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971.
On the basis of local measurements of hydraulic conductivity,geostatistical methods have been found to be useful in heterogeneity characterization of a hydraulic conductivity field on a regional scale. However,the methods are not suited to directly integrate dynamic production data,such as,hydraulic head and solute concentration,into the study of conductivity distribution. These data,which record the flow and transport processes in the medium,are closely related to the spatial distribution of hydraulic conductivity. In this study,a three-dimensional gradient-based inverse method-the sequential self-calibration (SSC) method-is developed to calibrate a hydraulic conductivity field,initially generated by a geostatistical simulation method,conditioned on tracer test results. The SSC method can honor both local hydraulic conductivity measurements and tracer test data. The mismatch between the simulated hydraulic conductivity field and the reference true one,measured by its mean square error (MSE),is reduced through the SSC conditional study. In comparison with the unconditional results,the SSC conditional study creates the mean breakthrough curve much closer to the reference true curve,and significantly reduces the prediction uncertainty of the solute transport in the observed locations. Further,the reduction of uncertainty is spatially dependent,which indicates that good locations,geological structure,and boundary conditions will affect the efficiency of the SSC study results.  相似文献   
972.
刘杰 《东北测绘》2007,30(6):66-67
通过对GIS软件Arclnfo二次开发语言进行二次开发EDITtools软件,生产人员不用手工输入任何命令,完全脱离了键盘操作方式,通过菜单和按钮的点击即可完成调图、编辑、存盘以及产品整体质量检查,排除部分错误。改变现今数据生产的编辑作业操作模式,为基础地理信息数据成果数字化生产找到一奈较为经济、优质、高效的开发方法。  相似文献   
973.
通过分析3种传统数据模型的特点,得出它们在管理地理复杂对象方面的局限性,从而引出了面向对象数据模型。本文利用面向对象数据模型中的各种操作,以基本地理对象为基础构建复杂地理对象,并且在VC++6.0平台上实现了面向对象几何数据模型。  相似文献   
974.
用 2003-2005 年宣城市环境保护监测中心PM10、NO2、SO2自动监测资料、宣城市气象台地面观测资料和美国NCEP/NCAR全球日平均再分析资料,分析了宣城市区空气污染浓度、典型大气持续高污染过程形成的气象条件.结果表明,PM10、SO2平均浓度从春季到冬季逐渐增大,NO2平均浓度冬季明显偏小;PM10、NO2、SO2浓度存在准12 d周期变化.典型大气持续高污染过程的环流形势是500 hPa沿海为低槽,槽后为弱冷平流区;地面为宽广的均压区.1000~925 hPa主要为下沉气流;且上层增温明显大于低层,气层稳定度增大,这两种因素均使污染物扩散受阻;1000~700 hPa各层风力微弱,不能将污染物输送至远处,造成污染大气长时间维持.  相似文献   
975.
分别对比分析了晴天无云和台风影响出现强降水条件下南宁市气溶胶的变化特征。结果表明:大的降水和大的风速对南宁市气溶胶有较大的清除作用,风速的作用要大于降水的作用;在一定的风速条件下,降水对气溶胶的冲刷作用有限,当降水量达到一定程度之后,降水对气溶胶主要组分的清除作用不再明显;降水和风速对PM10的影响比SO2的明显;晴天条件下,PM10浓度占主要优势,强降水条件下SO2浓度占优势;强降水天气未能屏蔽交通活动对南宁市气溶胶的影响。  相似文献   
976.
老航片在考古中的应用研究   总被引:1,自引:0,他引:1  
通过国家863计划项目“考古遥感与地球物理综合探测技术”和国家历史博物馆项目“周王陵历史变迁研究”的研究成果,介绍了老航片在考古研究中的应用方法和应用效果。  相似文献   
977.
We present H α , [N  ii ] and [O  iii ] ground-based and HST archive images, VLA–A 3.6-cm continuum and H92 α emission-line data and high-resolution long-slit [N  ii ] spectra of the planetary nebula Hu 2-1. A large number of structural components are identified in the nebula: an outer bipolar and an inner shell, two pairs of collimated bipolar structures at different directions, monopolar bow-shock-like structures, and an extended equatorial structure within a halo. The formation of Hu 2-1 appears to be dominated by anisotropic mass ejection during the late-AGB stage of the progenitor and by variable, 'precessing' collimated bipolar outflows during the protoplanetary nebula and/or early planetary nebula phases. Different observational results strongly support the existence of a binary central star in Hu 2-1, among them (1) the observed point-symmetry of the bipolar lobes and inner shell, and the departures from axial symmetry of the bipolar lobes, (2) the off-centre position of the central star, (3) the detection of mass ejection towards the equatorial plane, and (4) the presence of 'precessing' collimated outflows. In addition, (5) an analysis of the kinematics shows that the systemic velocity of the bipolar outflows does not coincide with the systemic velocity of the bipolar shell. We propose that this velocity difference is a direct evidence of orbital motion of the ejection source in a binary system. From a deduced orbital velocity of ∼10 km s−1, a semimajor axis of ∼ 9–27 au and period of ∼ 25–80 yr are obtained, assuming a reasonable range of masses. These parameters are used to analyse the formation of Hu 2-1 within current scenarios of planetary nebulae with binary central stars.  相似文献   
978.
We present a detailed analysis of multi-frequency observations of linear polarization in the intraday variable quasar 0917+624 (z = 1.44). The observations were made in May 1989 at five frequencies (1.4, 2.7, 5.0, 8.3 and 15GHz) with the VLA and the Effelsberg 100 m-telescope and in December 1988 at two frequencies (2.7 and 5.0 GHz) with the latter. It is shown that the relationship between the variations of the polarized and total flux density is highly wavelength dependent, and the multi-frequency polarization behavior may be essential for investigating the mechanisms causing these variations. It is shown that the variations observed at 20 cm can be interpreted in terms of refractive interstellar scintillation. However, after subtracting the variation due to scintillation, three 'features' emerged in the light-curve of the polarized flux density, indicating an additional variable component. Interestingly, these features are shown to be correlated with the variations at 2-6 cm, thus indicating that thes  相似文献   
979.
We report a V band photometry of the SU UMa star IR Gem at quiescence in January 2002. The observations were made with two telescopes spaced - 160° apart in longitude. Several photometric modulations have been found. One gives a period of 98.50(13) min, exactly equal to the orbital period determined spectroscopically. Two others occasionally strengthen and seem to be positive and negative superhumps with periods of 103.6(4) and 95.4(4) min, 5.2% longer and 3.1% shorter than the orbital period, respectively. A signal at - 0.6 c/d in the power spectrum is roughly consistent with the expected period of nodal precession of the disk. There is a puzzling peak at 0.21(3) c/d corresponding to the - 4.3 d sine wave seen in the raw light curve. We suspect it to be a beat frequency between the frequencies of apsidal and nodal precessions of the disk. Quasi-periodic cycles with amplitudes 0.15-0.6 mag can be seen in the light curve. The mechanism underlying this modulation is not clear.  相似文献   
980.
The Solar Guide Telescope (SGT), an important solar attitude sensor of the SST (Space Solar Telescope, a space solar observing instrument being developed in China), can accurately produce pointing error signals of the SST for attitude control at high speed. We analyze in detail the error algorithm of the heliocentric coordinates and the edge judging of solar images. The measuring accuracy of ±0.5 arcsec of the SGT is verified by experiments on the tracking of the Sun and by testing a sun simulator. Some factors causing the pointing errors are examined.  相似文献   
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