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研究了设计参数具有固定容差的阵列天线方向图综合法;给出了阵列天线方向图容差优化的数学模型;提出了求解容差优化最坏情况问题的离散化方法;建立了直线阵列天线容差区内误差任意分布的物理模型,并采用修正正多面体优化方法对激励幅度具有容差的侧射天线阵进行了综合。当设计参数偏离其标称值时,文中的综合方法可以使天线性能的偏差最小。 相似文献
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文中对直升机红外抑制器椭圆截面喷管排气的辐射热流进行数值分析,并预估排气温度分布、速度和燃气成分分布对辐射热流的影响。为了计算辐射热流和考虑尾焰对周围环境的传热,采用形式简单并可用通用方程计算程序计算的六热流辐射模型。由于排气流场内温度和密度变化较大,故紊流模型采用考虑密度变化的修正双方程k-ε模型。本文中所用的比热C_(pm)是随气流温度和成分而变化,温度用迭代法求得。喷管出口截面为椭圆形,排气为三元自由射流,控制方程为三元抛物形偏微分方程,可采用前进积分求解,这样既可满足计算精度要求,又可节省机时。并根据三元喷流周向边界条件周期性变化的特点,采用CTDMA解法。计算结果与试验结果基本一致,说明本计算方法是可行的。 相似文献
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柱面菲涅耳太阳聚光透镜的光学设计和光学效率 总被引:1,自引:1,他引:1
研究了柱面线聚焦菲涅耳太阳聚光透镜的光学设计和光学效率。依据理论分析,对透镜参数进行了优化设计,成功地研制出了柱面线聚焦菲涅耳聚光透镜。还分析了透镜相对孔径(F数)和成型模具等因素对透镜光学效率的影响。 相似文献
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N. Kylafis D. Giannios D. Psaltis 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2810-2812
We propose a jet model for the low/hard state of galactic black-hole X-ray sources which explains the energy spectra from radio to X-rays and a number of timing properties in the X-ray domain such as the time lag spectra, the hardening of the power density spectra and the narrowing of the autocorrelation function with increasing photon energy. The model assumes that (i) there is a magnetic field along the axis of the jet, (ii) the electron density in the jet drops inversely proportional to distance, (iii) the jet is “hotter” near its center than at its periphery, and (iv) the electrons in the jet follow a power-law distribution function. We have performed Monte Carlo simulations of Compton upscattering of soft photons from the accretion disk and have found power-law high-energy spectra with photon-number index in the range 1.5–2 and cutoff at a few hundred keV, power-law time lags versus Fourier frequency with index 0.8, and an increase of the rms amplitude of variability and a narrowing of the autocorrelation function with increasing photon energy as they have been observed in Cygnus X-1. The spectrum at long wavelengths (radio, infrared, optical) is modeled to come from synchrotron radiation of the energetic electrons in the jet. We find flat to inverted radio spectra that extend from the radio up to about the optical band. For magnetic field strengths of the order 105–106 G at the base of the jet, the calculated spectra agree well in slope and flux with the observations. 相似文献
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G. Smoot G. De Amici S.D. Friedman C. Witebski N. Mandolesi R.B. Partridge G. Sironi L. Danese G. De Zotti 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
New measurements of the Cosmic Background Radiation temperature at 12 cm, 6.3 cm, 3 cm, 0.9 cm and 0.3 cm have made in July 1982 from the White Mountain High Altitude Research Station. The results are presented and the existence of spectral distortions discussed. 相似文献
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Silvia Zane Roberto Turolla Luciano Nobili Nanda Rea 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
In this paper, we discuss our first attempts to model the broadband persistent emission of magnetars within a self-consistent, physical scenario. We present the predictions of a synthetic model that we calculated with a new Monte Carlo 3D radiative code. The basic idea is that soft thermal photons (e.g. emitted by the star surface) can experience resonant cyclotron upscattering by a population of relativistic electrons treated in the twisted magnetosphere. Our code is specifically tailored to work in the ultra-magnetized regime; polarization and QED effects are consistently accounted for, as well different configurations for the magnetosphere. We discuss the predicted spectral properties in the 0.1–1000 keV range, the polarization properties, and we present the model application to a sample of magnetars soft X-ray spectra. 相似文献