Plasma sheet stretching accompanied by field aligned energetic ion fluxes observed by the NUADU instrument aboard TC-2

The NUADU (NeUtral Atom Detector Unit) instrument aboard TC-2 recorded 4л solid angle images of charged particles (E >180 keV) spiraling around the magnetic field lines in the near-Earth plasma sheet (at ~ -7 RE, equatorial dawn-to-night side) during a geomagnetic storm (Dst =-219 nT) on August 24, 2005. Energetic ion beam events characterized by symmetrical, ring-like, solid angle distributions around ambient magnetic field lines were observed during a 34-minute traversal of the plasma sheet by the TC-2 spacecraft. Also, observations during these multiple crossings of the plasma sheet were monitored by the magnetometer experiment (FGM) aboard the same spacecraft. During each crossing, a whistler-mode chorus enhancement was observed in the anisotropic area by the TC-2 low frequency electromagnetic wave detector (LFEW/TC-2) at a frequency just above that of the local lower hybrid wave. A comparison of the ion pitch angle distribution (PAD) map with the ambient magnetic field shows that an enhancement in the field aligned energetic ion flux was accompanied by tailward stretching of the magnetic field lines in the plasma sheet. In contrast, the perpendicular ion-flux enhancement was accompanied by a signature indicating the corresponding shrinkage of the magnetic field lines in the plasma sheet. Since both parallel ion-flux and perpendicular ion-flux enhancements occurred intermittently, the data were interpreted to imply a dynamical, oscillatory process of the magnetic field line (stretching and shrinking) in the near-Earth plasma sheet, which might have acted to help establish an interaction region in this area which would support continuous aurora-substorm triggering during the ongoing magnetic storm. The whistler-mode chorus may have been produced due to ion gyro-resonance during particle pitch angle diffusion after the plasma sheet compression.     

进攻与防守——单片机的攻击与反攻击技术探析

当今世界以单片机为核心的智能产品在各行各业都得到了广泛的应用,为我们的生产、生活提供了极大的便利。然而由于我国的国情所限,电子产品设计师的权益却常常得不到保障。文章将系统地阐述单片机的攻击原理及方法以及反攻击的方法及手工段,为电子产品设计师维护自己的权益提供了有益的帮助。     

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11月26日，国家航天局发布了中国首次月球探测工程第一幅月面图。这标志着“嫦娥一号”卫星在进入环月工作轨道后开始实施的各项在轨测试任务基本完成。标志着中国首次月球探测工程取得圆满成功。     

阿秒光源在材料领域的应用

21世纪以来,阿秒(attosecond,1 as=10-18 s)技术从诞生逐渐走向快速发展,为我们带来了前所未有的时间分辨(time-resolved)探测能力.以往飞秒(1 fs=10-15 s)泵浦-探测(pump-probe)超快光谱技术被广泛应用于材料的超快动力学研究,其脉宽和光子能量可以很好地研究由外层电...     

基于空洞-稠密网络的交通拥堵预测模型

在利用卷积神经网络模型对短时交通拥堵情况等预测场景进行预测时,由于模型的卷积池化操作过程会丢失部分数据,使得目标位置的信息出现丢失及特征的分辨率持续下降,导致模型的预测能力降低.针对此,本文提出一种空洞-稠密神经网络模型.首先,利用空洞卷积用较少的网络参数获取更大感受野的特点,充分提取出复杂多变的数据时空特征.其次,通...     

南海北部地壳结构的深地震探测和研究新进展

南海是西太平洋最大的边缘海之一,其北部具有被动大陆边缘特征.深部地壳结构的研究对深入认识南海北部边缘的构造属性、演化历史、含油气盆地的形成过程,以及南海成因具有十分重要的意义.南海北部地壳结构的深地震探测经历了声纳浮标、双船扩展剖面和海底地震仪几个阶段,声纳浮标探测了解到上地壳的结构特征,双船扩展剖面首次获得了地壳结构和莫霍面起伏的情况,海底地震仪探测则得到了详细的地壳结构模型.文中回顾了这些深地震探测和研究的历史,介绍和总结了最新的研究进展和重要成果,并提出存在的问题和今后工作的建议.     

低噪声微光探测器设计与分析

探测微弱光信号时,为防止目标信号被噪声淹没,探测器的低噪声设计成为关键.选用合适的器件,采用低噪声设计技术,兼顾探测器的可靠性、稳定性考虑,提出了适用于微光探测系统的探测器设计方案.通过建模分析,估算出其电路本底噪声仅为333.09μVrms.结果表明低噪声探测器设计合理、可行,对于类似的微光探测系统中探测器低噪声设计及分析具有一定的借鉴意义.该方案已成功应用于某瞬态微光探测系统中.     

配电线路接点发热的探测与处理

由于配电线路辐射面广，分支线多，线路上的接点多而且分散，因此，线路接点发热造成的故障停电，已经成为影响供电可靠率指标和电网安全运行的一个主要因素。本文针对配电线路接点发热的问题，分析了接点发热的原因及相应的处理措施。     

Low-complexity and fast convergent multiuser detections for impulse UWB systems

To solve the problem that the conventional detections in DS-CDMA suffer from high complexity and poor robustness for the time-hopping pulse signals, the received pulse signals were remodeled, and a multipath-free detection scheme, which provides a simple approach to select samples of received signals, was introduced. By this scheme, the subsequent multiuser detection (MUD) would get rid of the mismatch due to the correlative multipath signal in IR-UWB. In addition, a computationally efficient recursive least squares (RLS) type algorithm based on least mean fourth (LMF) criterion is derived to suppress multi-access interference. The proposed multiuser detection algorithm performs well at low complexity, even in dense multipath environment.     

用紫外线看宇宙——紫外线观测卫星GALEX获得的最新照片

用紫外线波段观测刚形成不久的年轻星系，它们看起来是明亮的天体。美国宇航局发射的星系演化探测卫星，就是专门用来对年轻星系进行紫外线观测，探索星系演化的一座太空天文台。星系演化探测卫星对宇宙进行的观测，获得了十分宝贵的资料，甚至有助于揭示我们所居住的银河系当初是如何形成的。