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81.
82.
Barotropic flows in a circular ocean are studied. Flows are driven by an inflow and an outflow through openings at the circumference. A linear, steady state solution is interpreted in terms of dissipating planetary waves. A weakly nonlinear, steady state solution is obtained numerically. It differs remarkably from the linear solution; an intense anticyclonic polar gyre extending over the whole basin is formed. The nonlinear term is essential to the gyre and can not be neglected, although the Rossby number is small. 相似文献
83.
Yoshimasa Toyota Satoru Kanamori Michihiko Kodama Masahiro Furukawa Shiro Okabe 《Journal of Oceanography》1982,38(5):307-312
Sea water samples, still hot from volcanic emanations were taken in a bay of Nishinoshima-Shintô Island just after volcanic activity had ceased and were analysed for borate-B, fluoride-F and bromide-Br. The hot water is considered to be formed by the conservative mixing of volcanic emanations with sea water, and the emanations containedCl, B, F andBr in the ratio of 1∶1.84×10?3∶0.474×10?3∶6.47×10?3 by weight. RatiosB/Cl andF/Cl can be used as effective measures of the contribution of volcanic emanations to sea water. 相似文献
84.
To save lives immediately after a catastrophic earthquake occurs, it is essential for an urban transportation system to retain
its functional performance in order to carry injured people to hospitals. Recent seismic assessment studies have mostly been
based on cost-benefit analyses, carried out in monetary terms that are reasonable for long-term considerations. However, many
problems of seismic risk management still remain. For example, attributing a monetary value to a human life is considered
impossible. Also, requirements for functioning of a transportation system are different in the period immediately after an
earthquake. This paper concentrates on how to assess the importance of an urban transportation system as it relates to saving
human life, and what system enhancements should be made to improve performance.
This paper proposes a risk assessment method for the functional reliability of a transportation system immediately after an
earthquake. In that period, system malfunction adversely affects the saving of lives as a result of time delays when moving
injured people to medical facilities. A system dynamics simulation of transporting injured people is incorporated in the method,
which uses two assessment approaches to evaluate the differences of cumulative injured people who receive medical care. In
deciding on the destination of medical facility in the simulation, two ways of deciding are addressed; one uses information
only on the road network, and the other uses information on both road network and hospital availability. Results of an application
to an actual target area show the most vulnerable road links and differences of the two decision-making processes. A way to
mitigate the loss due to damage to road links is examined. The paper also summarizes future developments in advanced information
technology for emergency transportation systems. 相似文献
85.
An equivalent-boundary method for the shell analysis of buried pipelines under fault movement 总被引:2,自引:0,他引:2
Introduction The history of research work on the response of buried pipeline under the fault movement hasbeen about 30 years. Several simplified design methods have been proposed to obtain the maxi-mum stress or strain in pipe. These methods include the theoretical method and the finite elementmethod (FEM). In the theoretical method, the pipe is usually modeled as a cable (Newmark, Hall1975; Kennedy, et al, 1977) or a beam (Wang, Wang, 1995; LIU, ZHANG, 2002). These theoreti-cal me… 相似文献
86.
87.
Abstract K–Ar age determinations were carried out on phengite separates from pelitic schists collected systematically from the Sanbagawa southern marginal belt and the associated area. The petrography and phengite chemistry by electron probe micro-analyzer (EPMA) revealed the existence of detrital white micas in the schist that have an extremely older age (108 Ma) in comparison with the neighboring schists (88 Ma) without any detrital mica. The ages become gradually older from the north ( ca 78 Ma) to the south ( ca 90 Ma) except for some samples that contain detrital micas and/or have been reactivated thermally by intrusives. The age is interpreted as an exhumation-cooling age that has been controlled by the ductile deformation of the host rocks that have never experienced a culmination temperature higher than 350°C which corresponds to the closure temperature of the K–Ar phengite system. The southward aging of the recorded ages in the extensive chlorite zone of the central Shikoku, from the Dozan river area of the north ( ca 65 Ma) to the study area of the south ( ca 85 Ma) through the Asemi river area ( ca 75 Ma), is explained in terms of increasing exhumation/cooling rates of the host rocks from north to south. The phengite K–Ar ages in the pelitic schists from the Kyomizu tectonic zone, which is classically considered as a remarkable thrusting shear zone, have no significant difference in comparison with that of the neighboring schists. This fact suggests that the latest stage of brittle deformation during exhumation/uplift has not significantly affected the ages of phengite in the schists. 相似文献
88.
Motohiko Kashima Shiro Imawaki Shin-Ichiro Umatani Hiroshi Uchida Yuji Hashibe Hiroshi Ichikawa Masao Fukasawa 《Journal of Oceanography》2003,59(3):291-301
Theoretically, the geostrophic approximation holds for the low-frequency flow field, but no detailed examination has been
done on how well the estimated geostrophic velocity corresponds with the observed velocity. Intensive surveys were carried
out during 1993–1995 in the Kuroshio and its recirculation regions south of Shikoku, Japan, including repeated hydrographic
surveys and direct current measurements at nominal depths of 700, 1500 and 3000 m. For these depth intervals, vertical differences
of estimated geostrophic velocity are compared with those of observed velocity. For the intermediate layer (between 700 and
1500 m depths), the slope of the regression line is 0.99, correlation coefficient is 0.98, and the root-mean-square of difference
from geostrophic balance is 2.8 cm/s which is close to the estimated error of 2.1 cm/s. For the deep layer (between 1500 and
3000 m depths), the corresponding values are 0.82, 0.93, 1.2 cm/s and 2.0 cm/s, respectively. The results indicate that the
estimated geostrophic velocity compares well with the observed velocity in these regions.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
89.
Bin?Qi Akinori?Takami Shiro?HatakeyamaEmail author 《Journal of Atmospheric Chemistry》2005,52(1):63-79
Concentrations of peroxy radicals were measured by a chemical amplification technique at a remote forested site as part of
the Program for Research on Oxidants in a Forested Region in Nikko (PROFRN). During the measurement period of 22–27 July 2002,
the mixing ratios of peroxy radicals averaged for 3 min at midday ranged from 109 to 134 pptv at a height approximately 5
m above the forest canopy. Significant diurnal variation in concentrations of peroxy radicals was observed, with the maximum
usually occurring around noon. Most of the variation was driven by changes in the intensity of solar radiation. However, it
was found that the peroxy radical concentration reached its peak about 3-h later than that of solar radiation on 24 and 26
July. The origins of this delay are discussed based on an analysis of the total radical budget in that period. A transport
of polluted air masses to the site was one of possible causes for the inconsistency. In addition, the measured peroxy radical
concentrations were compared with those derived from the deviations of NO-NO2-O3 photo-stationary state (PSSD) for clear days. The estimated half-hour-average concentrations of peroxy radical were in agreement
with the PERCA measured in the morning and late afternoon. However the two techniques differed by as much as a factor of two
during the time of near midday. 相似文献
90.
The previous eccentric-orbit binary model for the recurrent X-ray sources is modified by taking account of the velocity field of the stellar wind. The resultant formula of the light curves for the X-ray sources may have an useful application to the observed X-ray sources. 相似文献