一类垂足多边形的有向面积公式及其应用

给出圆内接多边形的垂足多边形的有向面积公式，并利用该公式获得圆内接多边形的垂足多边形和正多边形的垂足多边形的若干结果，从而推广了垂足三角形的一些结论。     

可靠的电视监控系统控制电路

本文论述了工业电视监控系统主控制电路的应用与工作过程。     

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.     

The relationship between inductive electric field and flares

We observationally deduce the inductive electric field in the photosphere for the first time from the horizontal velocities computed by local correlation tracking (LCT) technique and the vector magnetic fields derived from vector magnetograms. We study the relationship between E and powerful flares (X-class) of four active regions (ARs): NOAA 10720, 10486, 9077 and 8100. It is found that the kernels of flares are roughly located near the inversion lines where maxima of E are observed. Our results show that E relates to the accumulation of non-potentiality in the photosphere and the transportation of non-potentiality from the photosphere to the corona.     

Magnetic coupling of the Sun–Earth system – The view from STEREO

The STEREO mission, launched on October 25 2006, will provide the first stereoscopic view of the Sun and its magnetic environment. A suite of identical instruments on two continuously separating spacecraft will monitor the onset of solar eruptive phenomena, and track them as the shocks and ejected material propagate through the interplanetary medium (IPM). The combination of remote sensing and in situ instrumentation will provide new insights into the onset of eruptions, the extent of their effects on the global structure of the low corona, and their subsequent evolution through the IPM. These observations will provide new constraints on the processes involved and allow us to distinguish between competing models of eruptive solar phenomena.     

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.     

Long-term photometric signature study of two GEO satellites

Geostationary earth orbit satellites have been extensively used for unique high-orbit stationary characteristics. Long-term precise investigation is an important issue in the observation of GEO satellites, since it can provide valuable information on the satellites’ operation state, discrimination and early warning analysis. Ground-based optical-electronic devices play a significant role in the observation. 4-month photometric signature variation of two satellites is presented based on the successive observations using the 1.56-meter telescope of Shanghai Astronomical Observatory (SHAO). It can be concluded that the long-term brightness change mainly results from the sun declination angle and regular orbit maneuver. Moreover, the solar panel offsets of the two satellites are analyzed and found to be approximately 4 degrees. Estimation of photometric accuracy reaches 0.15 mag for the application of CCD drift-scan optical-electronic technique.     

Helioseismology and the solar cycle

Helioseismic measurements stretching back for about three decades have clearly shown that the acoustic modes are sensitive to solar-cycle changes. 2006 marks the first full 11-year cycle of continuous observations from the Global Oscillation Network Group (GONG), and 10 years of observations with the Michelson Doppler Imager (MDI) aboard the SOHO spacecraft. For the first time, global helioseismology has traced the migrating zonal flow pattern of the torsional oscillation deep within the convection zone, while local helioseismology has revealed the changing pattern of meridional flows over the cycle. The frequencies, lifetimes, and amplitudes of acoustic modes all show variations that closely track the surface distribution of magnetic activity and may provide insight into the excitation and damping of the oscillations. Efforts to trace magnetic field and sound speed or density changes in the solar interior have proved more challenging.     

偏场使用的同轴三反系统畸变稳定性仿真分析

针对测绘图像几何精度对光学镜头畸变稳定的要求,仿真分析了一偏场使用的同轴三反光学系统镜头的畸变稳定性,从而论证该光学镜头用于测绘相机的可能性。将光学系统畸变误差源分解为加工误差、装调误差、工作温度变化引入的误差、以及调焦引入的误差4个主要部分,利用光学设计软件仿真分析了各误差源单独做用时对光学镜头畸变的影响情况,仿真结果表明在引入误差源的情况下,所分析的光学镜头的相对畸变不变,绝对畸变的最大变化范围小于2个像元尺寸,光学镜头的畸变稳定,有用于测绘相机的可能性。     

半导体激光器与单模光纤的球透镜耦合分析

建立了半导体激光器与单模光纤通过球透镜耦合的光传输模型,对双异质结激光器光束特性进行了分析。基于Huygens-Fresnel原理计算了激光光束远场发散角以及光束束腰半径。运用高斯光束与单模光纤耦合理论以及ABCD矩阵理论进行了激光器与单模光纤的球透镜耦合效率分析,给出了最优化的耦合封装工艺参数,以及各个影响耦合效率的参数容忍度,对半导体激光器与单模光纤的球透镜耦合封装具有重要意义。