主被动雷达复合制导中的主动通道最优辐射时机

反舰导弹复合导引头的主动通道在辐射时机取值上存在一个矛盾--过早辐射会增大过早暴露自身的风险,过晚辐射则有可能出现目标脱离视野范围或在最大过载情况下仍无法命中目标的问题。针对导弹仅在末制导阶段开启辐射的情况,提出了一种主动通道最晚辐射时机的求解方法,既保证了一定的命中概率,又降低了被敌方侦察截获的风险。     

磁悬浮柔性转子系统变学习速率单神经元PID控制

磁悬浮轴承柔性转子系统的转速范围较大,固定的控制参数很难同时保证系统所需的低频和高频特性。本文在一般单神经元PID控制的基础上,将转速信号引入磁悬浮轴承数字控制器,在不同转速段选择不同的学习速率以调节控制参数得到合适的磁悬浮轴承的刚度和阻尼。试验结果表明,变学习速率单神经元自适应PID控制能够明显减小转子在各阶临界转速时的振幅,有助于磁悬浮轴承柔性转子系统的安全稳定运行。     

一种新的泊位飞机阴影分割方法

飞机泊位自动引导系统中,识别跟踪定位泊位飞机时,会出现灰度较低区域被误判为阴影区域的现象,严重影响识别效果,因此分割飞机阴影是泊位成功与否的关键技术。提出一种将形态学的幂变换与无边界主动轮廓线模型结合的阴影分割方法,首先利用多方向权重形态学对泊位飞机图像中的噪声和微小的干扰区域进行滤除,然后进行幂变换来增强图像质量,最后利用无边界主动轮廓线模型分割阴影。实验结果表明,该方法不仅能够滤除噪声,保留图像细节,而且能提高分割阴影的精确度,并且抑制了泊位飞机分割产生的＂拖尾＂现象,有效地检测出运动飞机的阴影。     

X-ray redshifts with the International X-ray Observatory (IXO)

We explore the capabilities of the future space science mission IXO (International X-ray Observatory) for obtaining cosmological redshifts of distant Active Galactic Nuclei (AGNs) using the X-ray data only. We first find in which regions of the X-ray luminosity (L_X) versus redshift (z) plane the weak but ubiquitous Fe Kα narrow emission line can deliver an accurate redshift (δz < 5%) as a function of exposure time, using a CCD-based Wide Field Imager (IXO/WFI) as the one baselined for IXO. Down to a 2–10 keV X-ray flux of 10⁻¹⁴ erg cm⁻² s⁻¹ IXO/WFI exposures of 100 ks, 300 ks and 1 Ms will deliver 20%, 40% and 60% of the redshifts. This means that in a typical 18′ × 18′ IXO/WFI field of view, 4, 10 and 25 redshifts will be obtained for free from the X-ray data alone, spanning a wide range up to z ∼ 2–3 and fairly sampling the real distribution. Measuring redshifts of fainter sources will indeed need spectroscopy at other wavebands.     

词汇教学中的问题思考

词汇的记忆与掌握，对以后词汇的灵活和正确使用是非常必要的。对于任何语言的初学者来说，词汇的掌握都是一个繁重的任务。传统的词汇教学往往把重点放在学生的业余时间对词汇的机械记忆上，可是这种方法忽略了在课堂上来自于教师指导的重要性。本文建议每位教师在课堂上应该尝试创造不同的形式，以便学生能够积极主动而不是被动地学习词汇。     

主动引射高模试车台水喷雾冷却器等效热力系统模型的研究

水喷雾冷却器在主动引射高空模拟试车台中具有重要作用,其出口处温度的有效控制是保障试车正常运行的关键。针对某型号火箭发动机常压试验的喷雾冷却器,建立了等效热力系统模型,并在Simulink平台上建立了相应的动态仿真模型,计算结果与试车测试结果对比证明所建等效热力系统模型正确,从而为实现其出口处温度的有效控制提供依据。     

High resolution spectroscopy of Seyfert warm absorbers with XMM-Newton

We present results from the analysis of an XMM-Newton observation of the Seyfert 1 galaxy NGC 7469, the first high resolution X-ray spectrum of this source. The Reflection Grating Spectrometer (RGS) spectrum has several narrow absorption and emission lines of O, N, C and Ne, originating from gas at a range of ionisation parameters, from log ξ1.6 to log ξ−2 (where ξ has the units erg cm s⁻¹). We demonstrate that the ionisation state of the warm emitter is consistent with that of the high-ionisation phase of the warm absorber, and compare the warm absorber in this object with those in other sources.     

On the physical state in the narrow-line region of the classical Seyfert galaxy NGC 7469

Based on the spectrophotometric data, by decomposition of the observed continuum, the power - law continuum characteristics of the central source are obtained. The behaviour of both electron temperature T_e and density n_e in the Narrow - Line Region (NLR) of NGC 7469 is discussed on the thermal and ionization equilibria calculations. T_e in NLR of the Sy1 galaxies are higher than the Sy2 ones, and the possible explanation is the lack of the dense (n_e 10¹⁰ cm⁻³) zone close to the central source in the Sy2 galaxies.     

X-rays from the first massive black holes

X-ray studies of high-redshift (z > 4) active galaxies have advanced substantially over the past few years, largely due to results from the new generation of X-ray observatories. As of this writing X-ray emission has been detected from nearly 60 high-redshift active galaxies. This paper reviews the observational results and their implications for models of the first massive black holes, and it discusses future prospects for the field.     

Ultraviolet images of galaxies from the Optical Monitor on XMM-Newton

A large number of galaxies, both normal and active, have been observed in ultraviolet light by the Optical Monitor on XMM-Newton. These are some of the deepest wide-field ultraviolet images of these galaxies yet obtained, and in many cases the first collected in this waveband. We present images of five active galaxies, and discuss the potential uses of the ultraviolet surface brightness distribution and morphology, in association with X-ray data, for Active Galactic Nuclei, star formation and galaxy evolution studies.