全文获取类型
收费全文 | 918篇 |
免费 | 15篇 |
国内免费 | 5篇 |
学科分类
地球科学 | 938篇 |
出版年
2021年 | 5篇 |
2020年 | 5篇 |
2019年 | 17篇 |
2018年 | 11篇 |
2017年 | 8篇 |
2016年 | 18篇 |
2015年 | 12篇 |
2014年 | 18篇 |
2013年 | 40篇 |
2012年 | 29篇 |
2011年 | 35篇 |
2010年 | 37篇 |
2009年 | 60篇 |
2008年 | 43篇 |
2007年 | 31篇 |
2006年 | 36篇 |
2005年 | 34篇 |
2004年 | 34篇 |
2003年 | 31篇 |
2002年 | 30篇 |
2001年 | 17篇 |
2000年 | 11篇 |
1999年 | 19篇 |
1998年 | 10篇 |
1997年 | 17篇 |
1996年 | 12篇 |
1995年 | 20篇 |
1994年 | 26篇 |
1993年 | 12篇 |
1992年 | 11篇 |
1991年 | 19篇 |
1990年 | 16篇 |
1989年 | 12篇 |
1988年 | 10篇 |
1987年 | 9篇 |
1986年 | 13篇 |
1985年 | 8篇 |
1984年 | 15篇 |
1983年 | 17篇 |
1982年 | 13篇 |
1981年 | 7篇 |
1980年 | 15篇 |
1979年 | 7篇 |
1978年 | 5篇 |
1977年 | 12篇 |
1975年 | 8篇 |
1974年 | 8篇 |
1973年 | 14篇 |
1971年 | 6篇 |
1969年 | 4篇 |
排序方式: 共有938条查询结果,搜索用时 31 毫秒
921.
Rainer Beck 《地球物理与天体物理流体动力学》2013,107(1-3):3-4
Abstract Evidence from radio polarization measurements is reviewed that indicates that most galactic magnetic field structures fall into one of two categories: axisymmetric spiral and bisymmetric spiral. The resultant challenges to dynamo theorists is stated. Estimates of the magnetic field strengths based on equipartition of field and cosmic ray energies are given, but deviations from equipartition are inferred. Possible goals for future research are suggested. 相似文献
922.
Mathieu Duval Christophe Falguères Jean-Jacques Bahain Rainer Grün Qingfeng Shao Maxime Aubert Jean-Michel Dolo Jordi Agustí Bienvenido Martínez-Navarro Paul Palmqvist Isidro Toro-Moyano 《Quaternary Research》2012,77(3):482-491
The combined U-series/electron spin resonance (ESR) dating method was applied to nine teeth from two Early Pleistocene archaeological sites located in the Orce area (Guadix-Baza Basin, Southern Spain): Fuente Nueva-3 (FN-3) and Barranco León (BL). The combination of biostratigraphy and magnetostratigraphy places both sites between the Olduvai and Jaramillo subchrons (1.78–1.07 Ma).Our results highlight the difficulty of dating such old sites and point out the limits of the combined U-series/ESR dating method based on the US model. We identified several sources of uncertainties that may lead to inaccurate age estimates. Seven samples could not be dated because the dental tissues had (230Th/234U) activity ratios higher than equilibrium, indicating that uranium had probably leached from these tissues. It was however possible to calculate numerical estimates for two of the teeth, both from FN-3. One yielded a Middle Pleistocene age that seems to be strongly underestimated; the other provided an age of 1.19 ± 0.21 Ma, in agreement with data obtained from independent methods. The latter result gives encouragement that there are samples that can be used for routine dating of old sites. 相似文献
923.
Thomas S. Kruijer Peter Sprung Thorsten Kleine Ingo Leya Rainer Wieler 《Meteoritics & planetary science》2013,48(12):2597-2607
Cadmium is a highly volatile element and its abundance in meteorites may help better understand volatility‐controlled processes in the solar nebula and on meteorite parent bodies. The large thermal neutron capture cross section of 113Cd suggests that Cd isotopes might be well suited to quantify neutron fluences in extraterrestrial materials. The aims of this study were (1) to evaluate the range and magnitude of Cd concentrations in magmatic iron meteorites, and (2) to assess the potential of Cd isotopes as a neutron dosimeter for iron meteorites. Our new Cd concentration data determined by isotope dilution demonstrate that Cd concentrations in iron meteorites are significantly lower than in some previous studies. In contrast to large systematic variations in the concentration of moderately volatile elements like Ga and Ge, there is neither systematic variation in Cd concentration amongst troilites, nor amongst metal phases of different iron meteorite groups. Instead, Cd is strongly depleted in all iron meteorite groups, implying that the parent bodies accreted well above the condensation temperature of Cd (i.e., ≈650 K) and thus incorporated only minimal amounts of highly volatile elements. No Cd isotope anomalies were found, whereas Pt and W isotope anomalies for the same iron meteorite samples indicate a significant fluence of epithermal and higher energetic neutrons. This observation demonstrates that owing to the high Fe concentrations in iron meteorites, neutron capture mainly occurs at epithermal and higher energies. The combined Cd‐Pt‐W isotope results from this study thus demonstrate that the relative magnitude of neutron capture‐induced isotope anomalies is strongly affected by the chemical composition of the irradiated material. The resulting low fluence of thermal neutrons in iron meteorites and their very low Cd concentrations make Cd isotopes unsuitable as a neutron dosimeter for iron meteorites. 相似文献
924.
Rainer Wieler 《Earth, Moon, and Planets》2011,108(1):1-8
Some of the distinct noble gas “components” in meteorites represent a record of processes during and even before solar system
formation. This record is difficult to interpret. Often, one of the major problems is to recognize whether a certain noble
gas elemental and isotopic pattern has been established in a presolar epoch, later in the solar accretion disk, during meteorite
parent body formation or finally as a result of metamorphism on a parent body. It would also appear that noble gases are a
preferred tool to deduce the types of matter from which the Earth and other planets accreted—if the respective parent materials
are present in our extraterrestrial sample collections at all. However, also this issue is unsettled. Noble gas isotopes originating
from the decay of radioactive precursors allow us to study the early and later degassing history of terrestrial planets, although
the interpretation often remains model-dependent. This contribution briefly reviews some of the fundamental aspects of the
noble gas record in meteorites and planets. 相似文献
925.
Thomas KENKMANN Marcos A. R. VASCONCELOS Alvaro P. CRÓSTA Wolf U. REIMOLD 《Meteoritics & planetary science》2011,46(6):875-889
Abstract– Serra da Cangalha is a complex impact structure with a crater diameter of 13,700 m and a central uplift diameter of 5800 m. New findings of shatter cones, planar fractures, feather features, and possible planar deformation features are presented. Several ring‐like features that are visible on remote sensing imagery are caused by selective erosion of tilted strata. The target at Serra da Cangalha is composed of Devonian to Permian sedimentary rocks, mainly sandstones that are interlayered with siltstone and claystones. NNE–SSW and WNW–ESE‐striking joint sets were present prior to the impact and also overprinted the structure after its formation. As preferred zones of weakness, these joint sets partly controlled the shape of the outer perimeter of the structure and, in particular, affected the deformation within the central uplift. Joints in radial orientation to the impact center did not undergo a change in orientation during tilting of strata when the central uplift was formed. These planes were used as major displacement zones. The asymmetry of the central uplift, with preferred overturning of strata in the northern to western sector, may suggest a moderately oblique impact from a southerly direction. Buckle folding of tilted strata, as well as strata overturning, indicates that the central uplift became gravitationally unstable at the end of crater formation. 相似文献
926.
We use a lattice vibrational technique to derive thermophysical and thermochemical properties of the pure elements aluminum
and iron in pressure–temperature space. This semi-empirical technique is based on either the Mie–Grüneisen–Debye (MGD) approach
or an extension of Kieffer’s model to incorporate details of the phonon spectrum. It includes treatment of intrinsic anharmonicity,
electronic effects based on the free electron gas model, and magnetic effects based on the Calphad approach. We show that
Keane’s equation of state for the static lattice is better suitable to represent thermodynamic data for aluminum from 1 bar
to pressures in the multi-megabar region relative to Vinet’s universal and the Birch–Murnaghan equation of state. It appears
that the MGD and Mie–Grüneisen–Kieffer approach produce similar results, but that the last one better represents heat capacity
below room temperature. For iron we show that the high temperature behavior of thermal expansivity can be explained within
the Calphad approach by a pressure-dependent Curie temperature with a slope between –1 and 0 K/GPa. 相似文献
927.
Júlia Dégi Rainer Abart Kálmán Török Enikő Bali Richard Wirth Dieter Rhede 《Contributions to Mineralogy and Petrology》2010,159(3):293-314
The complex microstructure of kelyphitic rims around garnet in lower crustal garnet granulite xenoliths from the Bakony–Balaton
Highland Volcanic Field, Central Pannonian Basin has been studied in order to identify controls on garnet breakdown. Symplectites
comprised of a vermicular intergrowth of submicron sized anorthite, orthopyroxene and spinel replace garnet at a sharp reaction
front. Based on element distribution maps the transformation of garnet to symplectite is isochemical. Phase diagram calculations
indicate that this reaction was induced by a pressure decrease and/or a temperature increase. In site-specific TEM foils prepared
by focused ion beam technique and oriented parallel and perpendicular to the reaction front 200 nm wide rods of anorthite
and 20 nm wide rods of spinel are identified. The rods are oriented approximately perpendicular to the replacement front and
are embedded in an orthopyroxene matrix. The regular spacing of the symplectite phases along the reaction front suggests that
their growth is controlled by diffusion. The kinetics of symplectite formation has been modelled based on irreversible thermodynamics.
During interaction of the xenolith with the host basalt the microstructure and chemistry of the An–Opx–Spl symplectite was
significantly modified and it was partially replaced by an olivine bearing symplectite. In contrast to primary symplectite
formation, these processes were metasomatic in nature including addition of sodium, titanium and some trace elements from
the basaltic melt and can clearly be discerned from the garnet breakdown. Based on these observations it is inferred that
symplectite formation took place within the deep crust during the extension of the Pannonian Basin between 15 and 30 km depth
at high temperature (850–1,050°C) prior to the volcanic transport to the surface. 相似文献
928.
Ming-Sheng Wang Stephen F. Wolf Michael E. Lipschutz 《Meteoritics & planetary science》1999,34(5):713-716
Abstract— We have used radiochemical neutron activation analysis (RNAA) to determine 15 trace elements, including 10 moderately to highly volatile ones—Rb, Ag, Se, Cs, Te, Zn, Cd, Bi, Tl, In (in increasing volatility order), in 6 H chondrite falls with low-3He contents. These (plus prior RNAA data) provide a compositional database of 92 H4-6 chondrite falls. Three suites of samples can be identified from their noble gas contents: 44 with “normal” contents and, therefore, “normal” orbits and cosmic-ray exposure histories; 8 that lost radiogenic gases, presumably by shock late in their histories; and 17 that lost cosmogenic gases by heating during close solar approach. We used the standard multivariate statistical techniques of linear discriminant analysis and logistic regression to compare contents of the 10 moderately and highly volatile trace elements, listed above, in these three suites. We found no significant differences. This contrasts sharply with similar comparisons involving random falls and H4-6 chondrites that landed on Earth at specific time intervals. Apparently, contents of volatile trace elements in H4-6 chondrites were established early in their histories, and they are so retentively sited that loss during later heating episodes did not occur. 相似文献
929.
Determination of Trace Elements in the Quartz Reference Material UNS-SpS and in Natural Quartz Samples by ICP-MS 总被引:1,自引:0,他引:1
Thomas Monecke Gisela Bombach Werner Klemm Ulf Kempe Jens Götze Dieter Wolf 《Geostandards and Geoanalytical Research》2000,24(1):73-81
A procedure for the digestion and analysis of quartz samples was developed to measure trace element concentrations in natural quartz. The certified glass sand reference material UNS-SpS was chosen to assess the precision, accuracy and detection limit of the analytical method. Quartz was digested with HF/HNO3 in a closed glassy carbon vessel and analysed by means of quadrupole ICP-MS with external calibration. Analyte concentrations of the sand UNS-SpS were compared with certified and other values from the literature. The abundances of a number of elements (Pr, Gd, Ho and Er) in the reference material are reported here for the first time. The procedure was then applied to three quartz samples from different geological settings to show that trace element data by ICP-MS can distinguish the origin of the sample. 相似文献
930.
The Preparation and Preliminary Characterisation of Eight Geological MPI-DING Reference Glasses for In-Situ Microanalysis 总被引:13,自引:4,他引:9
Klaus Peter Jochum Donald B. Dingwell Alexander Rocholl Brigitte Stoll Albrecht W. Hofmann S. Becker A. Besmehn D. Bessette H.-J. Dietze P. Dulski J. Erzinger E. Hellebrand P. Hoppe I. Horn K. Janssens G.A. Jenner M. Klein W.F. McDonough M. Maetz K. Mezger C. Müker I.K. Nikogosian C. Pickhardt I. Raczek D. Rhede H.M. Seufert S.G. Simakin A.V. Sobolev B. Spettel S. Straub L. Vincze A. Wallianos G. Weckwerth S. Weyer D. Wolf M. Zimmer 《Geostandards and Geoanalytical Research》2000,24(1):87-133
Eight silicate glasses were prepared by directly fusing and stirring 50-100 g each of basalt, andesite, komatiite, peridotite, rhyolite, and quartz-diorite. These are referred to as MPI-DING glasses and were made for the purpose of providing reference materials for geochemical, in-situ microanalytical work. Results from various analytical techniques indicate that individual glass fragments are well homogenised with respect to major and trace elements at the μm to mm scale. Heterogeneities due to quench crystallisation of olivine have been observed in small and limited areas of the two komatiitic glasses. In order to obtain concentration values for as many elements as possible, the glasses were analysed by a variety of bulk and microanalytical methods in a number of laboratories. The analytical uncertainties of most elements are estimated to be between 1% and 10%. From the analytical data, preliminary reference values for more than sixty elements were calculated. The analytical uncertainties of most elements are estimated to be between 1% and 10%. 相似文献