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231.
L.K. Amekudzi A. Bracher K. Bramstedt A. Rozanov H. Bovensmann J.P. Burrows 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(11):1921-1932
Vertical profiles of stratospheric nitrogen dioxide (NO2) have been retrieved from moderate resolution lunar occultation transmission spectra measured by Scanning Imaging Absorption spectroMeter for Atmospheric CHartographY (SCIAMACHY) on board the European Environmental Satellite (ENVISAT). These measurements were taken over the high southern latitude of 50°–90° during the period of 2003–2005. To assess the accuracy of the retrieved NO2 profiles, the SCIAMACHY nighttime NO2 profiles were compared with NO2 profiles retrieved from sunrise solar occultation spectra measured by the Halogen Occultation Experiment (HALOE) and the Stratospheric Aerosol and Gas Experiments II (SAGE II) using a photochemical correction model. The validation results show good agreement of SCIAMACHY lunar occultation NO2 with scaled HALOE and SAGE II profiles. The relative mean differences (rmd) with scaled HALOE profiles are within −13% to +5% and standard deviations (rms) of the relative differences are within 3–19% between 25 and 38 km. The rmd and rms with scaled SAGE II NO2 profiles are in the range of −9 to +7 and 10–17% respectively between 22 and 39 km. 相似文献
232.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(9):2203-2215
In this paper, the complexity and nonlinear trends of Radio Refractivity Gradient (RRG) in the troposphere over selected locations in Nigeria are analyzed and discussed extensively. The RRG is an important parameter in estimating path clearance and propagation effects such as ducting, surface reflection and multi-path on terrestrial line of-sights links. Also, radio wave signal propagating in the troposphere is affected by unpredictability of a weather condition which includes the variations of meteorological parameters such as temperature, pressure and relative humidity. The complex state of the atmosphere, which is the medium for the transmission of radio signals tend to have very strong influence such as scintillation and ducting on the quality of the radio signal, amplitude and phase. Variations in the meteorological parameters also induce variations in the refractive index of the atmosphere which in-turn results in the effect known as radio refractivity. For effective prediction and modeling of radio signal propagation, one should be able to characterize the nature and predictability of the computed RRG information. Chaotic Quantifiers (CQ) such as Phase Plot Reconstruction (PPR), Average Mutual Information (AMI), False Nearest Neighbor (FNN), Recurrence Plot (RP) and Recurrence Quantification Analyses (RQA) are used to assess the RRG. The information reveal, however, is based on the prediction techniques, design and frequency planning of microwave networks which may be useful for optimum performances during atmospheric turbulence. 相似文献
233.
当米波射电望远镜的观测视场内,有三个以上的射电源时,考虑天线跟踪的影响,提出了一种确定电离层行波扰动水平速度的新方法,并给出计算实例,讨论了误差。 相似文献
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235.
无线电掩星技术在大气探测的应用 总被引:1,自引:0,他引:1
通过介绍GPS在大气探测中的应用,引入了一种新的研究大气模型的方法——无线电掩星技术。阐明了无线电掩星技术的发展历程、反演原理及应用前景,并结合我国航天实际,提出了一种利用北斗导航系统进行大气参数反演,修正航天器轨道测量数据,从而提高定轨精度的新思路。 相似文献
236.
A space-based Very Long Baseline Interferometry (VLBI) program, named as the Cosmic Microscope, is proposed to involve dual VLBI telescopes in the space working together with giant ground-based telescopes (e.g., Square Kilometre Array, FAST, Arecibo) to image the low radio frequency Universe with the purpose of unraveling the compact structure of cosmic constituents including supermassive black holes and binaries, pulsars, astronomical masers and the underlying source, and exoplanets amongst others. The operational frequency bands are 30, 74, 330 and 1670 MHz, supporting broad science areas. The mission plans to launch two 30-m-diameter radio telescopes into 2 000 km×90 000 km elliptical orbits. The two telescopes can work in flexibly diverse modes. (i) Space-ground VLBI. The maximum space-ground baseline length is about 100 000 km; it provides a high-dynamic-range imaging capacity with unprecedented high resolutions at low frequencies (0.3 mas at 1.67 GHz and 20 mas at 30 MHz) enabling studies of exoplanets and supermassive black hole binaries (which emit nanoHz gravitational waves). (ii) Space-space single-baseline VLBI. This unique baseline enables the detection of flaring hydroxyl masers, and more precise position measurement of pulsars and radio transients at mas level. (iii) Single dish mode, where each telescope can be used to monitor transient bursts and rapidly trigger follow-up VLBI observations. The large space telescope will also contribute in measuring and constraining the total angular power spectrum from the Epoch of Reionization. In short, the Cosmic Microscope offers astronomers the opportunity to conduct novel, frontier science. 相似文献
237.
238.
多GNSS掩星大气探测卫星星座设计 总被引:1,自引:0,他引:1
为减少无线电掩星(RO)大气探测星座的卫星数量并增加探测数据量,将北斗(BD)和GPS、Galileo、GLONASS共同作为探测信源,提出一种多全球导航卫星系统(GNSS)掩星大气探测星座概念和优化设计方法。融合先验大气模型和二维射线追踪算法,建立兼容多GNSS信源的掩星事件前向模拟算法,实现掩星事件快速精确仿真;给出多GNSS掩星大气探测星座参数对探测性能的影响特性,降低了星座模型的复杂度;并利用改进的蚁群算法实现星座参数寻优。设计结果与COSMICII星座相比,卫星数量减少2颗,探测数据量增加了40%,探测均匀性提高了67%。 相似文献
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240.
首先对国内外黑障问题研究历史进行了回顾,然后从等离子体鞘套形成机理和基本特征、电波传播机理及信道特征等方面阐述了高超声速飞行器黑障问题的成因。随后,着重介绍了等离子体流场和电波传播数值模拟方法并分析了方法的适用性。进一步对等离子体地面模拟方法和诊断技术进行了概述,并对国内外地面黑障实验结果进行了详细分析。在此基础上,针对临近空间高超声速飞行器的特点,采用层次分析法(AHP)对现有黑障消除技术进行了评估,给出了目前工程实用方法、近期可能实现的工程实用解以及未来具有应用潜力的消除技术。最后,对黑障问题后续研究方向提出了几点建议。 相似文献