane im südlichen Teil der penninischen Zone; zur Zeit der Ablagerung der Grauwacken waren die Vulkanite bereits in die Überschiebungsmassen mit einbezogen.Sehr wahrscheinlich sind die Überreste dieses nach-ophiolithischen Vulkanismus nicht auf den französisch-schweizerischen Abschnitt der Westalpen beschränkt, sondern werden sich auch andernorts speziell auf dem Apennin und in Sizilien finden lassen.
, (, ) , . , . , . . , Taveyane ( Coombs'y), , . .相似文献
82.
Ahmed Touil Abdelmajid El-Boukhari Essaid Bilal Jacques Moutte 《Journal of African Earth Sciences》1999,29(4):81
The Upper Proterozoic granitoids of the western part of the Siroua Massif (central Anti-Atlas, Morocco) are cut by doleritic dykes injected along submeridian and equatorial directions. These dykes were emplaced before deposition of late Neoproterozoic formations (PIII). According to
and incompatible element ratios, these dolerites constitue two discrete chemical groups unrelated to orientation and thickness. They are both enriched in large ion lithophile elements, Zr, Th and light rare earth elements, and correspond to continental tholeiites displaying an alkaline affinity. This alkaline affinity is also confirmed by clinopyroxene and amphibole chemistry. Emplacement of these doleritic dykes occurred under an extensional regime active in the Anti-Atlas range during the Upper Proterozoic. 相似文献
83.
Jacques Jedwab 《Meteoritics & planetary science》1975,10(3):191-207
In addition to the well known cosmic spheres, micron-size metallic flakes have been extracted magnetically from Pacific Ocean manganese nodules. The flakes were individually studied by several techniques (LM, SEM, EMP and XRD) and were found to be composed of iron, iron-nickel and nickel-iron. In general, the flakes are agglomerates of micron to sub-micron flat particles loosely held together. The cosmic origin of these flakes is discussed with regard to chemical composition, crystallinity, agglomeration and comparable terrestrial minerals. This finding makes available an inexhaustible and readily accessible source of cosmic minerals. At the same time, it gives a direct clue to the mineralogical and chemical differences between meteorites and micrometeorites. 相似文献
84.
The properties of rapidly changing inhomogeneities visible in the H and K lines above sunspot umbrae are described. We find as properties for these ‘Umbral Flashes’:
- A lifetime of 50 sec. The light curve is asymmetrical, the increase is faster than the decrease in brightness.
- A diameter ranging from the resolution limit up to 2000 km.
- A tendency to repeat every 145 sec.
- A ‘proper motion’ of 40 km/sec generally directed towards the penumbra.
- A Doppler shift of 6 km/sec.
- A magnetic field of 2100 G.
- A decrease in this field of 12 G/sec. This decrease is probably related to the flash motion.
- At any instant an average of 3–5 flashes in a medium-sized umbra. A weak feature often persists in the umbra after the flash. This post-flash structure initially shows a blue shift, but 100–120 sec after the flash, it shows a rapid red shift just before the flash repeats.
85.
We present here the numerical application of the theoretical results derived in Correia et al. (2003, Icarus 163, 1-23) for the spin evolution of Venus since its formation. We explore a large variety of initial conditions to cover the possible formation and evolutionary scenarios. In particular, we pay special attention to the evolutions which cross the chaotic zone resulting from secular planetary perturbations (Laskar and Robutel, 1993, Nature 361, 608-612). We demonstrate that Venus’ axis can be temporarily trapped in a secular resonance with the node of Neptune’s orbit, which can prevent it from being tilted to 180° and will drive it toward 0°. We test several dissipation models and parameters to evaluate their contribution to the planet’s spin history. We confirm that despite the variations in the models, only three of the four final spin states of Venus are possible (Correia and Laskar, 2001, Nature 411, 767-770) and that the present observed retrograde spin state of Venus can be attained by two different processes. In the first scenario (π−), the axis is tilted toward 180° while its rotation rate slows down, while in the second one, the axis is driven toward 0° obliquity and the rotation rate decreases, stops, and increases again in the reverse direction to a final equilibrium value (0−). 相似文献
86.
Jacques Hinderer 《中国科学D辑(英文版)》2006,49(12):1259-1269
New generation superconducting gravimeters (SGs), which have been demonstrated to be better than the best seismometers STS-1 at frequencies below 1 mHz, can be accepted as the quietest vertical seismometers for observation of long-period earth free oscillations. Wavelet filtering with narrow band-pass frequency response as shown in this paper is very helpful in removing at- mospheric pressure effects from on gravity records in long-period seismic mode frequency bands. The processing of high quality SG records after the great Sumatra earthquake (Dec. 26, 2004) with wavelet filtering leads to clear observations of all coupled toroidal modes below 1.5 mHz except these for 0T5, 0T7 and 1T1; moreover 1T2 and 1T3 are, for the first time, unambiguously revealed in the vertical components of the free oscillations. The three well-resolved splitting singlets of overtones 2S1 are observed from a single SG record for the first time. 相似文献
87.
新型超导重力仪已被证实在频率低于1 mHz的情况下优于最好的地震仪STS-1, 因而新型超导重力仪可作为极低噪音的地震仪, 观测长周期地球自由振荡. 具有良好窄带频率响应的小波滤波器非常有助于消除大气压波动对重力变化的影响. 用小波滤波器处理2004年12月26日苏门答腊大地震后的超导重力仪的观测数据, 清楚地检测到了1.5 mHz以下, 除0T5, 0T7, 1T1外所有的环形自由振荡的耦合现象, 并检测到了环形自由振荡1T2, 1T3的耦合现象. 此外, 还利用单台超导重力仪的观测数据清楚地检测到了球形自由振荡2S1的3个分裂谱峰. 相似文献
88.
We have performed holographic interferometry measurements of the dissolution of the (0 1 0) plane of a cleaved gypsum single crystal in pure water. These experiments have provided the value of the dissolution rate constant k of gypsum in water and the value of the interdiffusion coefficient D of its aqueous species in water. D is 1.0 × 10−9 m2 s−1, a value close to the theoretical value generally used in dissolution studies. k is 4 × 10−5 mol m−2 s−1. It directly characterizes the microscopic transfer rate at the solid-liquid interface, and is not an averaged value deduced from quantities measured far from the surface as in macroscopic dissolution experiments. It is found to be two times lower than the value obtained from macroscopic experiments. 相似文献
89.
The Zagros fold-and-thrust belt of SW-Iran is among the youngest continental collision zones on Earth. Collision is thought to have occurred in the late Oligocene–early Miocene, followed by continental shortening. The High Zagros Belt (HZB) presents a Neogene imbricate structure that has affected the thick sedimentary cover of the former Arabian continental passive margin. The HZB of interior Fars marks the innermost part of SE-Zagros, trending NW–SE, that is characterised by higher elevation, lack of seismicity, and no evident active crustal shortening with respect to the outer (SW) parts. This study examines the brittle structures that developed during the mountain building process to decipher the history of polyphase deformation and variations in compressive tectonic fields since the onset of collision. Analytic inversion techniques enabled us to determine and separate different brittle tectonic regimes in terms of stress tensors. Various strike–slip, compressional, and tensional stress regimes are thus identified with different stress fields. Brittle tectonic analyses were carried out to reconstruct possible geometrical relationships between different structures and to establish relative chronologies of corresponding stress fields, considering the folding process. Results indicate that in the studied area, the main fold and thrust structure developed in a general compressional stress regime with an average N032° direction of σ1 stress axis during the Miocene. Strike–slip structures were generated under three successive strike–slip stress regimes with different σ1 directions in the early Miocene (N053°), late Miocene–early Pliocene (N026°), and post-Pliocene (N002°), evolving from pre-fold to post-fold faulting. Tensional structures also developed as a function of the evolving stress regimes. Our reconstruction of stress fields suggests an anticlockwise reorientation of the horizontal σ1 axis since the onset of collision and a significant change in vertical stress from σ3 to σ2 since the late stage of folding and thrusting. A late right-lateral reactivation was also observed on some pre-existing belt-parallel brittle structures, especially along the reverse fault systems, consistent with the recent N–S plate convergence. However, this feature was not reflected by large structures in the HZB of interior Fars. The results should not be extrapolated to the entire Zagros belt, where the deformation front has propagated from inner to outer zones during the younger events. 相似文献
90.
Aspects of GLONASS Carrier-Phase Differencing 总被引:2,自引:0,他引:2