1984年2月18日耀斑后环速度场的分析

本文研究了耀斑后环内物质在太阳重力、磁压力梯度和气体压力梯度联合作用下的下落运动,并在非等温状态及定常假定下计算了环内物质分布。计算结果表明:在环的中上部,下落运动可当作太阳重力作用下的自由下落运动;在环的底部,环内物质密度和磁场强度对物质下落运动影响较显着。     

Shortcomings of the Standard Solar Model

The SSM, invented in early nineteen sixties, remains a useful construction. There are now much larger number of its predictions that may be compared with observations than when it was first introduced. Seismic sounding based on oscillations frequencies provides the best test of the physical input for modelling stellar evolution. The results of the test must be viewed as a support for the standard theory of stellar evolution. However, significant differences in the sound-speed, photospheric He abundance, and other parameters between the Sun and the current models remain. Shortcomings in the EOS and in treatment of convection have been revealed. The differences in the sound-speed in the radiative interior may be explained by small opacity errors but other explanations are possible. Results of seismic sounding support the idea that the element mixing in the outer part of the radiative interior occurred during a significant fraction of the Sun's life. Such mixing is considered as a possible explanation of the deficit of lithium. The shortcomings of SSM cannot explain the deficits of measured neutrino fluxes. This revised version was published online in June 2006 with corrections to the Cover Date.     

Solar physics with the Square Kilometre Array

The Square Kilometre Array (SKA) will be the largest radio telescope ever built, aiming to provide collecting area larger than 1?km². The SKA will have two independent instruments, SKA-LOW comprising of dipoles organized as aperture arrays in Australia and SKA-MID comprising of dishes in South Africa. Currently the phase-1 of SKA, referred to as SKA1, is in its late design stage and construction is expected to start in 2020. Both SKA1-LOW (frequency range of 50–350?MHz) and SKA1-MID Bands 1, 2, and 5 (frequency ranges of 350–1050, 950–1760, and 4600–15,300?MHz, respectively) are important for solar observations. In this paper we present SKA’s unique capabilities in terms of spatial, spectral, and temporal resolution, as well as sensitivity and show that they have the potential to provide major new insights in solar physics topics of capital importance including (i) the structure and evolution of the solar corona, (ii) coronal heating, (iii) solar flare dynamics including particle acceleration and transport, (iv) the dynamics and structure of coronal mass ejections, and (v) the solar aspects of space weather. Observations of the Sun jointly with the new generation of ground-based and space-borne instruments promise unprecedented discoveries.     

Standard Solar Composition

We review the current status of our knowledge of the chemical composition of the Sun, essentially derived from the analysis of the solar photospheric spectrum. The comparison of solar and meteoritic abundances confirms that there is a very good agreement between the two sets of abundances. They are used to construct a Standard Abundance Distribution. This revised version was published online in June 2006 with corrections to the Cover Date.     

一种高稳定度帆板驱动系统的T-S模糊复合控制器

为减少帆板驱动机构（SADA）对太阳帆板挠性模态的激励作用,以扰动力矩较小的永磁同步电机(PMSM)作为驱动源,提出一种T-S模糊控制与校正网络相结合的控制方法。利用校正网络增加系统的相位裕度和增益,并通过T-S模糊控制器降低系统的超调和非线性摩擦的影响,从而有效抑制太阳帆板的振动。通过圆判据对带有此控制器的驱动系统进行了稳定性证明,很好地解决了模糊控制系统在摩擦扰动下难以进行频域理论分析的缺陷。仿真结果表明,在非线性摩擦等扰动的影响下,该控制方法能够很好地抑制太阳帆板引起的挠性振动,提高系统的速度精度和稳定度,具有较好的动态性能。     

太阳同步轨道卫星电源系统设计计算方法研究

给出了太阳同步轨道卫星电源系统的两种基本结构框架 ;分析了这两种结构的电源系统的设计计算方法 ;推导出了基于单圈能量平衡和多圈能量平衡的计算公式。以一个算例验证了该算法 ,并计算出所需太阳电池阵的面积和蓄电池组的容量 ,最后进行了能量平衡分析 ,得到了单圈或多圈能量平衡的结果。     

一种永磁同步电机宽速域无传感器系统的控制策略

设计了一种改进型滑模观测器(SMO)实现永磁同步电机(PMSM)无传感器宽速域控制。使用反电动势观测器替代低通滤波器,避免了转子位置信息滞后的问题。在定子电流计算中引入随转速自适应调节反馈系数的反电动势反馈,减小了系统抖振,使宽速域下转子转速和位置估计更加精确。采用锁相环技术(PLL)来抑制高频信息,提取出准确的转子位置。基于dSPACE搭建了PMSM的快速控制原型试验平台,对无传感器控制系统进行了稳态和动态试验,结果验证了该算法的有效性。     

磁悬浮电励磁三相直线同步电机离线参数辨识

建立磁悬浮电励磁三相直线同步电机(MSEETPLSM)的连续时间参数型状态空间方程数学模型,利用前向一阶差分方法将连续时间数学模型离散化成离散时间参数型状态空间方程数学模型,再利用z变换写成递推最小二乘算法标准形式的数学模型。利用递推最小二乘算法在初级转子静止状态下辨识出MSEETPLSM的电阻及自感参数。利用计算机数值仿真软件仿真MSEETPLSM参数的离线辨识算法,得到MSEETPLSM的初级与次级电阻与电感时域辨识曲线,仿真曲线收敛速度较快且辨识精度较高。仿真结果验证了该参数离线辨识算法的有效性。