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131.
干涉SAR图像的降噪方法及水平地形效应消除 总被引:4,自引:1,他引:3
考察不同滤波器抑制干涉SAR(Synthetic Aperture Radar)图像噪声的效果.为有效地使用低通滤波处理,首先对原始干涉图像进行水平地形效应消除,保证图像信号频率的中心在零频处,降低由干涉SAR系统几何结构引起的信号频率偏移对滤波效果的影响.同时水平地形效应消除后的干涉SAR相位图可直观地反映地形的拓扑结构.实际数据处理结果证明本文提出的水平地形效应消除算法及滤波算法的可行性及有效性. 相似文献
132.
通过工艺试验和系统分析,研究出一套用真空感应铸造炉生产S-08钢铸件的工艺方法,解决S—08钢真空熔模精密铸造过程中的关键工艺技术问题,使S-08钢铸造的液氧/煤油发动机低压壳体、氧主阀下壳体等关键铸件满足高压、高冲击的负荷指标。 相似文献
133.
CompactPCI/PXI关键技术的发展与应用 总被引:2,自引:0,他引:2
CompactPCI技术具有高速、高性能、高可靠、热插拔、高可用、标准化、模块化、开放性等特点 ,被广泛应用于工业自动化、测量自动化、信息产业等领域 ,并正在迅速向其它领域扩展 ,同时其自身也处在不断地完善和发展过程中。本文综述了中国CompactPCI/PXI的关键技术发展及其应用。 相似文献
134.
135.
F. Marin F. Tamborra 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Asymmetric, broad iron lines are a common feature in the X-ray spectra of both X-ray binaries (XRBs) and type-1 Active Galactic Nuclei (AGN). It was suggested that the distortion of the Fe Kα emission results from Doppler and relativistic effects affecting the radiative transfer close to the strong gravitational well of the central compact object: a stellar mass black hole (BH) or neutron star (NS) in the case of XRBs, or a super massive black hole (SMBH) in the case of AGN. However, alternative approaches based on reprocessing and transmission of radiation through surrounding media also attempt to explain the line broadening. So far, spectroscopic and timing analyzes have not yet convinced the whole community to discriminate between the two scenarios. Here we study to which extent X-ray polarimetric measurements of black hole X-ray binaries (BHXRBs) and type-1 AGN could help to identify the possible origin of the line distortion. To do so, we report on recent simulations obtained for the two BH flavors and show that the proposed scenarios are found to behave differently in polarization degree and polarization angle. A relativistic origin for the distortion is found to be more probable in the context of BHXRBs, supporting the idea that the same mechanism should lead the way also for AGN. We show that the discriminating polarization signal could have been detectable by several X-ray polarimetry missions proposed in the past. 相似文献
136.
Luciana Bianchi Miriam Garcia 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We present an analysis of high resolution spectra in the far-UV – UV range (∼905–2000 Å) with non-LTE, spherical, hydrodynamical, line-blanketed models, of three O-type Galactic stars, and derive their photospheric and wind parameters. These data extend previously analyzed samples and fill a gap in spectral type coverage. The combined sample confirms a revised (downward) Teff scale with respect to canonical calibrations, as found in our previous works from UV and optical spectra, and in recent works by other authors. 相似文献
137.
Paola Marziani Jack W. Sulentic 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Quasars are the most luminous sources in the Universe. They are currently observed out to redshift z≈7 when the Universe was less than one tenth of its present age. Since their discovery 50 years ago astronomers have dreamed of using them as standard candles. Unfortunately quasars cover a very large range (8 dex) of luminosity making them far from standard. We briefly review several methods that can potentially exploit quasars properties and allow us to obtain useful constraints on principal cosmological parameters. Using our 4D Eigenvector 1 formalism we have found a way to effectively isolate quasars radiating near the Eddington limit. If the Eddington ratio is known, under several assumptions it is possible to derive distance independent luminosities. We discuss the main statistical and systematic errors involved, and whether these “standard Eddington candles” can be actually used to constrain cosmological models. 相似文献
138.
Chae Kyung Sim Huynh Anh Nguyen Le Soojong Pak Hye-In Lee Wonseok Kang Moo-Young Chun Ueejeong Jeong In-Soo Yuk Kang-Min Kim Chan Park Michael D. Pavel Daniel T. Jaffe 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We present a Python-based data reduction pipeline package (PLP) for the Immersion GRating INfrared Spectrograph (IGRINS), an instrument that covers the complete H- and K-bands in one exposure with a spectral resolving power of 40,000. The reduction steps carried out by the PLP include flat-fielding, background removal, order extraction, distortion correction, wavelength calibration, and telluric correction using spectra of A type standard stars. As the spectrograph has no moving parts, the PLP automatically reduces the data using predefined functions for the processes of order extraction, distortion correction, and wavelength calibration. Before the telluric correction of the target spectra, the intrinsic hydrogen absorption features of the standard A star are removed with a Gaussian fitting algorithm. The final result is the flux of the target as a function of wavelength. Users can customize the predefined functions for the extraction of the spectrum from the echellogram and adjust the parameters for the fitting functions for the spectra of celestial objects, using “fine-tuning” options, as necessary. Presently, the PLP produces the best results for point-source targets. 相似文献
139.
针对月球轨道交会对接地面高精度引导需求,对同波束干涉测量差分相延观测模型进行分析验证。根据甚长基线干涉测量几何时延观测量同一波前的定义,推导出同波束差分时延观测量的观测模型。并提出一种精确的同波束干涉测量差分相时延闭合算法,同时结合SELENE任务实测的数据计算差分相时延闭合值,用于对观测模型进行验证。实测数据计算结果表明,采用本文提出的精确算法显著地消除同一波前差分相时延闭合值中的趋势项,差分相时延闭合值的精度在0.5ps~1ps范围内,验证了观测模型的正确性。该研究对于后续的月球交会对接地面高精度测定轨任务分析设计将具有一定的参考价值。 相似文献
140.