基于GPU的S63标准电子海图数据解密算法     

钟云海  郑海  周红进 《测绘软科学研究》2014,(2):54-58

S63标准采用Blowfish算法对原始海图数据加密后发行,数据的解密成为电子海图系统数据转换和更新中一个耗时的过程。为提高数据处理的速度,针对Blowfish分组密码算法的特点,提出一种利用图形处理器（GPU）的海图并行解密算法,并采用数据传输和处理的同步技术进行了优化。测试表明,采用GPU的并行解密算法是纯CPU串行处理的9.8倍。该算法不仅可大大加快海图数据转换和更新过程,对地理信息系统海量数据处理也有一定的借鉴价值。  相似文献   

Identification of Shocks in the Spectra from Black Holes     

Samir Mandal  Sandip Kumar Chakrabarti 《Astrophysics and Space Science》2005,297(1-4):269-274

  相似文献   

Two-fluid Dynamics in Clusters of Galaxies     

Yu-Qing LouNational Astronomical Observatories  Chinese Academy of Sciences  Beijing Department of Physics & Tsinghua Center for Astrophysics 《中国天文和天体物理学报》2005,5(1):6-20

We develop a theoretical formulation for the large-scale dynamics of galaxy clusters involving two spherical ‘isothermal fluids‘ coupled by their mutual gravity and derive asymptotic similarity solutions analytically. One of the fluids roughly approximates the massive dark matter halo, while the other describes the hot gas, the relatively small mass contribution from the galaxies being subsumed in the gas. By properly choosing the self-similar variables, it is possible to consistently transform the set of time-dependent two-fluid equations of spherical symmetry with serf-gravity into a set of coupled nonlinear ordinary differential equations (ODEs). We focus on the analytical analysis and discuss applications of the solutions to galaxy clusters.  相似文献   

Weibel Turbulence in Laboratory Experiments and GRB/SN Shocks     

Mikhail V. Medvedev 《Astrophysics and Space Science》2007,307(1-3):245-250

It has recently been realized that the Weibel instability plays a major role in the formation and dynamics of astrophysical shocks of gamma-ray bursts and supernovae. Thanks to technological advances in the recent years, experimental studies of the Weibel instability are now possible in laser-plasma interaction devices. We, thus, have a unique opportunity to model and study astrophysical conditions in laboratory experiments – a key goal of the Laboratory Astrophysics program. Here we briefly review the theory of strong non-magnetized collisionless GRB and SN shocks, emphasizing the crucial role of the Weibel instability and discuss the properties of radiation emitted by (isotropic) electrons moving through the Weibel-generated magnetic fields, which is referred to as the jitter radiation. We demonstrate that the jitter radiation field is anisotropic with respect to the direction of the Weibel current filaments and that its spectral and polarization characteristics are determined by microphysical plasma parameters. We stress that the spectral analysis can be used for accurate diagnostics of the plasma conditions in laboratory experiments and in astrophysical GRB and SN shocks.  相似文献   

Analysis on the interplanetary causes of the great magnetic storms in solar maximum (2000-2001)     

X.H. Xue  Yuming Wang  P.Z. Ye  S. Wang  M. Xiong 《Planetary and Space Science》2005,53(4):443-457

In this paper, we analyze the interplanetary causes of eight great geomagnetic storms during the solar maximum (2000-2001). The result shows that the interplanetary causes were the intense southward magnetic field and the notable characteristic among the causal mechanism is compression. Six of eight great geomagnetic storms were associated with the compression of southward magnetic field, which can be classified into (1) the compression between ICMEs (2) the compression between ICMEs and interplanetary medium. It suggests that the compressed magnetic field would be more geoeffective. At the same time, we also find that half of all great storms were related to successive halo CMEs, most of which originated from the same active region. The interactions between successive halo CMEs usually can lead to greater geoeffectiveness by enhancing their southward field B_s interval either in the sheath region of the ejecta or within magnetic clouds (MCs). The types of them included: the compression between the fast speed transient flow and the slow speed background flow, the multiple MCs, besides shock compression. Further, the linear fit of the D_st versus gives the weights of and Δt as α=2.51 and β=0.75, respectively. This may suggest that the compression mechanism, with associated intense B_s, rather than duration, is the main factor in causing a great geomagnetic storm.  相似文献   

太阳米波和分米波Ⅱ型、Ⅲ型射电暴及其精细结构观测研究进展     

高冠男  林隽  汪敏  谢瑞祥 《天文学进展》2012,30(1):35-47

太阳米波和分米波的射电观测是对太阳爆发过程中耀斑和日冕物质抛射现象研究的重要观测手段。米波和分米波的太阳射电暴以相干等离子体辐射为主导,表现出在时域和频域的多样性和复杂性。其中Ⅱ型射电暴是激波在日冕中运动引起电磁波辐射的结果。在Ⅱ型射电暴方面,首先对米波Ⅱ型射电暴的激波起源问题和米波Ⅱ型射电暴与行星际Ⅱ型射电暴的关系问题进行了讨论;其次,结合Lin-Forbes太阳爆发理论模型对Ⅱ型射电暴的开始时间和起始频率进行讨论:最后,对Ⅱ型射电暴信号中包含的两种射电精细结构,Herringbone结构(即鱼骨结构)和与激波相关的Ⅲ型射电暴也分别进行了讨论。Ⅲ型射电暴是高能电子束在日冕中运动产生电磁波辐射的结果。在Ⅲ型射电暴方面,首先介绍了利用Ⅲ型射电暴对日冕磁场位形和等离子体密度进行研究的具体方法;其次,对利用Ⅲ型射电暴测量日冕温度的最新理论进行介绍;最后,对Ⅲ型射电暴和Ⅱ型射电暴的时间关系、Ⅲ型射电暴和粒子加速以及Ⅲ型射电暴信号中包含的射电精细结构(例如斑马纹、纤维爆发及尖峰辐射)等问题进行讨论并介绍有关的最新研究进展。  相似文献   

基于交叉梯度结构约束的大地电磁主轴各向异性并行三维反演     

王堃鹏  王绪本  曹辉  蓝星  段长生  罗威  原健龙 《地球物理学报》2021,64(4):1305-1319

各向异性介质对大地电磁观测数据的影响往往不可忽略,因此需要提高大地电磁各向异性三维反演的可靠性和有效性.为了满足大地电磁各向异性三维反演的需求,本文研究了一种基于交叉梯度结构约束的大地电磁主轴各向异性并行三维反演算法.根据大地电磁平面波理论假设,正演方程采用背景场与二次场分离的计算方式,二次场利用交错网格有限差分法求解.由于各向异性反演的多解性,本文将各向异性介质简化为主轴各向异性,并在此基础上进一步采用有限内存拟牛顿LBFGS法实现三维各向异性反演.为了提高各向异性反演的分辨率,反演目标函数中引入交叉梯度项,利用先验的结构信息,对三个方向的电阻率参数进行结构约束,最终的反演进一步利用MPI(Message Passing Interface,消息传递接口)技术实现分频并行计算,测试结果显示并行接近线性加速比.  相似文献   

细胞自动机地震波模拟的并行化算法   总被引：11，自引：5，他引：6       下载免费PDF全文

王真理  李幼铭 《地球物理学报》1999,42(3):410-415

采用区域分解的办法对格子气自动机地震波传播模拟的并行化算法进行了研究,提出了两种区域分解算法,并在SGIPowerChallenge并行计算机上进行了实际地质模型中平面波反射地震响应的计算,获得了较高的并行计算效率．  相似文献   

Signatures of storm sudden commencements in geomagnetic H, Y and Z fields at Indian observatories during 1958–1992     

R. G. Rastogi 《Annales Geophysicae》1999,17(11):1426-1438

The work describes an intensive study of storm sudden commencement (SSC) impulses in horizontal (H), eastward (Y) and vertical (Z) fields at four Indian geomagnetic observatories between 1958–1992. The midday maximum of δH has been shown to exist even at the low-latitude station Alibag which is outside the equatorial electrojet belt, suggesting that SSC is associated with an eastward electric field at equatorial and low latitudes. The impulses in Y field are shown to be linearly and inversely related to δH at Annamalainagar and Alibag. The average SC disturbance vector is shown to be about 10–20°W of the geomagnetic meridian. The local time variation of the angle is more westerly during dusk hours in summer and around dawn in the winter months. This clearly suggests an effect of the orientation of shock front plane of the solar plasma with respect to the geomagnetic meridian. The δZ at δC have a positive impulse as in δH. The ratio of δZ/δH are abnormally large exceeding 1.0 in most of the cases at Trivandrum. The latitudinal variation of δZ shows a tendency towards a minimum over the equator during the nighttime hours. These effects are explained as (1) resulting from the electromagnetic induction effects due to the equatorial electrojet current in the subsurface conducting layers between India and Sri Lanka, due to channelling of ocean currents through the Palk Strait and (2) due to the concentration of induced currents over extended latitude zones towards the conducting graben between India and Sri Lanka just south of Trivandrum.  相似文献   

基于二次场的可控源电磁法三维有限元-无限元数值模拟   总被引：2，自引：2，他引：0       下载免费PDF全文

张林成  汤井田  任政勇  肖晓 《地球物理学报》2017,60(9):3655-3666

本文提出了一种新的混合有限元-无限元三维可控源电磁法(CSEM)问题快速高精度正演模拟算法.首先从电场双旋度方程出发,推导了水平电偶极子源的二次场边值问题,采用无限元代替截断边界条件和有限元离散内部计算区域的新策略,达到减小计算区域的目的,基于并行直接求解技术,实现多源CSEM问题的快速精确求解.其次,通过层状解析模型测试,一方面验证了新算法的正确性,另一方面通过与其他三种已知CSEM问题求解策略进行对比,表明了本文提出的基于二次场有限元-无限元算法具有离散区域小、求解速度快和计算精度高等优点.最后,通过3D模型计算,清晰直观地模拟了场源阴影效应,为野外数据的处理与解释提供指导.  相似文献