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91.
D.N. Mukhin A.M. Feigin Ya.I. Molkov E.V. Suvorov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,37(12):2292-II
A technique for retrieving vertical distributions (profiles) of atmospheric gas constituents from data of passive remote sensing of the atmosphere is proposed. The goal of the technique based on the statistical (Bayesian) approach to solution of inverse problems is construction of probability distribution for a sought quantity throughout the interval of the studied heights. It is assumed that initial data contain measurement noise, and a priori information about properties of the profile is used. It is proposed to approximate the sought profile by a function in the form of an artificial neural network. This approximation allows optimal inclusion of a priori information into retrieval procedure, thus ensuring the most effective regularization of the problem. Efficiency of the proposed technique is demonstrated on an example of retrieval of vertical ozone profile from data of ground-based sounding of the atmosphere in the millimeter wavelength range. Results of profile retrieval from model data and from spectra of radiation temperature of the atmosphere measured in the Apatity (67° N, 33° E) in the winter of 2002–2003 are presented. 相似文献
92.
紧缩平面场扫描架系统研制 总被引:3,自引:0,他引:3
紧缩平面场(CATR)是在较小的微波暗室里模拟远场的电磁环境,以行进各种天线的测量和研究.其最终性能指标要由紧缩平面场扫描架评定.根据紧缩平面场扫描测量原理,及其对扫描架平面度、直线度、定位精度及自动化程度的要求,研制了极坐标型紧缩场扫描架系统,通过采用高精度直线导轨、平面度微调方式和基于工业控制计算机的数字控制技术,达到了所要求的检测精度,满足了紧缩平面场扫描测量的要求. 相似文献
93.
数据链作用距离的试飞结果受试验区电波传播衰减影响很大,需要对其进行精确计算,为分析试飞结果提供支持.Fock级数法是计算电波衰减的一种精确方法,本文详细讨论了应用该方法求解试验区电波传播衰减的工程计算问题. 相似文献
94.
95.
Patrick A. Nsumei Bodo W. Reinisch Xueqin Huang Dieter Bilitza 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The ionospheric characteristics of the F2 layer peak have been measured with ionosondes from the ground or with satellites from space. The most common characteristics are the F2-peak density NmF2 and peak height hmF2. In addition to these two parameters this paper studies the F2-peak scale height. Comparing the median values of hmF2 and NmF2 obtained from topside and bottomside sounding shows good agreement in general. The Chapman scale height values for the F2 layer peak derived from topside profiles, Hm,top, are generally several times larger than Hm,bot derived from bottomside profiles. 相似文献
96.
LIU Hua YANG Jia-ling LIU Kai-xin 《中国航空学报》2007,20(3):210-214
Theoretical analysis and numerical calculations of Love wave propagation in layered graded composites with imperfectly bonded interface are described in this paper. On the basis of WKB method, the approximate analytic solutions for Love waves are obtained. By the interface shear spring model, the dispersion relations for Love waves in layered graded composite structures with rigid, slip, and imperfectly bonded interfaces are given, and the effects of the interface conditions on the phase velocities of Love waves in SiC/Al lay- ered graded composites are discussed. Numerical analysis shows that the phase velocity decreases when the defined flexibility parameter is greater. For the general imperfectly bonded interface, the phase velocity changes in the range of the velocities for the rigid and slip interface conditions. 相似文献
97.
Milan S. Dimitrijević Magdalena Christova Zoran Simić Andjelka Kovačević Sylvie Sahal-Bréchot 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Stark broadening parameters for 36 multiplets of B IV have been calculated using the semi-classical perturbation formalism. Obtained results have been used to investigate the regularities within spectral series and temperature dependence. 相似文献
98.
Rafik Hamdi Nabil Ben Nessib Sylvie Sahal-Bréchot Milan S. Dimitrijević 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Using semiclassical perturbation approach in impact approximation, we have calculated Stark widths for 32 spectral lines of doubly charged argon (Ar III). Oscillator strengths are calculated using Hartree–Fock method with relativistic correction (HFR) and an atomic model including 17 configurations. Energy levels are taken from NIST database. For perturbing levels for which the corresponding energy does not exist in NIST database, the calculated energies are used. Our widths are compared with the experimental results. The results presented here are of interest for modelling and investigation of stellar atmospheres since argon in different ionization stages is observed in many astrophysical objects. Finally, the importance of Stark broadening mechanism is studied in the atmospheric conditions of sdB stars. Electron impact Stark widths are compared to thermal Doppler widths as a function of temperature and optical depth of atmospheric layers. 相似文献
99.
N.F. Allard 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
In order to calculate the opacity of a gas it is necessary to consider how its constituent atoms are perturbed by the surrounding medium. This is required both in order to calculate the equation of state, and in order to determine the profiles of the spectrum lines. In this work we report new theoretical Li line profiles perturbed by H2 and their dependence with temperature. 相似文献
100.
Egidio Landi Degl’Innocenti 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
A century has elapsed since the first observation of the polarimetric profile of a line of the solar spectrum. Since then, dramatic progress has been made in the instrumentation, which is now reaching unprecedented levels of sensitivity in the measurement of polarization signals in solar spectral lines. At the same time, the theoretical framework needed for the interpretation of polarimetric observations has steadily evolved from the pioneering methods, based on simple formulae, to the sophisticated structure that is nowadays used with success in the interpretation of solar observations. The present paper is intended to give a historical perspective of the evolution of this research field and of its major achievements, with particular emphasis on the role played by the magnetic field in determining the polarimetric shapes of spectral lines. 相似文献