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891.
利用江西省气象观测站降水资料、NCEP/NCAR提供的FNL 再分析资料以及GDAS 资料,在分析2020年7月7—10日的梅雨锋连续区域大暴雨过程的环流形势和大尺度水汽特征基础上,引入NOAA开发的HYSPLIT模式,分析了此次连续暴雨过程的水汽源地。结果表明:1) 此次连续性暴雨过程是在梅雨锋暴雨天气形势下,东北冷涡引导冷空气南下与副高北侧暖湿气流在长江中下游交汇形成的;2) 暴雨过程中不同时段水汽通道不相同,前两日以西南方向和偏南方向的水汽输送为主,后两日则以西南方向的水汽通道为主,且水汽通量大值区与强降水有较好的对应;3) 后向轨迹模拟显示暴雨过程水汽轨迹有5条:大部分为1 500 m高度以上源自印度洋的水汽(77.6%),其次是1 500 m高度以下源自印尼群岛中部海域的水汽(13.2%),其他三条路径总和不足10%。4) 垂直方向上,有多条水汽输送通道相互叠加后向暴雨区输送,导致江西上空产生强的水汽辐合。  相似文献   
892.
There is limited information available on CO2 concentration and flux over marsh. The objective of this work was to characterize CO2 concentration and flux within and above marsh plant (Carex lasiocarpa Ehrh. and C. pseudocuraica F. Schm) canopy at heights 0.5, 1.0 and 1.5 m. CO2 concentration was measured sequentially every 3 hours by using an infrared gas analyzer. Soil and air temperature, wind speed, net radiation and soil heat flux were also measured simultaneously. Extremely daily minimum and maximum CO2 concentration ranged from 250 to 754 μmd/mol for the 4-year work. The typical minimum and maximum values ranged from 314 to 464 μmol/mol at the height of marsh plant (about 0.5 m) during the fruiting period and mature date. The seasonal changes in CO2 concentration show that the minimum CO2 concentration occurred in the fruiting period and mature date, and both of their minimum values were 314 μmol/mol. This illustrates that CO2 consumed by photosynthesis was stable during the period. The flux of CO2 can be thought as a turbulent diffusion phenomenon. By micrometeorological methods, the diurnal CO2 fluxes were measured in the flowering period, fruiting period, early mature date, late mature date and yellow-ripe stage. Their values were −0.18, 38.15,24.13,10.9 and 4.91 μmol/mol respectively.  相似文献   
893.
As dust emission in the far infrared (FIR) is a characteristic property of planetary nebulae we searched the Infrared Astronomical Satellite (IRAS) point-source catalogue for confirmatory evidence on the two new possible planetary nebulae S 68 and 248 - 5 identified by Fesen, Gull & Heckathorn (1983) and the high-excitation planetary nebula 76 + 36 detected by Sanduleak (1983). We identify the nebulae 248 - 5 and 76 + 36 with IRAS sources 07404 - 3240 and 17125 + 4919, respectively and have determined their dust temperature, total FIR emission and optical depth. We also set a lower limit ranging in value from 1.2 × 10-6 to 3.7 × 10-5 forM dust /M bd of the nebula 248 - 5 depending on whether its grain material is silicate or graphite. S 68 could not be identified with an IRAS source.  相似文献   
894.
I.INTRODUCTIONIntherecentyears,theresearchershavepaidattentiontotheproblemsofcarbonbalanceandcarboncycleintheearthecosystem,withtheincreaseofCQZamountintheearthatmosphere.Mireisoneoftheecotypesinwhichcarbonaccumulationrateisthefastest,anditisthestrongestsinkforac(Branirgd,1980).Butthereislicitedinformationavailableaboutopconcentrationovermire.SomemeasurementsaboutthetemPOralandspatialgradientofopconcentrationhavebeenmadewithinoraboveasugarbeetcanopy(Brown,1970),corncanopy(Alien,1971;R…  相似文献   
895.
In this paper,fluxes of momentum and sensible heat are discussed with the data callected by tetheredballoon sounding system over the Philippine Sea during the cruise of the R/V SCIENCE 1 from Septem-ber through October in 1987.These fluxes were calculated using the semiempirical flux-profile relationshipsof Monin-Obkhov similarity theory with observed data.The friction velocity U.was determined by theobserved data's least-square fit with the similarity formulae under stable,neutral and unstable conditions.The roughness Z_0 was determined by Z_0=a_1(U./g),then substituted into the similarity formulae to com-pute U.again.The final values of U.and Z_0 could be determined through this iteration.The fluxtemperature θ.was calculated from the temperature profile with Z_0 determined above.Finally the fluxes'of momentum and sensible heat,and the drag coefficient C_D were obtained by computation with U.,θ.and the wind speed(U_(10))at 10 meters above the sea surface.  相似文献   
896.
Coronal Magnetic Flux Rope Equilibria and Magnetic Helicity   总被引:1,自引:0,他引:1  
1 INTRODUCTIONObservations show that the magnetic helicity of solar magnetic structures has a predominantsign in each hemisphere of the Sun, positive in the southern hemisphere and negative in thenorthern, regardless of the solar cycle (Rust, 1994). The magnetic helicity is strictly conservedin the frame of ideal MHD (WOltjer, 1958), and approximately conserved in the presence ofresistive dissipation and magnetic reconnection in a highly conductive plajsma (Taylor, 1974;Berger, 1984; H…  相似文献   
897.
The importance of the Baffin-Labrador region is explained in terms of the channelling through this area of the mass flux of meltwater from the Laurentide Ice Sheet and the probable effects of this on the thermohaline circulation of the North Atlantic. The chronology of glaciation and deglaciation in the region is summarised. Reference is made to recent marine records from the Baffin Shelf. Isotopic changes recorded in foraminiferal assemblages obtained from marine sediments in the Baffin Shelf-Labrador Sea area indicate the timing and possible magnitude of meltwater fluxes during the period 14.0-11.0 ka BP.  相似文献   
898.
介绍了地壳垂直运动的均衡理论 ,基于全球通量均衡基准 ,建立了任意坐标系下描述地壳垂直运动的动力学模型。该模型可表述为 L aplace方程的第二边值问题。将此模型与调和分析模型做了比较 ,认为此模型拟合精度较高 ,理论上更严密  相似文献   
899.
Results of the analysis of the Comet Halley spectrophotometry,which has been carried out by H.K. Nazarchuk in 1985 with the TVscanner of the 6-meter telescope (SAO, Russia) are presented. Timevariations in the intensities of the CN, CH, C2 and NH2bands were investigated using the series of spectra obtained inthe spectral region λλ=410÷ 510 nm. Theauto-correlation functions for all the bands, thecross-correlation functions for C2 lines and their Fouriertransformations are calculated to determine the frequencies andperiods of the variations. A possibility is considered thathigh-amplitude fast variations of spectral lines in Comet Halleyare caused by solar flares. The daily numbers of solar spots andproton fluxes with energies of more then 1 MeV are compared withthe spectral variations of these lines. It is shown that in theobservation periods the comet was projected onto an active regionof the Sun, but, among all the kinds of solar activity, mainlythe solar proton flux with energies less than 4 MeV coincides intime with fast intensity variations in the spectral lines. Analgorithm of cross-correlation analysis of discrete samplingseries with gaps is built, and average cross-correlation coefficientsare calculated.  相似文献   
900.
Based on the existing cumulus convective parameterization schemes,a mass flux scheme(MFS)for cumulus convective parameterization has been successfully developed by reference to thework of Chen et al.(1996).The MFS is a comprehensive scheme.In MFS,not only theimportance of the large-scale moisture convergence is taken into account,but also it includes thecumulus updrafts and downdrafts,cumulus-induced subsidence in the environmental air.entrainment,detrainment and evaporation.The interaction between the cumulus and theenvironment is described by using a one-dimensional bulk model.At the same time the schemeincludes the penetrative and shallow convections.The MFS has been successfully incorporated into the regional climate model RegCM2developed by NCAR.The new model has been applied to simulate summer monsoon characteristicsand their variations of heavy rainfall process in the Changjiang-Huaihe River Basins for threemonths from May to July 1991.The results show that the new model can successfully simulate thisrainfall prolonged process.By comparising the model outputs of RegCM2.using the Kuo schemeand the MFS.it is found that the MFS is better in simulating the surface temperature,rainfallposition and amount,and rainfall duration.  相似文献   
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