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541.
为了促进中波红外面阵遥感相机遥感数据的应用,提出了一种在轨相对辐射定标方法。该方法根据两点定标原理,以中波红外面阵遥感图像数据为基础,利用在轨其他卫星数据获得相机入瞳处辐亮度,计算出非均匀性系数,从而实现在轨相对辐射定标。它为同类红外面阵遥感相机在轨相对辐射定标提供了一种新的思路,同时也可作为星上黑体标的一种校验手段。 相似文献
542.
基于地面图像和卫星图像集成的火星车定位新方法 总被引:1,自引:0,他引:1
提出了一种基于地面图像和卫星图像集成的火星车定位新方法,该方法利用由导航相机立体图像得到的火星表面的点云数据提取石块,同时对高分辨率卫星图像局部灰度统计提取石块,通过地面和卫星图像中石块分布模式的匹配,实现火星车在卫星图像中的定位,从而消除仅利用地面传感器和影像定位产生的累计误差。采用NASA勇气号火星车在多个摄站获取的地面图像以及HiRISE卫星图像进行了实验验证,结果表明这种方法在石块较多的地区能够取得很好的自动定位结果,定位误差小于HiRISE卫星图像的一个像素(0.25m)。 相似文献
543.
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545.
文章介绍了2004年CBERS-O2星热红外波段绝对定标工作,结合野外试验情况和数据处理过程深入进行了不确定性因素分析(包括误差分析),并从亮温反演的角度分析定标精度,进而针对如何提高在轨卫星热红外波段绝对辐射定标的精度,进行了探讨。 相似文献
546.
CCD遥感相机信号处理电路降噪方法 总被引:1,自引:0,他引:1
针对中国遥感高分辨率传输型相机的发展趋势,提出了一些降低信号处理电路噪声的方法;从信号完整性理论出发,利用电子设计自动化(EDA)工具Cadence软件进行了仿真与验证,并经实际电路测试验证取得了良好的效果。 相似文献
547.
Jean-Philippe Combe Thomas B. McCord 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The High Resolution Stereo Camera (HRSC) onboard the Mars Express spacecraft in orbit about Mars has four detector channels dedicated to produce images in four spectral channels. Utilizing these spectrophotometric data requires understanding the instrument radiometric calibration and other photometric properties of the data. We present here some results of our investigation into the HRSC color data characteristics. This covers comparison of HRSC measurements with those of telescopes and the Observatoire pour la Minéralogie, l’Eau, les Glaces et l’Activité (OMEGA) instrument, also on Mars Express. We also investigate the dependence of HRSC Color measurements on solar phase angle and altitude of the Mars surface. These results confirm and extend our earlier findings [McCord, T.B., Adams, J.B., Bellucci, G., Combe, J.-Ph., Hansen, G., Hoffman, H., Jaumann, R., Lumme, K., Neukum, G., Pinet, P., Poulet, F., the HRSC Co-I Team, The Mars Express high Resolution Stereo Camera spectrophotometric data: characteristics and science analysis. J. Geophys. Res. 112, E6, 2007.]. A basic finding from our study is that there are nearly constant offsets between the I/F value derived from the HRSC data and those determined from OMEGA and groundbased telescope measurements, especially in the HRSC red bandpass. These offsets are nearly independent of solar phase angle and Mars surface altitude but are considerably larger for the one comparison at Phobos we were able to make. Several hypotheses could explain these effects: atmospheric scattering, surface photometric effects, shift of the spatial registration or calibration. All these possibilities were investigated. 相似文献
548.
Experimental investigation on static/dynamic characteristics of a fast-response pressure sensitive paint 总被引:2,自引:0,他引:2
An optical-based technique using Pressure-Sensitive Paint(PSP) is a promising method to measure the distribution of surface pressure on an aerodynamic model. The static and dynamic characteristics of a fast-response PSP that is developed in the Chinese Academy of Sciences(CAS)are analyzed and tested to serve as the basis for experiments on unsteady surface measurement using a fast-response PSP. Two calibration systems used for this study are set up to investigate the temperature dependency, response time, and resolution. A data processing method, used for dynamic data, is analyzed and selected carefully to determine the optimum signal. Results show that the fastresponse PSP can be used normally at temperatures from 25 ℃ to 80 ℃. The effect of temperature on the accuracy of the measurement must be considered when temperatures are beyond the temperature range of 30–40 ℃. The dynamic calibration device with a solenoid valve can achieve a pressure jump within a millisecond order. The resolution is determined by the signal-to-noise ratio of the photo-multiplier tube. Results of the measurement show that the response time of the PSP decreases with a large pressure variation, and the response time is below 0.016 s when the pressure variation is under 40 kPa. 相似文献
549.
在标定捷联惯组加速度计时,一般采用多位置试验,但是目前并未对多位置试验所能标定出的误差系数数量和标定结果的有效性进行分析,本文针对这一问题展开了研究.首先,阐述了带有高次误差项的捷联惯组加速度计误差模型.然后,针对一般6位置标定方法无法完成这一模型标定的缺陷,提出了一种18位置标定方法.进行标定后,运用显著性分析方法,对误差模型本身和其中的参数的有效性进行了分析.最后,通过重复进行去除最不显著项、再标定、显著性检验等步骤,获得了试验室条件下所能标定的捷联惯组加速度计组合误差模型. 相似文献
550.
GPS-based sea level measurements to help the characterization of land contamination in coastal areas
P. Bonnefond P. Exertier O. Laurain P. Thibaut F. Mercier 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The Corsica site has been established in 1996 to perform altimeter calibration on TOPEX/Poseidon and then on its successors Jason-1 and Jason-2. The first chosen location was under the #85 ground track that overflight the Senetosa Cape. In 2005, it was decided to develop another location close to Ajaccio, to be able to perform the calibration of Envisat and in a next future of SARAL/AltiKa that will flight over the same ground tracks. Equipped with various instruments (tide gauges, permanent GPS, GPS buoy, weather station…) the Corsica calibration site is able to quantify the altimeter Sea Surface Height bias but also to give an input on the origin of this bias (range, corrections, orbits, …). Due to the size of Corsica (not a tiny island), the altimeter measurement system (range and corrections) can be contaminated by land. The aim of this paper is to evaluate this land contamination by using GPS measurements from a fixed receiver on land and from another receiver onboard a life buoy. Concerning the altimeter land contamination, we have quantify that this effect can reach 8 mm/km and then affects the Sea Surface Height bias values already published in the framework of the Corsica calibration site by 5–8 mm for TOPEX and Jason missions. On the other hand, the radiometer measurements (wet troposphere correction) are also sensitive to land and we have been able to quantify the level of improvement of a dedicated coastal algorithm that reconciles our results with those coming from other calibration sites. Finally, we have also shown that the standard deviation of the GPS buoy sea level measurements is highly correlated (∼87%) with the Significant Wave Height derived from the altimeters and can be used to validate such parameter. 相似文献