全文获取类型
收费全文 | 171篇 |
免费 | 3篇 |
专业分类
测绘学 | 26篇 |
大气科学 | 4篇 |
地球物理 | 42篇 |
地质学 | 34篇 |
海洋学 | 6篇 |
天文学 | 31篇 |
自然地理 | 31篇 |
出版年
2021年 | 1篇 |
2018年 | 1篇 |
2017年 | 1篇 |
2016年 | 2篇 |
2015年 | 7篇 |
2014年 | 8篇 |
2013年 | 3篇 |
2012年 | 2篇 |
2011年 | 6篇 |
2010年 | 2篇 |
2009年 | 13篇 |
2008年 | 10篇 |
2007年 | 5篇 |
2006年 | 11篇 |
2005年 | 12篇 |
2004年 | 14篇 |
2003年 | 13篇 |
2002年 | 8篇 |
2001年 | 3篇 |
2000年 | 5篇 |
1999年 | 2篇 |
1998年 | 1篇 |
1997年 | 1篇 |
1994年 | 2篇 |
1993年 | 1篇 |
1992年 | 1篇 |
1991年 | 4篇 |
1990年 | 2篇 |
1989年 | 1篇 |
1988年 | 3篇 |
1987年 | 3篇 |
1986年 | 1篇 |
1985年 | 1篇 |
1984年 | 3篇 |
1983年 | 6篇 |
1981年 | 2篇 |
1980年 | 2篇 |
1979年 | 1篇 |
1977年 | 2篇 |
1976年 | 2篇 |
1974年 | 2篇 |
1973年 | 1篇 |
1972年 | 1篇 |
1971年 | 1篇 |
1970年 | 1篇 |
排序方式: 共有174条查询结果,搜索用时 889 毫秒
11.
12.
13.
Preferential release into solution of radionuclides that result from alpha decay is a contributor to natural isotopic disequilibrium. Such release is critical to geochemical understanding of alpha-decay products and would be an undesirable characteristic of solidified nuclear waste in deep geological formations. Spontaneous annealing of the radiation damage that is responsible for the preferential release is shown to diminish the effect in thorianite and uraninite which we have found to be 550 to 1000 M.y. old, respectively. Leaching experiments and measurements of the thorium and uranium isotopes show that there is strongly enhanced release of short-lived 228Th relative to 232Th, but only slight enhancement of long-lived 234U and 230Th relative to 238U and 232Th. These results are interpreted in terms of natural annealing of damage occurring on a time scale between the ~10 and 105 years of the alpha-decay products. With a simple assumption actual times for the survival of the enhanced leaching in these minerals are ~ 15,000 years. 相似文献
14.
Helmut Bock 《Rock Mechanics and Rock Engineering》1971,3(4):225-238
SummaryComputer Simulation of Second Order Faults Faults of the second order can be simulated in the computer with an accuracy hitherto unknown, by using Malina's (1969, 1970) program version of the Finite Element Method. The computations show that stress rearrangements occur with shear movements along the principal fault and with propagation of the fault. These stress rearrangements contribute to the development of new secondary faults. The computed second order faults can be classified according to Chinnery (1966) as shear plane typesA, B, E, andF. Moreover, the computation shows two dominant shear planes which cannot be classified according to Chinnery.
With 11 Figures 相似文献
ZusammenfassungSimulation von Störungen zweiter Ordnung im Computer Störungen zweiter Ordnung lassen sich mit einer bisher noch nicht gekannten Genauigkeit mit Hilfe einer von Malina (1969, 1970) entwickelten Programmversion der Finite-Element-Methode im Computer simulieren. Die Rechnungen zeigen, daß mit einer Scherbewegung entlang der Hauptstörung und dem Weiterreißen der Störung Spannungsumlagerungen einhergehen, die mitbewirken, daß neue sekundäre Störungen entstehen. Die ermittelten Störungen zweiter Ordnung lassen sich nach der Klassifikation von Chinnery (1966) als die ScherflächentypenA, B, E undF einordnen. Darüberhinaus liefert die Rechnung zwei sehr häufig auftretende Scherflächen, die sich nach Chinnery nicht klassifizieren lassen.
RésuméSimulation de failles de deuxième ordre par l'ordinateur Les failles de deuxième ordre peuvent être simulées avec une précision encore jamais atteinte grâce à l'utilisation d'une version d'une programme développé par Malina (1969, 1970) à partir de la méthode des éléments finis. Le calcul montre que, conjointement au cisaillement le long de la faille principale et à la propagation de cette faille, de nouvelles redistributions des contraintes apparaissent. Ces nouvelles redistributions contribuent essentiellement au développement de nouvelles surfaces de failles secondaires. Les failles de deuxième ordre peuvent être classées d'après Chinnery (1966) suivant les catégories de surfaces de cisaillementA, B, E, etF. De plus, le calcul indique fréquemment deux autres types de surfaces de cisaillement n'entrant pas dans la classification de Chinnery.
With 11 Figures 相似文献
15.
Melchiorri A Ade PA de Bernardis P Bock JJ Borrill J Boscaleri A Crill BP De Troia G Farese P Ferreira PG Ganga K de Gasperis G Giacometti M Hristov VV Jaffe AH Lange AE Masi S Mauskopf PD Miglio L Netterfield CB Pascale E Piacentini F Romeo G Ruhl JE Vittorio N 《The Astrophysical journal》2000,536(2):L63-L66
We use the angular power spectrum of the cosmic microwave background, measured during the North American test flight of the Boomerang experiment, to constrain the geometry of the universe. Within the class of cold dark matter models, we find that the overall fractional energy density of the universe Omega is constrained to be 0.85=Omega=1.25 at the 68% confidence level. Combined with the COBE measurement, the data on degree scales from the Microwave Anisotropy Telescope in Chile, and the high-redshift supernovae data, we obtain new constraints on the fractional matter density and the cosmological constant. 相似文献
16.
The migmatite complex of the Magrish area is part of a large crystalline massif south of Elat. The mineralogical composition of the migmatites is very uniform. The components of the melanosome are biotite, quartz and plagioclase, with small amounts of garnet and very rarely sillimanite and those of the leucosome — quartz and plagioclase. On the basis of chemical composition of the migmatites and possible premigmatitic parent rocks, absence of orthoclase in the leucosome, similar composition of plagioclase in the leucosome and in neighbouring melanosome, and Qz:Plag values which do not plot around a cotectic line, it is concluded that migmatisation occurred in a nearly closed system, without the presence of a melt phase. Thus, injection of granitic material, metasomatism or partial anatexis as possible main formation mechanisms are rejected and metamorphic differentiation is favoured. 相似文献
17.
18.
19.
20.
Cristiano Porciani Avishai Dekel Yehuda Hoffman 《Monthly notices of the Royal Astronomical Society》2002,332(2):325-338
We evaluate the success of linear tidal-torque theory (TTT) in predicting galactic-halo spin using a cosmological N -body simulation with thousands of well-resolved haloes. The protohaloes are identified by tracing today's haloes back to the initial conditions. The TTT predictions for the protohaloes match, on average, the spin amplitudes of the virialized haloes of today, if linear growth is assumed until ∼ t 0 /3, or 55–70 per cent of the halo effective turn-around time. This makes it a useful qualitative tool for understanding certain average properties of galaxies, such as total spin and angular momentum distribution within haloes, but with a random scatter of the order of the signal itself. Non-linear changes in spin direction cause a mean error of ∼50° in the TTT prediction at t 0 , such that the linear spatial correlations of spins on scales ≥1 h −1 Mpc are significantly weakened by non-linear effects. This questions the usefulness of TTT for predicting intrinsic alignments in the context of gravitational lensing. We find that the standard approximations made in TTT, including a second-order expansion of the Zel'dovich potential and a smoothing of the tidal field, provide close-to-optimal results. 相似文献