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991.
山东黄泛平原区浅层地下水丰富,但由于含水层岩性以粉砂为主,单井出水量小,井水含泥沙量高,井易淤易堵,因而影响该层地下水的开发利用。通过对填砾厚度与单井出水量及井水泥沙含量试验资料的分析,得出适宜细颗粒地层分布区成井的最佳填砾厚度为150~200mm。这一结论对该类地区浅层地下水开发利用具有指导意义 相似文献
992.
This paper discuses four stern difficulties and challenges faced by the development of grain production in China. According
to the basic national conditions of China and the amount of grain resources in the world market, China must meet the grain
demands mainly by her own domestic production. Using the input-occupancy-output techniques and system science methods, this
paper makes a forecast about China’s grain output, grain import and self-support rate in the year 2030.
The research was supported by the National Natural Science Foundation of China. 相似文献
993.
Manuela Cecconi Antonio DeSimone Claudio Tamagnini Giulia M.B. Viggiani 《国际地质力学数值与分析法杂志》2002,26(15):1531-1560
A constitutive model for granular materials is developed within the framework of strain–hardening elastoplasticity, aiming at describing some of the macroscopic effects of the degradation processes associated with grain crushing. The central assumption of the paper is that, upon loading, the frictional properties of the material are modified as a consequence of the changes in grain size distribution. The effects of these irreversible microscopic processes are described macroscopically as accumulated plastic strain. Plastic strain drives the evolution of internal variables which model phenomenologically the changes of mechanical properties induced by grain crushing by controlling the geometry of the yield locus and the direction of plastic flow. An application of the model to Pozzolana Nera is presented. The stress–dilatancy relationship observed for this material is used as a guidance for the formulation of hardening laws. One of the salient features of the proposed model is its capability of reproducing the stress–dilatancy behaviour observed in Pozzolana Nera, for which the minimum value of dilatancy always follows the maximum stress ratio experienced by the material. Copyright © 2002 John Wiley & Sons, Ltd. 相似文献
994.
Forms of phosphorus and silicon in the natural grain size surface sediments of the southern Bohai Sea 总被引:5,自引:0,他引:5
The forms of phosphorus and silicon in the natural grain sizes surface sediments of the southern Bohai Sea were studied. In sediments, the organic matter bound form of phosphorus was the main form of transferable phosphorus and ranged from 0.37μmol/g to 1.57μmol/g, accountingfor 10.7% of the total phosphorus, others were the carbonate bound form, iron-manganeso oxide bound form and ion-exchange able form; the transferable form of phosphorus accounted for 19.2% of the total phosphorus. Silicon‘ s carbonate bound form was predominant over others among its transferable forms, and content ranged from 1.55μmol/g to 8.94μmol/g, accounting for 0.05% of the total silicon; the total amount of transferable silicon forms accounted for only 0.12% of the total silicon. Therefore, 19.2% of the total phosphorus and 0.12 % of the total silicon contained in the surface sediments of the southern Bohai Sea could participate in the biogeochemical cycling. 相似文献
995.
According to the analysis of grain size, mineral composition and inclusion in quartz grain of the suspended and bed load sampled
from the Changjiang (Yangtze) River and the Huanghe (Yellow) River, the authors reveal the differentiation of loads between
the two rivers. In the Huanghe River the size of suspended load is coarser than that in the Changjiang River, while the bed
load is on the contrary. Through heavy mineral analysis, the biotite content of the Huanghe River loads is much higher than
that of the Changjiang River, and the monomorillonite content of the former is about two times higher than the latter. All
those may be attributed to the effects of different material sources and hydraulic conditions on load. The analysis of inclusion
in quartz grain definitely illustrates the environmental difference of material sources between the two rivers. In the meantime,
it provides a new method in seeking source of river load.
Subsidized by the National Natural Science Foundation. This paper is attributed to careful guidance from Prof. Wang Ying &
Prof. Shi Yunliang. 相似文献
996.
Philippe Stee 《Astrophysics and Space Science》2003,286(1-2):225-236
Interferometry in the visible provides milliarcsecond spatial resolution and thus has been used for studying the circumstellar
environment of active hot stars. In this paper I will illustrate how the visibility modulus and phase can be used to better
constrain the physics of Be disks through results from the VLA, the MkII and the GI2T interferometers. I will insist on the
importance and the potential of coupling high angular resolution with high spectral resolution to the study of Be shells.
Finally I will present a possible study of the circumstellar disk of Be stars using the VLTI.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
997.
998.
1 IntroductionSnowdensificationiscriticalforcalculationsinengineering glaciology,snowavalancheforecasting ,springflooding,andotherpracticalaspects.Itisalsoimportantforinterpretingicecoredataincludingthosetakenfromratherwarmsiteswheresurfacelay ersexperiencemelting ,sinceitwouldaffectthechangeofannuallayerthicknesswithtime.Whileextensivestudies(e.g .AndersonandBenson 1 963 ;Bader1 960 ,1 962 ;Koji ma 1 95 4,1 95 5 ,1 95 6,1 95 7,1 95 8,1 95 9,1 964;Keeler 1 967;Gow 1 975 ;MaenoandE binuma 1… 相似文献
999.
B. Sicardy C. Beaugé S. Ferraz-Mello D. Lazzaro F. Roques 《Celestial Mechanics and Dynamical Astronomy》1993,57(1-2):373-390
We review here some relevant problems connected to the evolution of circumstellar dust grains, subjected to Poynting-Robertson (PR) drag, and perturbed by first-order resonances with a planet on a circular orbit. We show that only outer mean motion resonances are able to counteract the damping effect of PR drag. However, the high orbital eccentricities reached by the particle lead to orbit crossings with the planet. This is a serious difficulty for a permanent trapping to be achieved. In any case, we show that the time spent in the resonance is long enough for statistical effects (accumulation at the resonant radius) to be significant. We underline some difficulties associated with this problem, namely, the non-adiabaticity of motion in the resonance phase space and the existence of close encounters with the planet at high eccentricities. 相似文献
1000.