What Determines the Composition of SEPs in Gradual Events?

Gradual solar energetic particle (SEP) events are evidently accelerated by coronal/interplanetary shocks driven by coronal mass ejections. This talk addresses the different factors which determine the composition of the accelerated ions. The first factor is the set of available seed populations including the solar wind core and suprathermal tail, remnant impulsive events from preceding solar flares, and remnant gradual events. The second factor is the fractionation of the seed ions by the injection process, that is, what fraction of the ions are extracted by the shock to participate in diffusive shock acceleration. Injection is a controversial topic since it depends on the detailed electromagnetic structure of the shock transition and the transport of ions in these structured fields, both of which are not well understood or determined theoretically. The third factor is fractionation during the acceleration process, due to the dependence of ion transport in the turbulent electromagnetic fields adjacent to the shock on the mass/charge ratio. Of crucial importance in the last two factors is the magnetic obliquity of the shock. The form of the proton-excited hydromagnetic wave spectrum is also important. Finally, more subtle effects on ion composition arise from the superposition of ion contributions over the time history of the shock along the observer’s magnetic flux tube, and the sequence of flux tubes sampled by the observer.     

Relationship between daily variation of cosmogenic nuclide Be-7 concentration in atmosphere and solar activities

Daily Be-7 concentrations in air at the height of 15 m are continuously observed at 38°15.2′N, 140°20.9′E, between 2000 and 2001. The average concentration and the relative standard deviation were 4.0 mBq/m³ and 50% in 2000–2001, respectively. The Be-7 concentrations increased 2.5% with the decrease in the sunspot numbers by 6.7% for the term of two years. From the power spectral analysis, the periodicity of 26 days is shown for the daily Be-7 concentrations. The folding analysis indicates that the time variation of the Be-7 concentration is similar to that of the ground-based neutron counting rate, and the phase delay for the minimum portion of Be-7 concentration was roughly 8 days to the maximum sunspot number. These results indicate that the Be-7 concentrations in the air at ground level have 26 day periodicity as a component of time variations and the time variation is caused by the solar modulation of galactic cosmic rays, which corresponds to the variation of the sunspot number due to the rotation of the sun.     

复合材料元件吸能能力的数值模拟

运用MSC／DYTRAN有限元软件，对碳纤维一环氧树脂“┼”字型、“┬”字型、“┐”字型3种典型复合材料元件的破坏过程、峰值栽荷、平均栽荷和能量吸收能力进行了数值模拟研究。鉴于MSC／DYTRAN有限元软件不能直接用于复合材料的吸能分析，分析时采用了等效的方法。将复合材料结构元件的数值计算结果与准静态轴向压溃试验的结果进行对比，两者较为一致，从而说明运用该有限元软件并采用等效的方法模拟复合材料结构吸能能力的可行性。     

非线性条件下编队卫星周期性相对运动条件

利用编队卫星机械能守恒原理，提出了非线性条件下求解编队卫星周期性相对运动条件的新方法，给出了非线性周期相对运动的初始条件。编队卫星相对距离较近时，利用非线性周期运动条件，可修正Hill方程的初始条件，抑制编队卫星的长期漂移。编队卫星相对距离较大，非线性因素不可忽略时，利用非线性周期运动条件，可找到不需消耗任何燃料的周期性相对运动轨道。最后的数值仿真结果验证了该方法的正确性。     

地球同步卫星远地点变轨期间的三轴姿态稳定

本文提供了地球同步三轴稳定卫星在远地点变轨机动过程中的卫星动力学模型,其中考虑了刚体、液体晃动和帆板振动的耦合,这些模型经过实际工程验证,证明是正确的。本文还给出了控制器结构,它由PID和各种晃动滤波器及帆板挠性滤波器组成。工程设计证明,这种控制器结构可满足设计要求且简单可靠。本文还给出了系统稳定性分析结果及数字仿真结果。     

含氧杂环丁烷粘合剂的先进固体推进剂

综述了国内外氧杂环丁烷粘合剂研究的新进展。介绍了ＢＡＭＯ／ＡＭＭＯ固体推进剂的配方和性能。通过与常规推进剂的比较，分析并指出ＢＡＭＯ／ＡＭＭＯ推进剂的潜在优点。     

1989年3月大宇宙线暴事件的特征

本文分析了1989年3月一系列大耀斑等离子体抛射引起的宇宙线强度变化的特征.除对中子成分分析外,还对μ介子成分及其各向异性特征作了分析,讨论了宇宙线强度变化与太阳耀斑特性和地磁扰动之间的关系。分析发现,宇宙线的Forbush下降不仅与太阳耀斑的级别、持续时间,以及在日面上的位置有关,而且还与光学耀斑是否伴有强的X射线暴、是否有强的射电爆发,以及是否引起强的地磁暴紧密有关.各向异性分析表明,3月大事件的各向异性明显小于宁静时的各向异性,这可能是因为受到太阳活动强烈调制之后,宇宙线各向异性趋于减小的原因.     

Prompt effects of solar wind variations on the inner magnetosphere and midlatitude ionosphere

It is well known that the solar wind can significantly affect high-latitude ionospheric dynamics. However, the effects of the solar wind on the middle- and low-latitude ionosphere are much less studied. In this paper, we report observations that large perturbations in the middle- and low-latitude ionosphere are well correlated with solar wind variations. In one event, a significant (20–30%) decrease of the midlatitude ionospheric electron density over a large latitudinal range was related to a sudden drop in the solar wind pressure and a northward turning of the interplanetary magnetic field, and the density decrease became larger at lower latitudes. In another event, periodic perturbations in the dayside equatorial ionospheric E × B drift and electrojet were closely associated with variations in the interplanetary electric field. Since the solar wind is always changing with time, it can be a very important and common source of ionospheric perturbations at middle- and low-latitudes. The relationship between solar wind variations and significant ionospheric perturbations has important applications in space weather.     

太阳宁静及耀斑期间1AU附近等离子体轫致辐射研究

在太空等离子体中，尤其在等离子体内部磁场较弱时，轫致辐射是等离子体能量损失的主要机制．本文对太阳宁静及耀斑期间1AU处等离子体轫致辐射计算表明，等离子体辐射强度If的变化与辐射的电磁波频率有直接的关系．当辐射频率，接近于等离子体频率，fpe时，辐射强度显著增大．随着电磁波辐射频率的增大，辐射强度随频率增大作缓慢对数下降．辐射亮温Tb与等离子体电子温度Te、介质光深成正比．Tb与If随辐射频率变化的整体趋势一致．在相同的辐射频率情况下，太阳宁静期间If值、Tb值低于太阳耀斑期间If值、Tb值．     

Progress on Space Solar Telescope in 2004 - 2006

The progress on Chinese Space Solar Telescope (SST) in 2004-2006 is introduced. The scientific objectives are further clarified and the ground operation system has been planned. The 7 key technical problems of SST satellite platform and payloads have been tackled, which lay solid scientific and technological foundations for engineering prototype phase of the SST project. At present the SST project undergoes evaluation by CNSA and CAS so as to enter the engineering prototype phase of the SST project if it is finally approved.