高层大气臭氧对于太阳紫外辐射27天波动的响应

本文利用Ｓｏｌａｒ Ｍｅｓｏｓｐｈｅｒｅ Ｅｘｐｌｏｒｅｒ（ＳＭＥ）卫星１９８２年和１９８３年太阳紫外辐射和赤道地区５０－９０ｋｍ臭氧分布的红外观测资料，对臭氧地太阳紫外辐射２７天振荡的响应进行了研究，并且利用大气光化波动模式对其进行了理论计算，计算结果与实测结果基本一致。     

Heavy ion observations by MARIE in cruise phase and Mars orbit

The charged particle spectrum for nuclei from protons to neon, (charge Z=10) was observed during the cruise phase and orbit around Mars by the MARIE charged particle spectrometer on the Odyssey spacecraft. The cruise data were taken between April 23, 2001 and mid-August 2001. The Mars orbit data were taken March 5, 2002 through May 2002 and are scheduled to continue until August 2004. Charge peaks are clearly separated for charges up to Z=10. Especially prominent are the carbon and oxygen peaks, with boron and nitrogen also clearly visible. Although heavy ions are much less abundant than protons in the cosmic ray environment, it is important to determine their abundances because their ionization energy losses (proportional to Z²) are far more dangerous to humans and to instruments. Thus the higher charged nuclei make a significant contribution to dose and dose equivalent received in space. Results of the charged particle spectrum measurements will be reported.     

Artificial equilibrium points and bi-impulsive maneuvers to observe 243 Ida

In the restricted three-body problem, the traditional Lagrange points L₁ and L₂ are the only equilibrium points near the asteroid 243 Ida. The thrust generated by a solar sail over a spacecraft enables the existence of new artificial equilibrium points, which depend on the position of the spacecraft with respect to the asteroid and the attitude of the solar sail. Such equilibrium points generate new spots to observe the body from above or below the plane of motion. Such points are very good observational locations due to their stationary condition. This work provides a preliminary analysis to observe Ida through the use of artificial equilibrium points as spots combined with transfer maneuvers between them. Such combination can be used to observe the asteroid from more different points of view in comparison to fixed ones. The analyses are made for a spacecraft equipped with a solar sail and capable of performing bi-impulsive maneuvers. The solar radiation pressure is used both to maintain the equilibrium condition and to reduce the costs of the transfers and/or to create transfers with longer duration. This is a new aspect of the present research, because it combines the continuous thrust with initial and final small impulses, which are feasible for most of the spacecraft, because the magnitudes of the impulses are very low. These combined maneuvers may reduce the transfer times of the maneuvers in most of the cases, compared with the maneuvers based only on continuous thrust. Several options involved in these transfers are shown, like to minimize the fuel spent ($\mathrm{\Delta }\mathit{v}$) as a function of the transfer time or to extend the duration of the travel between the points. Extended transfer times can be useful when observations are required during the transfers.     

固体火箭羽流中Al2O3粒子的辐射特性

基于Lorentz-M ie电磁理论,建立了计算A l2O3粒子辐射特性,包括散射截面、吸收截面、散射系数、吸收系数、散射相函数的计算方法,并在假设粒子散射为单次、独立散射的基础上,推导了粒子系辐射特性的计算方法。采用此方法计算了含铝推进剂固体发动机尾喷流在2~5μm光谱范围内A l2O3粒子的辐射特性。结果表明,用Lorentz-M ie电磁理论计算A l2O3粒子的辐射特性是有效的、可靠的。     

激光辐照30CrMnSiNi2A钢的微观组织与疲劳性能

对30CrMnSiNi2A钢带孔板和带槽板试样进行了不同工艺参数的激光辐照,并对辐照前后试样的疲劳性能、硬化层显微组织和硬度分布作了试验与分析。试验表明,不适当的激光工艺会导致疲劳寿命明显下降,显微组织和硬度分布不良。只有在适当的激光工艺参数辐照时,才能提高30CrMnSiNi2A低合金超高强度钢的疲劳寿命。     

质子单粒子效应引发卫星典型轨道下SRAM在轨错误率分析

利用中国原子能科学研究院100 Me V质子回旋加速器(CY CIAE-100)的单粒子效应辐照装置,测量了典型静态随机存储器(SRAM)的质子单粒子翻转截面;利用Space Radiation 7.0软件计算了卫星搭载该器件在典型轨道条件下运行的在轨错误率;同时研究了航天器在不同轨道高度、轨道倾角和屏蔽条件下对质子单粒子效应引发的在轨错误率的影响。计算结果表明:航天器运行于地球同步轨道高度及以下时,质子单粒子效应引发的在轨错误率均高于重离子的,最高可相差3个数量级左右。     

超声速混合层中边频扰动的气动声场

为研究超声速流动下混合层声辐射机理,提高对超声速混合层气动噪声的认识,利用抛物化稳定性方程(PSE)考察一对频率接近失稳扰动的非线性演化,分析近场差频扰动的演化特征,并结合Wu积分理论计算远场声辐射特性。结果表明,超声速混合层中频谱拓宽与差频扰动有关,差频扰动的产生,拓宽了远场马赫波辐射范围,增大了远场马赫波辐射强度。对于快模态扰动,差频扰动频率越小,其增长能力越强,远场马赫波辐射区域越宽;对于慢模态扰动,差频扰动频率大小对其增长能力影响不明显,远场马赫波辐射范围和强度变化不大。      

火箭发动机出口参数对喷焰流动及辐射的影响

基于详细化学反应机理+逐线积分法+视在光线法开展了火箭发动机喷焰流动与辐射特性研究,分析了不同化学反应机理对流动与辐射的影响,利用地面试验数据校验了模型的正确性,并详细分析了火箭发动机出口参数变化对喷焰流动及辐射的影响规律。研究结果表明:喷管出口温度增加,对流场结构影响较小,但会显著提升喷焰的复燃效应;喷管出口压强增加,会对流场马赫波系结构产生影响,但对喷焰二次燃烧影响较小;喷焰红外辐射强度会随着出口温度或出口压强的升高而增加,且红外辐射强度与出口推力正相关。      

巡航导弹红外辐射及大气衰减计算模型

对巡航导弹3个主要辐射源:蒙皮、尾喷管及羽流进行了深入分析,建立了巡航导弹红外辐射计算模型.此外,在红外辐射的大气传输理论基础上,综合考虑高度、倾斜及气象条件等各种因素,分析了大气衰减对红外辐射的影响,建立了大气透过率的理论模型与计算方法.最后,以某型号巡航导弹为例,利用此模型计算了3~5μm和8~12μm两个波段的红外辐射强度、大气光谱透过率和平均透过率,以及经过大气衰减后的红外辐射强度,并对计算结果进行了分析.结果表明,这是一种计算巡航导弹红外辐射的简单方法.      

电大尺寸天线罩电磁特性高效数值仿真技术

针对电大尺寸天线罩电磁特性,分析研究了快速求解表面积分方程的多层快速多极子算法及其改进技术。构造了具有良好矩阵性态的积分方程形式,提出加速迭代求解的并行预条件技术,利用分组稀疏化方式构造预条件矩阵,显著降低了迭代求解次数。采用快速球谐展开技术对聚合和配置因子项进行压缩,将其存储量降低了2/3。通过数值算例验证了方法的精确性和高效性,并实现了大型带罩阵列天线辐射特性的仿真分析。