The spatial distributions of the sources of UV solar Explosive Events at different velocities

We analyze five solar Explosive Events observed in the Si iv emission line at 139.37 nm during SUMER/SoHO raster scans near disk center. The Doppler velocities from −45 km s⁻¹ to +45 km s⁻¹ were sorted into eleven symmetrically organized velocity bins, five equally-sized bins on each side and one bin for the line at rest. The radiance values along the NS oriented slit around the maximum of each EE are used to build one-dimensional distributions. We study these distributions and their development in space and time for different velocity bins to unveil the 3D-structure and evolution of Explosive Events. The spatial radiance distributions for the EE maximum and around it were made. For some Explosive Events the dispersion direction is not oriented orthogonally to the slit direction; consequently, the blueshifted emission is in a linear way offset from the redshifted emission by several pixels. The largest offset (∼5″) is observed between distributions whose velocities differ by ∼36 km s⁻¹. The linear relation agrees with an scenario of flows inside magnetic arcs.     

孙中山民生主义的理论流变及现实意义

孙中山先生的民生主义学说是其三民主义思想的重要组成部分,这一思想的形成经历了一个历史过程。从理论渊源来看,既有中国传统政治思想中民本主义思想的影响,也有对西方资本主义政治经济学有关内容的吸纳,还受到社会主义思想的影响。民生主义提出后,在不同的政治势力之间引发了激烈的争论,这种争论也推动了孙中山三民主义的不断发展演变。民生主义学说对于当代中国民生问题具有重要的启示和借鉴意义。     

Metric radio bursts and fine structures observed on 17 January, 2005

A complex radio event was observed on January 17, 2005 with the radio-spectrograph ARTEMIS-IV, operating at Thermopylae, Greece; it was associated with an X3.8 SXR flare and two fast Halo CMEs in close succession. We present dynamic spectra of this event; the high time resolution (1/100 s) of the data in the 450–270 MHz range, makes possible the detection and analysis of the fine structure which this major radio event exhibits. The fine structure was found to match, almost, the comprehensive Ondrejov Catalogue which it refers to the spectral range 0.8–2 GHz, yet seems to produce similar fine structure with the metric range.     

巴拉克·奥巴马胜选演说翻译的生态学视角

从生态学视角研究翻译的整合性。基于翻译适应选择论,分别从语言维、文化维和交际维分析奥巴马胜选演说三个中译本的适应性选择转换情况,指出应注重体现翻译生态系统的整体性,注意语言维、文化维和交际维等多维度的有机结合。在翻译过程中力求做出与翻译生态环境相适应的选择,达到兼顾原文原语、译语和译语读者之间平衡和协调的目的。     

一种基于HMM的多用户检测算法

针对以概率统计为基础信道估计收敛速度慢、状态估计存在非合理性的问题进行研究,提出了一种新的多用户检测方法.该算法以隐马尔可夫模型为基础,为了避免由于相邻状态序列后向概率相差很大而造成的信道估计发散,采用固定延迟的方法,利用锯齿延时的办法计算后向序列概率以减少计算复杂度.根据前后序列之间的相关性和最陡下降法,提出了解相关最小均方(DLMS)多用户上行复合信道的盲估计. 考虑到由于发射序列状态之间可能存在时序非继承性,而搜索与前向序列对应的具有最大转移概率的后续序列,给出了最大后验(MAP)多用户检测方法.计算机仿真实验表明,该算法提高了信道响应估计速度,具有全局收敛性和系统的稳定性.      

FY—1C卫星空间粒子成分监测器及其探测结果

简要介绍了FY－1C星空间粒子成分监测器的任务目标、工作原理、创新特色及在轨探测结果。空间粒子成分监测器用于卫星轨道空间的带电粒子辐射监测，为卫星的在轨安全和抗辐射加固设计服务。监测器在世界上实现用1套传感器完成对高能电子、质子、α粒子至铁离子的全成分监测，使我国首次获得了870km高太阳同步轨道全空间的各种重离子分布、质子能谱分布和电子通量分布，捕捉到大量的地磁暴和太阳质子事件，获得了批重要的探测成果。     

空间太阳X射线成像望远镜技术

阐述了空间太阳X射线成像望远镜(SXT)在近地环境空间天气观测中的作用和意义。介绍了国内外SXT技术的发展和应用情况，分析了仪器的工作原理、主要观测目标和应具备的基本功能以及关键部件。     

橡胶"O"形密封圈结构参数和失效准则研究

利用大变形、接触的非线性有限元理论建立了某固体火箭发动机密封结构的二维轴对称模型,用有限元软件计算出该结构在工作状态下的变形和应力。通过计算可知,在橡胶“O”形密封圈与上下法兰接触的位置产生最大的接触压应力,在密封槽槽口转角位置产生最大的剪切应力。对密封性能的各结构参数进行了分析,讨论了上下法兰张开间隙、初始压缩率、密封槽槽口及槽底倒角半径、密封槽宽、密封圈材料等典型参数的影响:上下法兰张开间隙、密封圈的初始压缩率对最大接触压应力的影响较大,而密封槽槽口和槽底处倒角半径对剪切应力影响明显。三维壳体结构的有限元分析结果表明,上下法兰在内压作用下产生不均匀的张开间隙,体现了三维结构的特点。不均匀的张开间隙与二维轴对称结果对比可知,以最小间隙作为设计间隙,二维轴对称分析模型可取代三维模型来分析该结构的密封性能。最后,确定了“O”形圈密封结构的最大接触应力和剪切应力失效准则。     

On mid-term periodicities of high-latitude solar activity

The mid-term periodicities of polar faculae are studied separately for the total disk, northern and southern hemispheres of the Sun for a time interval from 1951 August to 1998 December. Apart from the 11-year Schwabe cycle which is the fundamental period and is found in all of the three time series, the following prominent results are found: (1) the rotational periodicity of solar activity at high latitudes is approximately from 28 to 32 days; (2) a large number of quasi-periods appearing in low-latitude solar activity (annual variation, 1.3–1.7 years, quasi-biennial oscillation, and 4–5 years) also exist in polar faculae; (3) the periodicities on both hemispheres are not identical.     

Synoptic magnetic field in cycle 23 and in the beginning of the cycle 24

The SOHO/MDI data provide the uniform time series of the synoptic magnetic maps which cover the period of the cycle 23 and the beginning of the cycle 24. It is very interesting period because of the long and deep solar minimum between the cycles 23 and 24. Synoptic structure of the solar magnetic field shows variability during solar cycles. It is known that the magnetic activity contributes to the solar irradiance. The axisymmetrical distribution of the magnetic flux (Fig. 3c) is closely associated with the ‘butterfly’ diagram in the EUV emission (Benevolenskaya et al., 2001). And, also, the magnetic field (B_∥) shows the non-uniform distributions of the solar activity with longitude, so-called ‘active zones’, and ‘coronal holes’ in the mid-latitude. Polar coronal holes are forming after the solar maxima and they persist during the solar minima. SOHO/EIT data in the emission of Fe XII (195 Å) could be a proxy for the coronal holes tracking. The active longitudinal zones or active longitude exist due to the reappearance of the activity and it is clearly seen in the synoptic structure of the solar cycle. On the descending branch of the solar cycle 23 active zones are less pronounced comparing with previous cycles 20, 21 and 22. Moreover, the weak polar magnetic field precedes the long and deep solar minimum. In this paper we have discussed the development of solar cycles 23 and 24 in details.