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The outflow from the Sea of Okhotsk to the North Pacific is important in characterising the surface-to-intermediate-depth
water masses in the Pacific Ocean. The two basins are separated by the Kuril Islands with numerous straits, among which the
Bussol and the Kruzenshterna Straits are deeper than 1000 m. The physics governing the transport between the two basins is
complicated, but when the semidiurnal and diurnal tides are subtracted, the observed density and velocity structures across
the Bussol Strait suggest a significant contribution from geostrophic balance. Using a two-layer model with the interface
at 27.5σ
θ
, part of the upper layer transport that is not driven by tides is estimated using two previously unexplored data sets: outputs
from the Ocean General Circulation Model for Earth Simulator (OFES), and historical hydrographic data. The Pacific water flows
into the Sea of Okhotsk through the northeastern straits. The greatest inflow is through the Kruzenshtern Strait, but the
OFES results show that the contributions from other shallower straits are almost half of the Kruzenshtern inflow. Similarly,
the outflow from the Sea of Okhotsk is through the southwestern straits of the Kuril Islands with the largest Bussol Strait
contributing 60% of the total outflow. The OFES and hydrographic estimates agree that the exchange is strongest in February
to March, with an inflow of about −6 to −12 Sv (negative indicates the flow from the North Pacific, 1 Sv = 106 m3s−1), and an outflow from the Sea of Okhotsk of about +8 to +9 Sv (positive indicates the flow from the Sea of Okhotsk), which
is weakest in summer (−3 to +1 Sv through the northeastern straits and +0 to +3 Sv through the southwestern straits). The
estimated seasonal variation is consistent with a simple analytic model driven by the difference in sea surface height between
the two basins. 相似文献
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By means of in situ observation, the nucleation and growth of triclinic, pseudo-orthorhombic and pseudo-hexagonal CaAl2Si2O8 were investigated and their relative stabilities established. Pseudo-hexagonal and pseudo-orthorhombic CaAl2Si2O8 nucleate prior to anorthite and grow in a supercooled anorthite melt before the latter appears. They either dissolve or transform to anorthite once the latter nucleates and starts to grow. Corundum and mullite also nucleate metastably prior to anorthite in this melt. The liquidus temperatures of the four metastably nucleated phases were determined precisely by in situ measurements of the transformation temperatures from a polyhedral to a rounded morphology. On the basis of the supercooling thus determined, the growth rate versus supercooling relations were measured and analysed for the respective phases. The growth rate of the stable phase is one order of magnitude higher than those of any metastable phases. However, the growth rates of the three CaAl2Si2O8 polymorphs normalized by the viscosities are nearly the same. 相似文献
17.
Fission tracks and point defects in natural zircon are directly observed by a 1 MV electron microscope at atomic resolution for three types of samples adjusted to the 100 orientation. Lattice planes intersecting the fission tracks at high angles are distorted in a rather irregular manner over a wide region up to more than 100 Å wide. Diameter of the tracks, ranging from 25 Å to 40Å, is much narrower than those so far reported for the U-doped synthetic zircon (100–200 Å), UO2 thin film (100 Å), mica (66 Å, 240 Å) or fluorophlogopite (150 Å). The fact that fairly long tracks thousands of angstroms in length are observed in thin 100-oriented sample hundreds of angstroms in thickness and that some of them are nearly parallel to a low index lattice plane suggest a possible occurrence of channelling in the process of track formation. Parallel tracks often observed in chemically etched specimens support the idea of channelling. Slightly bent tracks are sometimes observed. It is concluded from computer simulation that many contrast anomalies of bright and dark spots in the lattice image are due to point defects of vacancies and interstitial atoms, mainly produced by the direct atomic collision with α-particles or by passage of ionizing nuclear particles. Optimum conditions of the observation of point defects with highest contrast are studied. One interstitial Zr atom or one Zr ion vacancy will give very low contrast and will be not detectable unless the crystal is less than two unit cells thick. A pair of Zr ion vacancies, however, yields extended detectable limit of thickness. Some of the observed defects are in good accordance with those simulated. 相似文献
18.
Mitsuhiko Hayashi Ichiro Tamura Osamu Shimomura Hiroshi Sawamoto Haruki Kawamura 《Physics and Chemistry of Minerals》1987,14(4):341-344
Néel temperature (Tm N of α-Fe2SiO4 (fayalite) was measured as a function of pressure by means of Mössbauer spectroscopy in the pressure range 0–16 Gpa. High pressure was generated using a clamp-type miniature diamond anvil cell which was inserted into a cryostat. The Néel temperature increased linearly with increasing pressure at a rate of dT N /dp=2.2±0.2 K/GPa. The result is discussed on the basis of the model proposed for the magnetic structure of fayalite by Santoro et al. (1966). The observed dT N /dp suggests that the superexchange interactions vary as the ?10/3 power of the volume while the volume dependence of the direct exchange interactions is positive and small. 相似文献
19.
Whole mantle SH velocity model constrained by waveform inversion based on three-dimensional Born kernels 总被引:1,自引:0,他引:1
Nozomu Takeuchi 《Geophysical Journal International》2007,169(3):1153-1163
A whole mantle SH velocity model is obtained by using a unique data set and techniques. Body and surface waveforms including major and multi-orbit phases are used as a data set and are inverted by using 3-D Born kernels. The resultant model, SH18CE, reveals the different natures of the two major upwelling systems: the strong low velocity anomalies beneath Africa extend for more than 1000 km from the core–mantle boundary (CMB), whereas those beneath the Pacific are restricted to 300–400 km from the CMB. The results also show the variable natures of stagnant slabs on the 670 discontinuity around Japan: the depths of the strongest high velocity anomalies within the stagnant slabs are different region by region, which is consistent with the detailed delay time tomography model in this area. 相似文献
20.