Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations

The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P_sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P_sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P_sw. It proved that the enhancement of P_sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P_sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P_sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause.     

Wave-Particle-Electric Field Synergetic Auroral Electron Acceleration

Space Science Reviews - We discuss afresh the problem of the auroral electron acceleration based on the controversy reports of Bryant, D. A. et al.: 1992, Phys. Rev. Lett. 68, 37, and Borovsky, J.:...     

电子会议系统在型号产品研制中的应用

计算机技术和通信技术的结合把计算机从传统的孤立应用推进到支持群体协同工作，从而产生了计算机支持的协同工作和多媒体电子会议系统等新型应用。本文结合本单位的实际，进行了基于Sametime电子会议协同研制工作的研究，详细论述了型号研制对电子会议系统的要求及其实现。     

丁羟推进剂拉伸断裂行为的扫描电镜研究

利用扫描电镜及附属微型动态拉伸装置实验手段，对丁羟基复合固体推进剂进行了断口微观形貌观察和电镜微型拉伸试件在应变状上的断裂行为分析。结果表明，从推进剂拉伸力学行为的微观结构变化以预示其宏 同力学性能，改善丁羟推进剂粘合剂与固体颗粒之间的界面性质，是固体推进剂力学性能的一个重要方向。     

高超声速小钝锥尾流转捩规律与光电特性

显式有限差分方法用于求解小钝锥高超声速化学非平衡尾流的轴对称边界层方程。该方法既适用于层流也适用于湍流。应用 Goldburg 转捩准则确定转捩初始位置。详细地计算了小钝锥尺寸、飞行速度、高度对尾流转捩和光电特性的影响。从计算中得到转捩和光电特性变化的一些有用规律。对湍流亚密部分的雷达散射截面进行了规律性分析。计算结果具有实用参考价值。     

极光区电离层Hall电导率的观测及其在E层电子加热情况下的特征

本文利用欧洲的ＥＩＳＣＡＴ雷达观测资料及与这配合的地磁观测数据，用电离层参数直接计算和地面磁场反演两种方法导出了极区电离层Ｈａｌｌ电导率，特别显示出在强对流电场激发的Ｅ层等离子体不稳定波对电子加热情况下，电导率明显增高。     

A survey of radio jets with Chandra and HST

Relativistic jets are a common property of radio-loud Active Galactic Nuclei (AGN). Understanding jet physical properties is an essential precursor to understanding the mechanisms of energy transport, and ultimately, how energy is extracted from the central black hole. In this paper, I highlight recent developments from Chandra and HST observations of kpc-scale jets in AGN, with particular emphasis on our survey of 17 radio jets in a sample of FRII radio galaxies. These observations show that (1) X-ray and optical emission is common from kpc-scale jets, (2) a large fraction of the bolometric luminosity is emitted at X-rays, and (3) in most sources, a candidate emission process for the X-rays is inverse Compton scattering of the Cosmic Microwave Background off the relativistic electrons in the jet. If the latter scenario holds, the implication is that jets are still relativistic on kpc scales.     

微量气味成分的自由基簇射技术脱除

研究了密闭体系中微量气味污染物的脱除作用与机理。采用电晕放电自由基簇射技术，实现了人工环境下氧化性自由基的产生；以电子自旋共振技术（ESR）对气态羟基自由基实施了捕集和检测，验证了在羟基自由基的存在下NH3被氧化为N2。通过U—I获得反应能耗和污染物去除效率为：NH3脱除效率为90．6％时，能耗1．0W。研究表明：自由基簇射技术产生的氧化性自由基可有效去除密闭生存环境中产生的NH3等微量有害气味成分，将在空间站等密闭生存系统内空气净化中有很好的应用前景。