PWM型半桥式开关稳压电源的设计

介绍了一款基于PWM技术的半桥式开关稳压电源.给出了高频变压器、PWM控制及驱动电路的详细设计方法.用该方法设计了一台功率为150 W、输出电压为 15 V的半桥式开关稳压电源,并给出了实验波形.     

The Coma of Comet 9P/Tempel 1

As comet 9P/Tempel 1 approaches the Sun in 2004–2005, a temporary atmosphere, or “coma,” will form, composed of molecules and dust expelled from the nucleus as its component icy volatiles sublimate. Driven mainly by water ice sublimation at surface temperatures T > 200 K, this coma is a gravitationally unbound atmosphere in free adiabatic expansion. Near the nucleus (≤ 10² km), it is in collisional equilibrium, at larger distances (≥10⁴ km) it is in free molecular flow. Ultimately the coma components are swept into the comet’s plasma and dust tails or simply dissipate into interplanetary space. Clues to the nature of the cometary nucleus are contained in the chemistry and physics of the coma, as well as with its variability with time, orbital position, and heliocentric distance. The DI instrument payload includes CCD cameras with broadband filters covering the optical spectrum, allowing for sensitive measurement of dust in the comet’s coma, and a number of narrowband filters for studying the spatial distribution of several gas species. DI also carries the first near-infrared spectrometer to a comet flyby since the VEGA mission to Halley in 1986. This spectrograph will allow detection of gas emission lines from the coma in unprecedented detail. Here we discuss the current state of understanding of the 9P/Tempel 1 coma, our expectations for the measurements DI will obtain, and the predicted hazards that the coma presents for the spacecraft. An erratum to this article is available at .     

Deep Impact Mission Design

The Deep Impact mission is designed to provide the first opportunity to probe below the surface of a comet nucleus by a high-speed impact. This requires finding a suitable comet with launch and encounter conditions that allow a meaningful scientific experiment. The overall design requires the consideration of many factors ranging from environmental characteristics of the comet (nucleus size, dust levels, etc.), to launch dates fitting within the NASA Discovery program opportunities, to launch vehicle capability for a large impactor, to the observational conditions for the two approaching spacecraft and for telescopes on Earth.     

Thermoelectric Properties of Mg2Si1-xSnx Synthesized by Bulk Mechanical Alloying

Bulk mechanical alloying （BMA） has been successfully applied to solid-state synthesis of p-type and n-type thermoelectric materials Mg2Si1-xSnx （x = 0, 0.2, 0.4, 0.6, 0.8, 1） from element-powders at the room temperature in a relatively short time. The electrical conductivity, the Seebeck coefficient and the thermal conductivity of the Mg2Si1-xSnx are quite sensitive to the x-content. With the x-content rising, the electrical conductivity increases. When x = 0.6, it reaches the lowest and Mg2Si shows an n-type of semi-conducting However, when x = 0.2 and T 〉525 K, the Seebeck coefficient of the samples will change the opposite way. While x≥0.4, the samples present a p-type of semi-conducting. The figure of merit, Z of Mg2Si1-xSnx will be obtained in the range from 300 K to 700 K. When x = 0.6, Z proves to be higher than that of other samples at 300 K≤ T≤650 K.     

“嫦娥一号”卫星观测近月太阳风离子特征

"嫦娥一号"卫星的太阳风离子探测器(SWIDs)的科学目标是研究太阳风与月球的相互作用以及相应的近月空间等离子体环境。文章利用"嫦娥一号"卫星SWIDs探测器在2007年12月30日的观测数据对近月太阳风等离子体环境,包括向阳侧太阳风离子、"拾起"离子以及在月球尾迹边界处的太阳风离子的特征进行分析,得到以下主要观测结果:1)在慢速太阳风中观测到双峰结构,分别为太阳风中的氢离子和二价氦离子;2)在行星际磁场具有明显昏向(+By)分量期间,在月球向阳侧持续观测到有月表散射或反射后被拾起的太阳风离子;3)与入射的太阳风离子不同,这些拾起的太阳风离子具有明显的角度分布特征;4)在行星际磁场昏向(晨向)期间,太阳风中的氢离子在月球尾迹北半球的边界处呈现减速(加速)特征并进入尾迹;而并未发现氦离子进入尾迹的特征。"嫦娥一号"卫星的这些观测数据对于认识近月空间等离子体环境有着重要的意义。     

平流层飞艇流固耦合分析方法研究

平流层飞艇为了在平流层环境下获得足够的浮力,要求其体积庞大,由于跨度较大的充气柔性气囊结构容易发生变形,使得流固耦合特性非常显著。针对该类飞行器的流固耦合方法的研究是对其流固耦合特性分析的首要条件。本文基于流体动力学计算软件FLUENT和结构动力学分析软件ABAQUS,形成了分析平流层飞艇这类大型柔性充气结构流固耦合特性的非线性动态流体－结构交错积分耦合法。通过充气的圆球薄膜的解析解和NACA65A006机翼颤振特性的实验结果与计算结果的比较对该方法的有效性进行了分析。这为平流层飞艇流固耦合问题的研究提供了一种有效的分析工具,并对某平流层飞艇的突风干扰响应特性进行了分析,得出其流固耦合特性的变化规律。     

后掠翼边界层横流不稳定转捩预测模型

通过对经典Falkner-Skan-Cooke三维边界层相似解的理论分析和数值求解,结合二维边界层转捩判据的思想,采用由试验数据标定的C1准则关系式求解横流不稳定转捩位移厚度雷诺数,建立了针对固定前缘后掠角机翼的横流转捩判据,并且通过方程求解和数据拟合得到了该转捩判据的数学结果.应用该模型对30°前缘后掠角的ONERA-M6机翼和45°前缘后掠角的NLF(2)-0415无限展长机翼进行了横流不稳定转捩数值模拟.模拟结果显示:改进后的转捩模型预测所得到的转捩位置精度较高,均与后掠翼横流试验数据吻合较好,从而证明了构建的横流不稳定转捩判据的合理性和实用性.      

2A12 铝合金锻坯开裂故障分析

某产品用2A12铝合金锻坯在生产过程中发生开裂故障。本文对开裂锻坯进行了形貌观察与断口分析,并对比研究了热处理后开裂锻坯、未热处理锻坯和原材料铝棒。结果表明:开裂锻坯上的开裂模式为脆性开裂;开裂锻坯上的裂纹形成于热处理过程,形成原因应与锻造工艺控制不当导致锻坯在热处理过程中形成的粗晶有关。     

Spin parameters of Low Earth Orbiting satellites Larets and Stella determined from Satellite Laser Ranging data

Satellite Laser Ranging (SLR) measurements contain information about the spin parameters of the fully passive, geodetic satellites. In this paper we spectrally analyze the SLR data of 5 geodetic satellites placed on the Low Earth Orbits: GFZ-1, WESTPAC, Larets, Starlette, Stella, and successfully retrieve the frequency signal from Larets and Stella only. The obtained signals indicate an exponential increase of the spin period of Larets: T = 0.860499·exp(0.0197066·D) [s], and Stella: T = 13.5582·exp(0.00431232·D) [s], where D is in days since launch. The initial spin periods calculated from the first month of the SLR observations are: Larets: T_initial = 0.8239 s, Stella: T_initial = 13.2048 s. Analysis of the apparent effects indicates the counter-clockwise spin direction of the satellites. The twice more heavy Stella lost its rotational energy more than four times slower than Larets. Fitting the spin model to the observed spin trends allows determination of the spin axis orientation evolution for Larets and Stella before their rotational period becomes equal to the orbital period.     

Effects of simulated weightlessness on the intestinal mucosal barrier of rats

This study employed a rat tail-suspension model to investigate the effects of simulated weightlessness on the intestinal mucosal barrier. Twenty-four Wistar rats were randomly divided into control (CON), 14-day tail-suspension (SUS-14d), and 21-day tail-suspension (SUS-21d) groups (n = 8 per group). Expression of occludin and zonula occludins-1 (ZO-1), proteins of the tight junction (TJ), in the intestinal mucosa was measured by immunohistochemical analysis, Western blotting, and mRNA fluorescent quantitation PCR. Plasma concentrations of diamine oxidase (DAO) and d-lactate were determined using an enzymatic spectrophotometric assay. Expression of occludin and ZO-1 was reduced in the SUS-14d and SUS-21d groups as compared to the CON group, with lowest expression observed in the SUS-21d group (P < 0.01). Examination by transmission electron microscopy (TEM) of the jejunal epithelium revealed increased intercellular space, decreased TJ and desmosome densities, and destruction of microvilli in the SUS-14d and SUS-21d groups. Plasma DAO and d-lactate concentrations in the SUS-21d group were higher than those in SUS-14d group and significantly higher than those in the CON group (P < 0.01). In all three groups, the expression of occludin and ZO-1 was found to correlate negatively with DAO (P < 0.01) and d-lactate (P < 0.01) concentrations. It is concluded that simulated weightless results in down-regulation of expression of TJ proteins in the rat intestinal mucosa. Simulated weightlessness is proposed to increase intestinal permeability through damage to the TJ.