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181.
Time-relative positioning makes use of observations taken at two different epochs and stations with a single global positioning
system (GPS) receiver to determine the position of the unknown station with respect to the known station. The limitation of
this method is the degradation over time of the positioning accuracy due to the temporal variation of GPS errors (ionospheric
delay, satellite clock corrections, satellite ephemerides, and tropospheric delay). The impact of these errors is significantly
reduced by adding to the one-way move from the known to the unknown station, a back move to the known station. A loop misclosure
is computed from the coordinates obtained at the known station at the beginning and at the end of the loop, and is used to
correct the coordinates of the unknown station. The field tests, presented in this paper, show that using the loop misclosure
corrections, time-relative positioning accuracy can be improved by about 60% when using single frequency data, and by about
40% with dual frequency data. For a 4-min processing interval (an 8-min loop) and a 95% probability level, errors remain under
20 cm for the horizontal components and 36 cm for the vertical component with single frequency data; and under 11 cm for the
horizontal components and 29 cm for the vertical component with dual frequency data. 相似文献
182.
WEI Erhu LIU Jingnan SHI Chuang 《地球空间信息科学学报》2006,9(1):6-12
Introduction Astorealizetheprojectofspatialgeodesyby geodeticsatellites,itisnecessarytoestablisha satellitecontrollingandsurveyingnetwork(SC SN)totrack,tosurvey,toremotelycontroland tocommunicatewithearth orbitsatellite,forre alizingtheprojectofdeepspaced… 相似文献
183.
184.
梅雨期是江淮流域从春季到夏季一个重要的过渡时期。传统诊断入梅的方法主要根据雨日和温度及副热带高压位置等来确定。由于雨日的不连续, 天气形势的多变, 常会引起诊断入梅日期的分歧。利用长江三角洲地区地基GPS网所反演的连续的大气水汽总量 (GPS/PWV) 资料详细分析了长江三角洲地区2002—2005年入梅情况, 发现GPS/PWV资料可以反映出入梅前后大气中水汽发生显著季节性跳跃的特征, 总结出利用大气中水汽变化特征来诊断入梅时间的方法 (PWV方法)。采用1980—2000年的历史探空资料计算的大气水汽总量 (PWV) 资料, 对该方法进行了检验:21年中有13年的入梅日期与历史上传统方法诊断的入梅日期相吻合; 对两种方法诊断的入梅日期相差较大的3年的入梅情况进行的分析表明, PWV方法诊断出的入梅日比原定入梅日更合理。该方法在2006年入梅诊断的应用也得到验证。 相似文献
185.
Adrian A. Borsa Jean-Bernard Minster Bruce G. Bills Helen A. Fricker 《Journal of Geodesy》2007,81(2):157-170
We develop and test an algorithm for modeling and removing elevation error in kinematic GPS trajectories in the context of
a kinematic GPS survey of the salar de Uyuni, Bolivia. Noise in the kinematic trajectory ranges over 15 cm and is highly autocorrelated,
resulting in significant contamination of the topographic signal. We solve for a noise model using crossover differences at
trajectory intersections as constraints in a least-squares inversion. Validation of the model using multiple realizations
of synthetic/simulated noise shows an average decrease in root-mean-square-error (RMSE) by a factor of four. Applying the
model to data from the salar de Uyuni survey, we find that crossover differences drop by a factor of eight (from an RMSE of
5.6 to 0.7 cm), and previously obscured topographic features are revealed in a plan view of the corrected trajectory. We
believe that this algorithm can be successfully adapted to other survey methods that employ kinematic GPS for positioning. 相似文献
186.
Multipath error is considered one of the major errors affecting GPS observations. One can benefit from the repetition of satellite
geometry approximately every sidereal day, and apply filtering to help minimize this error. For GPS data at 1 s interval processed
using a double-difference strategy, using the day-to-day coordinate or carrier-phase residual autocorrelation determined with
a 10-h window leads to the steadiest estimates of the error-repeat lag, although a window as short as 2 h can produce an acceptable
value with > 97% of the optimal lag’s correlation. We conclude that although the lag may vary with time, such variation is
marginal and there is little advantage in using a satellite-specific or other time-varying lag in double-difference processing.
We filter the GPS data either by stacking a number of days of processed coordinate residuals using the optimum “sidereal”
lag (23 h 55 m 54 s), and removing these stacked residuals from the day in question (coordinate space), or by a similar method
using double-difference carrier-phase residuals (observational space). Either method results in more consistent and homogeneous
set of coordinates throughout the dataset compared with unfiltered processing. Coordinate stacking reduces geometry-related
repeating errors (mainly multipath) better than carrier-phase residual stacking, although the latter takes less processing
time to achieve final filtered coordinates. Thus, the optimal stacking method will depend on whether coordinate precision
or computational time is the over-riding criterion. 相似文献
187.
斜拉桥是一个受力结构复杂、各构件间相互影响较大的超静定结构体,斜拉索锚管的安装定位是其施工的重点与难点之一。本文结合湛江海湾大桥工程实践,介绍一种涉及到大跨度斜拉桥主塔锚管安装定位的原理、放样数据计算的理论、现场安装测量控制和精度等内容的新方法。 相似文献
188.
采用平差计算中得到的观测值的残差来估计指数函数经验模型中的参数,从而使随机模型更真实地反映观测值中的随机误差和偏差。由实际GPS观测数据厦广播里历,按以上的函数模型和随机模型采用逐次滤波方法进行解算。结果表明,此方法在未剔除和修复周跳的情况下,可以使单点静态定位的平面外符合精度达1.46m,高程方向的外符合精度为1.72m。 相似文献
189.
提出了利用精密单点定位(precise point positioning,PPP)技术进行海啸预警的方法,并利用TriP软件对实测浮标数据进行了处理,将得出的海面高数据和海啸波模型叠加进行了模拟分析。仿真结果表明,利用精密单点定位技术进行海啸预警,能够监测判断海啸的发生,并获得海啸波到达海岸的波高和时间,提供一定的预警信息。 相似文献
190.
C. M. Sykes I. W. A. Browne N. J. Jackson D. R. Marlow S. Nair P. N. Wilkinson R. D. Blandford J. Cohen C. D. Fassnacht D. Hogg T. J. Pearson A. C. S. Readhead D. S. Womble S. T. Myers A. G. de Bruyn M. Bremer G. K. Miley & R. T. Schilizzi 《Monthly notices of the Royal Astronomical Society》1998,301(2):310-314
We report the discovery of the most complex arcsec-scale radio gravitational lens system yet known. B1933+503 was found during the course of the CLASS survey and MERLIN and VLA radio maps reveal up to 10 components. Four of these are compact and have flat spectra; the rest are more extended and have steep spectra. The background lensed object appears to consist of a flat-spectrum core (quadruply imaged) and two compact 'lobes' symmetrically disposed relative to the core. One of the lobes is quadruply imaged while the other is doubly imaged. An HST observation of the system with the WFPC2 shows a galaxy with an axial ratio of 0.5, but none of the images of the background object is detected. A redshift of 0.755 has been measured for the lens galaxy. 相似文献