ASAP: A systematic approach to plasma spectral synthesis

ASAP (Analysis System for Astrophysical Plasmas), developed at the Osservatorio Astronomico di Palermo, is a package of procedures based on IDL. It is aimed at the detailed presentation of theoretical models of astrophysical plasmas and the accurate comparison with observational data, up to fittings of specific observations. It is also useful for the prediction of specific observations, and for the simulation of the expected performances of forthcoming instruments, for instance those on board SOHO.     

大型民机增升装置噪声分析

随着低噪声发动机的使用,飞机机体噪声所占比例日益增大。尤其在飞机进场阶段,机体噪声中的增升装置噪声不容忽视。着重讨论了大型民机增升装置的噪声原理、降噪技术和预测方法,分析了增升装置前缘缝翼和后缘襟的流动特性,并阐述其噪声特性。然后对几种增升装置降噪技术的应用和发展进行了总结。最后介绍了气动噪声的几种预测方法。     

Efficiency tests for estimating the gas and stellar population parameters in Type 2 objects

We investigated the efficiency of estimating characteristics of stellar populations (SP) and Active Galactic Nuclei (AGN) emission using ULySS code. To analyze simultaneously AGN and SP components in the integrated spectrum of Type 2 active galaxies, we modeled the featureless continuum (FC) and emission lines, and we used PEGASE.HR stellar population models provided by ULySS. In order to validate the method, we simulated over 7000 integrated spectra of Seyfert 2 galaxies. Spectra were generated using different characteristics of the featureless AGN continuum, signal-to-noise ratio (SNR), spectral ranges, properties of emission lines and single stellar population (SSP) model whose initial mass function (IMF) and abundance pattern is similar to the solar neighborhood. Simulated spectra were fitted with ULySS to evaluate the ability of the method to extract SP and AGN properties. We found that the analysis with ULySS can efficiently restore the characteristics of SP in spectra of Seyfert 2 AGNs, where signal-to-noise ratio is higher than 20, and where SP contributes with more than 10% to the total flux. Degeneracies between AGN and SP parameters increase with increasing the AGN continuum fraction, which points out the importance of simultaneous fitting of the FC and SP contributions.     

高阶DG格式多重网格方法构造中的不同隐式策略影响研究

DG方法是一种非常具有潜力的高精度方法,但其在对复杂外形的数值模拟方面仍存在内存需求量大、计算量巨大等不足.为了进一步提高DG方法求解Euler方程的效率,在传统p型多重网格的基础上,结合LU-SGS和GMRES两种隐式迭代方法,研究其整体加速性能.p型多重网格方法通过对不同阶次多项式近似解进行递归迭代求解,来达到加速收敛的目的.高阶近似(p＞0)使用显式龙格库塔格式,最低阶近似(p=0)使用隐式格式.对NACA0012翼型和ONERA M6机翼跨音速无粘流动进行数值模拟,结果表明:与显式TVD-RKDG时间格式相比,DG(p0)层上采用LU-SGS和GMRES的p型多重网格方法收敛速度均得到明显提高,且GMRES迭代法性能最佳,LU-SGS迭代法次之.     

直线度误差测定中几个问题的探讨

讨论了在直线度误差测量中应注意遵循的几个原则：测量值直接作用原则、测量线与工作线一致原则和两测头联线垂直被测风面原则；建议以最小包容区域计算机精确算法作为今后评定直线度误差的主要方法；提出了一种新的最小包容区域计算机精确算法—“构造封闭凸多边形法”；在采样点测量值直接作用和非直接作用两种情况下，根据其采样点偏差值的分布，给出了相应的直线度误差的测量下确定度评定公式。