巡航导弹红外辐射及大气衰减计算模型

对巡航导弹3个主要辐射源:蒙皮、尾喷管及羽流进行了深入分析,建立了巡航导弹红外辐射计算模型.此外,在红外辐射的大气传输理论基础上,综合考虑高度、倾斜及气象条件等各种因素,分析了大气衰减对红外辐射的影响,建立了大气透过率的理论模型与计算方法.最后,以某型号巡航导弹为例,利用此模型计算了3~5μm和8~12μm两个波段的红外辐射强度、大气光谱透过率和平均透过率,以及经过大气衰减后的红外辐射强度,并对计算结果进行了分析.结果表明,这是一种计算巡航导弹红外辐射的简单方法.      

在大气紊流中飞行的弹性飞行器动力学模型

本文以大展弦比、后掠翼飞机和轴对称导弹为例,分别建立了弹性飞机和细长体弹性飞行器在大气紊流中飞行时的动力学模型。该模型考虑了非定常气动力的影响以及刚性运动和弹性变形模态之间的气动耦合作用,并给出了其状态空间方程的标准形式。     

对飞机纵向沉浮模态解析法的探讨

本文通过对现有沉浮模态各种近似解析解的分析比较，修正了经典解析法完全略去△ａ自由度的假设，计及了对此模态有相当影响的气动导数Ｃｍａ和Ｃｍｑ的作用，导出了沉浮模态二阶近似方程。算例结果证实，本方法具有较高精度，优于现有的几种近似解析解。     

The management of stray radiation issues in space optical systems

The performance of infrared and submillimeter systems can be severely degraded by stray light. Stray light includes off-axis radiation, system diffraction and scattering effects, and thermal self-emission. The purpose of this paper is to identify several keys to preventing system degradation due to stray radiation. The first key is to apply stray light design rules and analysis techniques early in the program before the design is finalized. A systems level analysis using stray light analysis software is often necessary in order to identify more subtle problems and to assess the magnitude of their effect on system performance. Another key is to address contamination control and the choice of surface coatings early in the program. The management of stray radiation issues is extremely cost-effective, if begun early in the program, and can reduce later schedule hardships.     

Measurement of Total and Spectral Solar Irradiance

The Sun’s electromagnetic radiation powers our solar system. In the case of the Earth it heats the lands and ocean, maintains our atmosphere, generates clouds, and cycles water. For other planets and minor bodies, similar and appropriate physical processes occur, also powered by the Sun. The Sun varies on all time scales and a precise knowledge of the Sun's irradiance and its variation is essential to our understanding of environments and physical conditions throughout our solar system. Measurements of solar irradiance and its variation can only be made from space, and almost thirty years of observation have now established that the total solar irradiance (TSI) varies by only 0.1 to 0.3%, while certain portions of the solar spectrum, the ultraviolet for example, vary by orders of magnitude more. This paper provides an overview of TSI observations and of spectral irradiance observations from the ultraviolet to the near infrared.     

Quality characteristics of the radish grown under reduced atmospheric pressure

This study addresses whether reduced atmospheric pressure (hypobaria) affects the quality traits of radish grown under such environments. Radish (Raphanus sativus L. cv. Cherry Bomb Hybrid II) plants were grown hydroponically in specially designed hypobaric plant growth chambers at three atmospheric pressures; 33, 66, and 96 kPa (control). Oxygen and carbon dioxide partial pressures were maintained constant at 21 and 0.12 kPa, respectively. Plants were harvested at 21 days after planting, with aerial shoots and swollen hypocotyls (edible portion of the radish referred to as the “root” hereafter) separated immediately upon removal from the chambers. Samples were subsequently evaluated for their sensory characteristics (color, taste, overall appearance, and texture), taste-determining factors (glucosinolate and soluble carbohydrate content and myrosinase activity), proximate nutrients (protein, dietary fiber, and carbohydrate) and potential health benefit attributes (antioxidant capacity). In roots of control plants, concentrations of glucosinolate, total soluble sugar, and nitrate, as well as myrosinase activity and total antioxidant capacity (measured as ORAC_FL), were 2.9, 20, 5.1, 9.4, and 1.9 times greater than the amount in leaves, respectively. There was no significant difference in total antioxidant capacity, sensory characteristics, carbohydrate composition, or proximate nutrient content among the three pressure treatments. However, glucosinolate content in the root and nitrate concentration in the leaf declined as the atmospheric pressure decreased, suggesting perturbation to some nitrogen-related metabolism.     

多功能大气探测激光雷达应用

激光雷达具有高的时间和空间分辨率、优越的方向性和相干性、高的探测精度和实时快速的数据获取能力，已经被广泛应用于大气探测、环境监测等领域。随着技术的发展，大气探测激光雷达由最初的单波长、单功能朝着多波长、多功能方向发展，技术更加成熟，操作更加方便。本文将介绍大气探测激光雷达的基本原理，及其在探测大气气溶胶和云、水汽、温度、污染物和大气边界层高度等方面的数据应用。最后，对多波长多功能大气探测激光雷达的数据应用发展进行了总结和展望。     

Mars Global MHD Predictions of Magnetic Connectivity Between the Dayside Ionosphere and the Magnetospheric Flanks

Atmospheric photoelectrons have been observed well above the ionosphere of Mars by the ASPERA-3 ELS instrument on Mars Express. To systematically interpret these observations, field lines from two global MHD simulations were analyzed for connectivity to the dayside ionosphere (allowing photoelectron escape). It is found that there is a hollow cylinder behind the planet from 1–2 R _M away from the Mars-Sun line that has a high probability of containing magnetic field lines with connectivity to the dayside ionosphere. These results are in complete agreement with the ELS statistics. It is concluded that the high-altitude photoelectrons are the result of direct magnetic connectivity to the dayside at the moment of the measurement, and no extra trapping or bouncing mechanisms are needed to explain the data.     

CF4/SF6反应气体对大气压等离子体温度的影响

为了探究CF4/SF6反应气体及其含量对大气压等离子体的温度的影响规律,采用红外热像仪记录等离子体反应区域的温度.实验结果表明在系统输入功率为260W时,对于CF4气体,等离子体区域的温度随着CF4含量的增加先升高然后降低;对于SF6气体,等离子体区域的温度随着SF6含量的增加而逐渐降低;在相同条件下,反应气体为SF6...     

某新型大气总温传感器的设计改进探讨

介绍了总温传感器的设计原理,并将国内外各型号进行对比和评价,提出了某新型总温传感器设计改进的方案原理.