某控制组合电磁发射超标分析及解决方案

本文针对电磁兼容测试中，传导发射和辐射发射超过标准限值要求问题，首先介绍了发射超标主要原因，继而梳理超标定位方法和常用电磁兼容加固措施。并以某控制组合为例，应用上述方法制定排查方案，完成电磁发射测试超标问题的干扰定位；并针对干扰源，使用线缆添加屏蔽层、电源端口添加滤波器等加固措施，经验证，措施有效，发射明显降低。同时，本文所述排查方法和加固措施，可为后续电子产品电磁兼容性设计和通过测试提供参考。     

Sporadic emission of ultra high energy gamma rays from crab pulsar

In a further study of sporadic emission from pulsars we find evidence for short lived intense emission from the Crab pulsar.     

Thermal and nonthermal flare emission observed with the Nobeyama Radio Heliograph

The early phases of three flares, observed by the Nobeyama Radio Heliograph, are studied. Nonthermal and thermal radio sources are identified by comparison with soft X-ray images taken by the Soft X-ray Telescope onboard the Yohkoh satellite. Two of the flares are mainly of nonthermal origin and their location coincides with one of the footpoints of soft X-ray loops. Another flare has both thermal and nonthermal components which start to brighten simultaneously. This suggests that particle acceleration and plasma compression develop simultaneously.     

基于化学反应器网络模型法的预混气组分对NOx反应路径影响研究

摘 要：为探究预混气组分对不同反应路径下NOx生成影响,针对高压射流反应器,基于CFD流场特征等,构建优化了单PSR、2PSR、3PSR以及PSR+PFR四种化学反应器网络模型。在贫预混燃烧条件下,研究了纯CH4及其混合气燃烧时不同反应路径下NOx的生成情况,得出了燃烧室内不同反应区域每条反应路径NOx的生成量。结果表明,纯CH4燃烧产生的NOx主要来自于热力型、快速型和N2O-中间体型三条反应路径。绝热火焰温度的提高主要促进了热力型和N2O-中间体型NOx的生成。随着CH4或CO中加入H2摩尔分数的增加,NOx排放总量降低,快速型NOx生成速率降低,特别是火焰刷区域的。另外,混合气中CO摩尔分数的增加会导致NOx生成量增多。     

调整复合推进剂配方改善喷焰微波衰减特性

对复合固体推进剂喷焰的微波衰减特性与其主要组分，即铝粉，黑索金和过氯酸铵的影响的关系进行了分析，得出了一些基本规律。通过调整ＲＤＸ、ＡＰ和铝粉含量的比例，可以不显著降低推进剂能量特性的基础上，在一定程度上改善复合固体推进剂喷焰的微波衰减特性。对复合固体推进剂的配方优化设计和研究具有参考意义。     

计入带电粒子入射角度对次级电子效应影响时航天飞行器的带电特性

本文采用由实验得到的带电粒子入射角度对次级电子的影响关系,根据轨道限制电流收集理论,导出了不同几何形体航天器的次级电子数通量表达式;并按局部电流平衡模型,计算了航天器背阴面的带电电位。结果表明,计入带电粒子入射角的影响后,航天器表面负电位的数值有一定减少。因此,在计算航天器表面带电时,应当考虑这种影响。     

无线输电技术与卫星太阳能电站的发展前景

文章简要叙述了无线输电和卫星太阳能电站的概念,特别强调了无线输电技术和建造卫星太阳能电站的科学技术意义和深远的战略意义;扼要介绍分析了国外在该领域的研究进展;概括叙述了建造卫星太阳能电站的技术经济性及科技界共同关心的几个问题;充分肯定了它的科学技术研究价值、应用前景和未来所带来的巨大的社会经济效益。     

辐射计反射面天线面形精度对其主波束效率影响研究

以FY-3卫星微波成像仪天线为模型,对反射面天线面形精度对天线主波束效率的影响进行了分析。提出基于数值拟合法的公式,用GRASP软件半物理仿真结果,修正Ruze公式关于面形精度影响因子的表达式,实现了工程中天线主波束效率快速估算。该方法减小了Ruze公式中由于假设口径场等幅同相分布引起的计算误差,采用该方法后计算精度可控制在1%以内。最后针对多馈源共用反射面的辐射计天线提出了分区域分析面形精度的方法。     

3D Imaging of the OH mesospheric emissive layer

A new and original stereo imaging method is introduced to measure the altitude of the OH nightglow layer and provide a 3D perspective map of the altitude of the layer centroid. Near-IR photographs of the OH layer are taken at two sites separated by a 645 km distance. Each photograph is processed in order to provide a satellite view of the layer. When superposed, the two views present a common diamond-shaped area. Pairs of matched points that correspond to a physical emissive point in the common area are identified in calculating a normalized cross-correlation coefficient (NCC). This method is suitable for obtaining 3D representations in the case of low-contrast objects. An observational campaign was conducted in July 2006 in Peru. The images were taken simultaneously at Cerro Cosmos (12°09′08.2″ S, 75°33′49.3″ W, altitude 4630 m) close to Huancayo and Cerro Verde Tellolo (16°33′17.6″ S, 71°39′59.4″ W, altitude 2272 m) close to Arequipa. 3D maps of the layer surface were retrieved and compared with pseudo-relief intensity maps of the same region. The mean altitude of the emission barycenter is located at 86.3 km on July 26. Comparable relief wavy features appear in the 3D and intensity maps. It is shown that the vertical amplitude of the wave system varies as exp (Δz/2H) within the altitude range Δz = 83.5–88.0 km, H being the scale height. The oscillatory kinetic energy at the altitude of the OH layer is comprised between 3 × 10⁻⁴ and 5.4 × 10⁻⁴ J/m³, which is 2–3 times smaller than the values derived from partial radio wave at 52°N latitude.