全文获取类型
收费全文 | 218篇 |
免费 | 9篇 |
国内免费 | 6篇 |
专业分类
测绘学 | 2篇 |
大气科学 | 16篇 |
地球物理 | 50篇 |
地质学 | 62篇 |
海洋学 | 25篇 |
天文学 | 63篇 |
综合类 | 1篇 |
自然地理 | 14篇 |
出版年
2021年 | 4篇 |
2020年 | 2篇 |
2018年 | 5篇 |
2017年 | 6篇 |
2016年 | 3篇 |
2015年 | 8篇 |
2014年 | 2篇 |
2013年 | 5篇 |
2012年 | 4篇 |
2011年 | 8篇 |
2010年 | 5篇 |
2009年 | 7篇 |
2008年 | 6篇 |
2007年 | 12篇 |
2006年 | 15篇 |
2005年 | 12篇 |
2004年 | 12篇 |
2003年 | 14篇 |
2002年 | 8篇 |
2001年 | 9篇 |
2000年 | 6篇 |
1999年 | 11篇 |
1998年 | 2篇 |
1997年 | 5篇 |
1996年 | 1篇 |
1995年 | 3篇 |
1994年 | 2篇 |
1993年 | 5篇 |
1992年 | 4篇 |
1991年 | 4篇 |
1990年 | 1篇 |
1989年 | 5篇 |
1988年 | 1篇 |
1987年 | 1篇 |
1986年 | 4篇 |
1985年 | 3篇 |
1984年 | 1篇 |
1983年 | 3篇 |
1982年 | 1篇 |
1980年 | 3篇 |
1979年 | 2篇 |
1976年 | 1篇 |
1973年 | 1篇 |
1972年 | 3篇 |
1971年 | 1篇 |
1970年 | 2篇 |
1969年 | 4篇 |
1968年 | 2篇 |
1964年 | 1篇 |
1962年 | 1篇 |
排序方式: 共有233条查询结果,搜索用时 16 毫秒
101.
The paper provides a detailed analysis for the second-order diffraction of monochromatic waves. For the second-order potential on the free surface, the paper proposed a forward prediction method for computing the integration on the free surface. By this method we only need to run the infinity integration on the free surface directly for a few points; a one-step quadrature can then be applied successively outward from the body for potentials at other points. For wave diffraction from a body of revolution with a vertical axis, the paper derives a new integral equation, which can cancel the leading singularity in the derivative of ring Green's functions automatically. To obtain accurate results, different approaches are also used to deal with singularities in the ring Green's functions in the integration on both the body surface and free surface. The method has been implemented for bodies of revolution with vertical axes, but the theory is also available for arbitrary bodies.A numerical examination is made to validate the numerical code by comparing the second-order forces and moments on uniform and truncated cylinders and second-order diffraction potentials on the free surface with some published results. The comparison shows that the present results are in good agreement with those published. The method is also used to compute the second-order wave elevation around uniform and truncated cylinders. 相似文献
102.
Gradients of absorption line indices are studied and mean stellar metallicities are estimated for 46 elliptical galaxies.
The mean stellar metallicities range from 〈 [Fe/H] 〉 ≃ =0.8 to +0.2 and ellipticals with smaller central velocity dispersions
tend to have lower 〈 [Fe/H] 〉 thus the mass-metallicity relation holds not only for the galaxy center but also for the whole
part of the galaxy. There is an evidence that the magnesium is enhanced systematically in all ellipticals by 0.2 dex with
respect to the iron. Giant elliptical galaxies show lack of metal-poor stars (the G-dwarf problem). Metal-poor globular clusters
of ellipticals formed well in advance of the formation of metal-rich ones which formed simultaneously with the bulk of stars
of mother galaxies under the influence of galaxy chemical enrichment. The bimodal [Fe/H] distribution of globular clusters
does not necessarily mean that elliptical galaxies formed by the mergers of disc galaxies.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
103.
104.
The innermost region of slim accretion disks with standard viscosity is unstable against axisymmetric radial inertial acoustic perturbations under certain conditions. Numerical simulations are performed in order to demonstrate behaviors of such unstable disks. It is shown that oscillations with the period of 10–3 (M
BH/M
) s can be excited near the inner edge of the disks, whereM
BH is the mass of the central object. This kind of unstable disks is a possible origin of the periodic X-ray time variabilities with period of 104s observed in a Seyfert galaxy NGC 6814. 相似文献
105.
Chiaki Uyeda Akira Tsuchiyama Takamitu Yamanaka Muneyuki Date 《Physics and Chemistry of Minerals》1993,20(2):82-85
The harmonic oscillations of large diamagnetic mineral samples induced by a magnetic field is reported, for single crystals of quartz, corundum, and calcite. It was seen for the first time that the period of oscillation, , was proportional to the reciprocal of the magnetic field, H, where the restoring force of the string suspending the crystal became negligible in the high magnetic field. Accordingly, the value of diamagnetic anisotropy, , could be measured from the — H curve with a sensitivity of 5 × 10–10 emu/cc. The values were 5.50 × 10–9 emu/cc for quartz, 4.20 × 10–9 emu/cc for corundum, 9.9 × 10–8 emu/cc for calcite, and 8.8 × 10–8 emu/cc for polycrystalline talc piled with the (001) planes aligned parallel. Significant field-induced rotations were observed for the suspended crystals. When the field was applied along the direction of the diamagnetic hard axis of the stationary crystal, the crystal gradually rotated with increasing field, so that the direction of the hard-axis was perpendicular to the applied field. The field-induced energy has a the maximum value when the field is applied along the diamagnetic hard axis. This reorientation of the crystal occurs because the torque due to the field-induced anisotropic energy exceeds that of the restoring force in high magnetic fields. 相似文献
106.
Single crystalline San Carlos olivine (1 mm cube) was transformed to (Mg,Fe)2SiO4β-phase at 13.5–15 GPa, 1030–1330 °C for 0–600 min using a multi-anvil high pressure apparatus. The α-β transformation occurred
by incoherent surface nucleation and interface-controlled growth and recovered partially transformed samples showed sharply
defined reaction rim. The growth rate of the β-phase rim significantly decreased with time and the growth eventually ceased.
TEM observations revealed that many dislocations were created in both the relict olivine just near the α-β interface and the
β-phase in the rim, which show evidence for deformation caused by interfacial stresses associated with the misfit elastic
strain of the transformation. The observed tangled dislocation texture in β-phase suggested that the β-phase rim was hardened
and relaxation of the interfacial stress was retarded. This probably caused a localized pressure drop in the relict olivine
and decreased the growth rate. Time-dependent growth rates of β-phase is possibly controlled by the rheology of β-phase, which
must be considered for the prediction of the olivine metastability in the subducting slabs.
Received: 24 January 1997 / Revised, accepted: 24 July 1998 相似文献
107.
A. G. Rodnikov A. G. Gainanov B. V. Yermakov V. M. Kovylin V. A. Seliverstov Ya. B. Smirnov P. A. Stroev Yu. K. Shchukin T. Kato H. Shimamura 《Marine Geophysical Researches》1985,7(3):379-387
The paper presents the results of geological-geophysical research carried out during the Soviet-Japanese cooperative study of the structure and dynamics of the Earth's crust and upper mantle in the transition zone from the Pacific Ocean to the Asian continent. The 300 km deep geological-geophysical section of the tectonosphere (geotraverse) has been compiled on the basis of combined interpretations of seismic, geological, petrographic, gravimetric, magnetometric, electromagnetic and heat flow measurements. Estimates were made of deep temperatures along the geotraverse and of the depths of the partial melting level that can be identified with the upper boundary of the asthenosphere. 相似文献
108.
Giant Megamullion in the Parece Vela Backarc Basin 总被引:1,自引:0,他引:1
Ohara Yasuhiko Yoshida Tsuyoshi Kato Yukihiro Kasuga Shigeru 《Marine Geophysical Researches》2001,22(1):47-61
We present results of high-resolution bathymetric studies of the extinct intermediate-spreading Parece Vela Basin in the northwestern Pacific, where we have identified an extremely large mullion structure, here termed a giant megamullion. We find that the giant megamullion is nearly an order of magnitude larger than the similar structures in the slow-spreading Mid-Atlantic Ridge (`megamullions'). The giant megamullion has slightly elevated mantle Bouguer anomaly, and yields serpentinized peridotites and gabbros, suggesting that they are exposing oceanic crust and upper mantle. An off-axis rugged `chaotic terrain' was also identified in the Parece Vela Basin. The terrain consists of isolated and elevated blocks capped by corrugated axis-normal lineations, and associated deeps. We thus interpret it as analogues to the Mid-Atlantic Ridge megamullions. We propose that amagmatic tectonics producing the giant megamullion and the chaotic terrain occupied a significant part in crustal construction in the Parece Vela Basin evolution. 相似文献
109.
Michael A. Dopita Lawrence M. Krauss Ralph S. Sutherland Chiaki Kobayashi Charles H. Lineweaver 《Astrophysics and Space Science》2011,335(2):345-352
Recent observations show that the measured rates of star formation in the early universe are insufficient to produce re-ionization,
and therefore, another source of ionizing photons is required. In this Letter, we examine the possibility that these can be supplied by the fast accretion shocks formed around the cores of the most massive
haloes (10.5<log M/M
⊙<12) on spatial scales of order 1 kpc. We model the detailed physics of these fast accretion shocks, and apply these to a
simple 1-D spherical hydrodynamic accretion model for baryonic infall in dark matter halos with an Einasto density distribution.
The escape of UV photons from these halos is delayed by the time taken to reach the critical accretion shock velocity for
escape of UV photons; 220 km s−1, and by the time it takes for these photons to ionize the surrounding baryonic matter in the accretion flow. Assuming that
in the universe at large the baryonic matter tracks the dark matter, we can estimate the epoch of re-ionization in the case
that accretion shocks act alone as the source of UV photons. We find that 50% of the volume (and 5-8% of the mass) of the
universe can be ionized by z∼7–8. The UV production rate has an uncertainty of a factor of about 5 due to uncertainties in the cosmological parameters
controlling the development of large scale structure. Because our mechanism is a steeply rising function of decreasing redshift,
this uncertainty translates to a re-ionization redshift uncertainty of less than ±0.5. We also find that, even without including
the UV photon production of stars, re-ionization is essentially complete by z∼5.8. Thus, fast accretion shocks can provide an important additional source of ionizing photons in the early universe. 相似文献
110.
Variability of the central region in active galactic nuclei 总被引:3,自引:0,他引:3
Summary We review implications of the observed optical and X-ray variability (periodicities and light-curves), relevant for the understanding of physical conditions in the deep interiors of active galactic nuclei. We discuss in detail kinematical, hydrodynamical, thermal and radiative transfer effects which may be responsible for observed variability patterns. We put emphasis on theoretical options which can predict basic accretion parameters, such as the mass of the central black hole, the accretion rate and the inclination angle, in terms of observable quantities. Closed analytical results are given whenever available. 相似文献