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71.
在分析了几种传统的电机制动方案基础上,提出了一种适合陀螺马达的能耗制动方案,该方案依据马达逐渐停转时自身产生的微弱电信号,再经放大处理后作为能耗制动的控制信号,实现陀螺马达准确、可靠、平稳的停止,避免了不及时切断电源而烧坏定子绕组的情况. 相似文献
72.
本文研究的是以MCS-51系列单片机为核心的计算机控制系统,用以实现化工催化剂活性检测过程床层温度程序控制。被控对象是具有3~8分钟的纯滞后,时变,非线性特性的催化剂电加热炉。控制难度大。 采用了广义最小方差自校正控制算法,具有时变滞后的极点自校正PID算法,极点对消直接PID三种算法进行了仿真与现场试验研究。前两种,由于工作过程允许的信号对系统激励不够充分,对象在线辩识有困难,试验结果表现,不能实现预期的控制要求。最终采用了极点对消直接PID算法,成功地实现了催化剂活性温度自动控制。该系统工作稳定、可靠,控制精度达到了检测标准要求。 相似文献
73.
梁家昌 《中国民航学院学报》1994,12(3):79-87
通过变温与变激发强度的近红外光致发光研究了用MOCVD方法、生长在GaAs衬底上的Ga0.5In0.5P(GaInP2)外延薄膜的1.17eV发射带的发光特性。1.17eV发光带性质与0.99eV及0.85eV发光带的性质有着明显的差别。1.17eV发光带的机理可用施主-受主对的复合发光来解释,其中施主-受主对系白处在Ga格位上的Si(SiGa)及其最邻近的Ga空位(VGa)所组成,记作SiGa-VGa。考虑到GaInP2中存在着很强的电子-格子耦合作用及其Ⅲ族子格子为部分有序,所以在施主-受主对复合发光中应计及Franck-Condon位移△FC及该对在等效的部分有序势场中的相互作用能Es(DAP)。X—射线衍射实验表明,部分有序结构相当于成分调制,因而可用Kronig-Penney模型来计算Es(DAP)值。这样,我们就导出了施主-受主对复合发光的新的能量表示式。 相似文献
74.
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76.
Marian Karlický 《Space Science Reviews》2006,122(1-4):161-168
An acceleration process in the collapsing magnetic trap, formed in the flare with cusp magnetic field topology, is described.
Computations show that high-energy electrons are accumulated in the central part of the collapsing magnetic trap due to an
increase of their pitch angles. The effect explains in a natural way the formation of X-ray loop-top sources. Then, using
the model with the collapsing trap and considering only the adiabatic heating process, a possible explanation for the motion
of the X-ray loop-top source observed at the beginning of some cusp-type flares is presented. 相似文献
77.
Oxygen Isotopes in the Solar System 总被引:1,自引:0,他引:1
The oxygen three-isotope system has major advantages over the two-isotope systems of hydrogen, carbon, and nitrogen because
different fractionation laws govern intraplanetary and interplanetary processes. This permits discriminating between solar
nebular processes and parent-body processes. Oxygen isotopes also serve as a sensitive natural tracer for meteorite classification.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
78.
The spectral and polarization properties of thermal cyclotron radio emission from a hot coronal loop with a current along the axis are computed. The magnetic field is supposed to have a component along the loop axis as well as a poloidal part due to the current, both components being of comparable magnitude. In this specific configuration a helical magnetic field is present with a remarkable minimum of its absolute value along the loop axis and a maximum at its periphery. The presence of one or two maxima of magnetic field value along the line of sight results in increasing optical thickness of the gyroresonance layers at appropriate frequencies in the microwave band and, therefore, in enhanced radio emission at those harmonics which are optically thin (for example,s=4). These cannot be observed in models with the commonly employed magnetic field configuration (longitudinal along the loop axis).We show that the frequency spectrum of thermal cyclotron radiation from a hot coronal loop with a helical magnetic field differs from that of the standards-component source (with smooth frequency characteristics and polarization corresponding toe-mode) in that plenty of fine structures (line-like features and cut-offs) are present and theo-mode is prevalent in some frequency intervals. The enhanced radio emission at high harmonics and the complicated form of frequency spectrum in the model considered imply that some microwave sources, which are poorly explained in traditional models of solar active regions, may be associated with helical magnetic fields in hot coronal loops. Computations allow one to indicate spectral and polarizational peculiarities of local sources testifying to the presence of a helical magnetic field. 相似文献
79.
简要介绍了波音757-200客改装货时航电系统改装的主要工作内容和改装工作中的关键点,以及为保证整体改装工作的进度而实施的的创新手段。 相似文献
80.
Wiesław M. Macek 《Space Science Reviews》2006,122(1-4):329-337
The question of multifractality is of great importance because it allows us to investigate interplanetary hydromagnetic turbulence.
The multifractal spectrum has been investigated with Voyager (magnetic field) data in the outer heliosphere and with Helios
(plasma) data in the inner heliosphere. We use the Grassberger and Procaccia method that allows calculation of the generalized
dimensions of the solar wind attractor in the phase space directly from the cleaned experimental signal. We analyze time series
of plasma parameters of the low-speed streams of the solar wind measured in situ by Helios in the inner heliosphere. The resulting spectrum of dimensions shows a multifractal structure of the solar wind
attractor. In order to quantify that multifractality, we use a simple analytical model of the dynamical system. Namely, we
consider the generalized self-similar baker’s map with two parameters describing uniform compression and natural invariant
measure on the attractor of the system. The action of this map exhibits stretching and folding properties leading to sensitive
dependence on initial conditions. The obtained solar wind singularity spectrum is consistent with that for the multifractal
measure on the weighted baker’s map. 相似文献