The Deep Impact Earth-Based Campaign

Prior to the selection of the comet 9P/Tempel 1 as the Deep Impact mission target, the comet was not well observed. From 1999 through the present there has been an intensive world-wide observing campaign designed to obtain mission critical information about the target nucleus, including the nucleus size, albedo, rotation rate, rotation state, phase function, and the development of the dust and gas coma. The specific observing schemes used to obtain this information and the resources needed are presented here. The Deep Impact mission is unique in that part of the mission observations will rely on an Earth-based (ground and orbital) suite of complementary observations of the comet just prior to impact and in the weeks following. While the impact should result in new cometary activity, the actual physical outcome is uncertain, and the Earth-based observations must allow for a wide range of post-impact phenomena. A world-wide coordinated effort for these observations is described.     

多架无人作战飞机攻击行为的协调

建立了基于Agent的无人作战飞机指挥控制系统的形式化语义模型，提出了无人作战飞机编队的联合作战目标、联合作战意图和协同攻击效能的定义，以及结合联合作战意图、协同作战效能的多架无人作战飞机编队攻击行为的协调方法。仿真结果表明，结合联合作战意图和协同攻击效能的攻击行为可有效地提高编队的作战效能。     

三维机翼大迎角低速绕流及其涡控制的数值模拟

通过数值求解三维非定常可压缩雷诺平均Navier-Stokes方程，研究了三维机翼大迎角低速绕流及其带表面周期性吹吸气的流动控制，并探讨了非定常质量引射作为外激发手段对机翼气动力特性的影响，计算表明，在机翼前缘附近的小区域内施加周期性吹吸气进行流动控制，这类外激发手段对三维机翼的大迎角分离流动的控制是可行的，通过选择适当的控制参数，尤其是合适的周期性激振频率，可以有效地改善气动力特性。     

Three-dimensional model of a dispersed-film flow in a cylindrical channel

A mathematical model of the dispersed-film two-phase flow with phase slip in the vertical cylindrical channel is described.     

气温的局部线性及多项式预测

利用局部线性预测法及局部多项式预测法,对气温非线性时间序列进行预测,并分析了预测误差,结果显示,局部线性预测法、局部多项式预测法对非线性时间序列具有良好的特性。     

An Overview of the Instrument Suite for the Deep Impact Mission

A suite of three optical instruments has been developed to observe Comet 9P/Tempel 1, the impact of a dedicated impactor spacecraft, and the resulting crater formation for the Deep Impact mission. The high-resolution instrument (HRI) consists of an f/35 telescope with 10.5 m focal length, and a combined filtered CCD camera and IR spectrometer. The medium-resolution instrument (MRI) consists of an f/17.5 telescope with a 2.1 m focal length feeding a filtered CCD camera. The HRI and MRI are mounted on an instrument platform on the flyby spacecraft, along with the spacecraft star trackers and inertial reference unit. The third instrument is a simple unfiltered CCD camera with the same telescope as MRI, mounted within the impactor spacecraft. All three instruments use a Fairchild split-frame-transfer CCD with 1,024× 1,024 active pixels. The IR spectrometer is a two-prism (CaF₂ and ZnSe) imaging spectrometer imaged on a Rockwell HAWAII-1R HgCdTe MWIR array. The CCDs and IR FPA are read out and digitized to 14 bits by a set of dedicated instrument electronics, one set per instrument. Each electronics box is controlled by a radiation-hard TSC695F microprocessor. Software running on the microprocessor executes imaging commands from a sequence engine on the spacecraft. Commands and telemetry are transmitted via a MIL-STD-1553 interface, while image data are transmitted to the spacecraft via a low-voltage differential signaling (LVDS) interface standard. The instruments are used as the science instruments and are used for the optical navigation of both spacecraft. This paper presents an overview of the instrument suite designs, functionality, calibration and operational considerations.     

The Tanaka-Enome criterion and solar activity in October–November 2003 as observed by the Large Pulkovo Radio Telescope

We present the results of spectral and polarization observations of two large sunspot groups, NOAA 0484 and NOAA 0486 + 0488, which determine high solar activity in October–November 2003. The observations are made with the Large Pulkovo Radio Telescope (LPRT) in the range 2.7–20 cm, the one-dimensional (E-W) resolution of observations being 1–6 arc min, respectively. The main characteristics of the corona radio emission above these active regions are measured, allowing us to follow their dynamics during the entire period of their existence on the solar disk with a period of one day. The analysis of the obtained results is presented from the point of view of the well-known Tanaka-Enome criterion [1–2] (on the basis of this criterion one can predict strong flares from characteristics of radio emission of an active region in quasi-quiet state). Using the activity in October–November 2003 as an example, we demonstrate the capabilities of a new method for estimating the level of solar activity. It was developed on the basis of long-term observations of the Sun by LPRT [3].Translated from Kosmicheskie Issledovaniya, Vol. 42, No. 6, 2004, pp. 585–594.Original Russian Text Copyright © 2004 by Borisevich, Ilin, Korzhavin, Peterova, Topchilo, Shpitalnaya.     

熵产控制体方法对压气机近零间隙流动损失的演变规律

以澄清近零间隙流动结构及流动损失随间隙的变化规律为目标,提出熵产控制体分析方法,可精确量化流场任意位置的局部不可逆损失.数值模拟发现,间隙在0.4%叶高范围内(称近零间隙)效率水平最高且出现一对应峰值效率最高的最佳非零间隙.熵产控制体分析表明:通道内总熵产随间隙变化规律与效率一致;间隙变化对动叶端区20%~80%弦长范围内的熵产改变最为明显,主导了总熵产的变化;间隙变化时熵产改变的流动区域不同,这是由于动叶端区主导损失的流动结构发生改变造成的.进一步结合流场结构,探讨近零间隙流动损失演变的可能原因:间隙为零时壁面剪切力是造成损失的主导因素;最佳间隙时流动均匀,损失最小.      

基于未知输入观测器的涡扇发动机直接推力控制

针对某型涡扇发动机,进行直接推力控制回路设计方法研究.基于未知输入观测器(UIO)原理建立了涡扇发动机机载模型和推力估计器,UIO通过解耦外界干扰实现了全飞行包线推力的准确估计;提出了直接推力闭环反馈控制的双回路结构设计方案,内环转速控制,外环推力控制,有利于实现各回路控制参数的独立设计.仿真验证结果表明:基于UIO的模型基涡扇发动机直接推力控制具有良好的控制稳定性和抗干扰性能,对于发动机不同工作点直接推力控制,推力控制误差不超过0.1%,转速控制偏差不超过0.2%.      

火箭仪器舱仪器安装板的振动控制试验研究

本文在对长Ⅲ甲运载火箭仪器舱进行了试验模态分析的基础上，对长Ⅲ甲运载火箭仪器舱进行了可控约束阻尼层主被动一体化振动控制试验研究，研究结果表明，可控约束阻尼层结构对火箭仪器舱这一大型复杂结构进行振动控制是非常有效的。