27-day variation in solar-terrestrial parameters: Global characteristics and an origin based approach of the signals

The Earth and the near interplanetary medium are affected by the Sun in different ways. Those processes generated in the Sun that induce perturbations into the Magnetosphere-Ionosphere system are called geoeffective processes and show a wide range of temporal variations, like the 11-year solar cycle (long term variations), the variation of ～27?days (recurrent variations), solar storms enduring for some days, particle acceleration events lasting for some hours, etc.In this article, the periodicity of ～27?days associated with the solar synodic rotation period is investigated. The work is mainly focused on studying the resulting 27-day periodic signal in the magnetic activity, by the analysis of the horizontal component of the magnetic field registered on a set of 103 magnetic observatories distributed around the world. For this a new method to isolate the periodicity of interest has been developed consisting of two main steps: the first one consists of removing the linear trend corresponding to every calendar year from the data series, and the second one of removing from the resulting series a smoothed version of it obtained by applying a 30-day moving average. The result at the end of this process is a data series in which all the signal with periods larger than 30?days are canceled.The most important characteristics observed in the resulting signals are two main amplitude modulations: the first and most prominent related to the 11-year solar cycle and the second one with a semiannual pattern. In addition, the amplitude of the signal shows a dependence on the geomagnetic latitude of the observatory with a significant discontinuity at approx. ±60°.The processing scheme was also applied to other parameters that are widely used to characterize the energy transfer from the Sun to the Earth: F10.7 and Mg II indices and the ionospheric vertical total electron content (vTEC) were considered for radiative interactions; and the solar wind velocity for the non-radiative interactions between the solar wind and the magnetosphere. The 27-day signal obtained in the magnetic activity was compared with the signals found in the other parameters resulting in a series of cross-correlations curves with maximum correlation between 3 and 5?days of delays for the radiative and between 0 and 1?days of delay for the non-radiative parameters. This result supports the idea that the physical process responsible for the 27-day signal in the magnetic activity is related to the solar wind and not to the solar electromagnetic radiation.     

考虑辐射的化学平衡流驻点线解

本文用数值方法求解了化学平衡的高超声速粘性激波层驻点线流场。考虑了辐射和质量引射对流场的影响。辐射模型采用线和连续谱模型。文中讨论了引射率、头部半径、来流速度对壁面传热的影响。与有关文献结果比较表明,本文的方法是可行的。     

Stellar infrared astronomy with EDISON

In this review the IR emission from circumstellar material is discussed, both of ionized gas and dust grains, and the astrophysical information that can be extracted from such observations. Some emphasis is placed on the possibilities of stellar IR astronomy using a large space-borne telescope, especially with respect to the much better spatial and spectral resolution of such a telescope compared to the current generation of ground-based and space IR telescopes.     

强辐射条件下应变测量的抗干扰技术研究

文章从动力学结构分析应变测量的基本原理入手,着重介绍了国防高科技试验中,在强辐射、强电磁脉冲干扰环境条件下,为保证应变测量的实现,经模拟试验研究,在应变测量时采用了一系列抗干扰技术措施,包括特殊环境条件下所用元器件材料的选择,传感应变计安装方式,组桥接线方式,密封屏蔽等技术。并介绍了这些技术措施在某试验现场应变测试试验中的应用概况.     

弹道靶红外辐射测量

为深入认识再入物理现象 ,在弹道靶上做了模型头部和近尾流红外辐射测量。发射器为 1 4.5mm口径的二级轻气炮 ,模型为1 0mm的球 ,材料为聚碳酸酯和铝 ,模型发射速度 4～6km/s,使用红外InSb探测器测量波长 3～ 5 .4μm的红外辐射 ,靶室压力 5 .32kPa。实验中使用光电法测量模型速度 ,两站阴影照相进行模型姿态监测和速度核实。实验结果表明 :球模型的红外辐射强度强烈依赖于模型材料和模型飞行速度。对不同材料模型头部和尾流部辐射强度的定性比较说明由于低温材料烧蚀产物的存在 ,极大地增强了头部和近尾流区的辐射强度 ,而且延长了尾流辐射长度     

反辐射导弹设计技术

反辐射导弹（ＡＲＭ）是一种利用雷达辐射源的电磁波，发现、跟踪并摧毁雷达系统的导弹。反辐射导弹的出现，使仅有“软”杀伤能力的电子战有了“硬”摧毁能力。论述了反辐射导弹的特点及其局限性，讨论了提高反辐射导弹性能的技术方法。这些技术包括：缩窄工作频带、采用比相比幅单脉冲侧向体制、数字化和集成化设计等。     

卫星抗辐射加固技术

分析了FY－1C卫星运行轨道空间辐射环境，介绍了整星、单机、器件抗辐射要求。卫星研制过程中，对各单抗和系统在技术设计、元器件设计、软件编制等的抗辐射加固设计要求。特别对有CPU和存储器的单粒子翻转效应（SEU）和闩锁效应（SEL）试验。仪器和系统的软件均用故障注入的方法完成了抗SEU的仿真试验。     

用FVM法计算固体火箭羽流的红外特性

建立了有限体积法(FVM)的理论模型模拟固体火箭羽流的红外特性,研究了燃气组分H2O,CO2,CO,HCL,OH,NO的吸收和发射,以及AL2O3粒子云的吸收、发射和散射,还研究了两相流场中气相和粒子云温度不均匀时对辐射传输方程的修正。计算一单喷管固体火箭的二维轴对称羽流在光谱2~5μm的红外特性,给出羽流辐射的空间分布和光谱分布并与文献计算的结果对比。研究表明:有限体积法能较好地模拟固体火箭羽流的红外特性;粒子辐射占固体火箭羽流红外辐射的主要部分;在光谱2~4μm粒子辐射使羽流辐射增强,而在光谱4~5μm粒子辐射使羽流辐射减弱。     

SPACE LIFE SCIENCE IN 2000-2001

Chinese scientists studied some of the problems in the field of space life science and achieved success in the area during 2000-2001. Space biological experi ments were carried out in the orbit and the results of ground studies on protein crystallization, space radiation, space motion sickness were introduced in this paper. The influences of simulated weightlessness on the brain-function, the car diovascular, endocrine hormones, immunity, skeletal and muscle systems were presented. In addition, gravity medicine and space environment medicine, as well as countermeasures to space deconditioning, such as the traditional Chinese medicine, were also reported.     

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．