Amplification of primordial magnetic fields by anisotropic gravitational collapse     

Emma J. King  Peter Coles 《Monthly notices of the Royal Astronomical Society》2006,365(4):1288-1294

If a magnetic field is frozen into a plasma that undergoes spherical compression, then the magnetic field B varies with the plasma density ρ according to   B ∝ρ^2/3  . In the gravitational collapse of cosmological density perturbations, however, quasi-spherical evolution is very unlikely. In anisotropic collapses the magnetic field can be a much steeper function of gas density than in the isotropic case. We investigate the distribution of amplifications in realistic gravitational collapses from Gaussian initial fluctuations using the Zel'dovich approximation. Representing our results using a relation of the form   B ∝ρ^α  , we show that the median value of α can be much larger than the value  α= 2/3  resulting from spherical collapse, even if there is no initial correlation between magnetic field and principal collapse directions. These analytic arguments go some way towards understanding the results of numerical simulations.  相似文献   

On the possibility of investigation of the magnetic field structure in subphotospheric layers of the Sun according to observations of sunspot torsional oscillations     

O. S. Gopasyuk  S. I. Gopasyuk 《Bulletin of the Crimean Astrophysical Observatory》2008,104(1):52-58

A method of investigation of the magnetic field structure in subphotospheric layers of the Sun has been developed. The method is based on observations of the torisonal oscillations of single sunspots. Characteristics of the torsional oscillations have been obtained from observations of the longitudinal magnetic field and radial velocities of seven single sunspots in the photospheric line Fe I λ5253 Å. The parameters of the torsional oscillations and magnetic tubes in the deep layers have been determined. The radius of the cross section of a magnetic flux tube forming a sunspot is greatest near the Sun’s surface and is approximately equal to the radius of a sunspot umbra. Down to the deeper layers, it decreases quite quickly. The longitudinal electric current appearing in the magnetic tube changes direction. The typical time of the current changes is determined by the period of the torsional oscillations. The intensity of the longitudinal magnetic field in the tube increases with depth. The Alfven wave velocity averaged over the length of a magnetic tube is tens or hundreds of times less than this velocity in a sunspot umbra. It decreases with an increase in the period of oscillations. A decrease in the Alfven wave velocity leads to an increase in the twisting angle of magnetic field lines.  相似文献   

Dynamo models and the flip-flop phenomenon in late-type stars     

David Moss 《Monthly notices of the Royal Astronomical Society》2004,352(2):L17-L20

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磁场中p模/s模的转换及黑子对声波的吸收     

张衡  曹莹  孔勇进 《天文研究与技术》1997,(2)

在柱坐标下将黑子周围的环形区域（黑子除外）内的振荡分解为朝向黑子传播的（入射的）波和离开黑子传播的（出射的）波。对无黑子的环形区域内的振荡也进行了同样的分解。将黑子周围的入射波看成是被黑子磁流管磁化了的介质（介质内的磁场基本是水平的）中的波。而无黑子区的入射波看成是非磁化介质中的波。比较这两种波在固定波数下功率随频率的分布发现，在磁化介质中不同径向除ｎ的声波（ｐ模）频率系统降低，同时功率也降低，降低的功率最高达非磁化介质中波的功率的３０％。而比较在固定频率下功率随波数的分布发现，磁场中ｆ模及ｎ＝１，２，３的ｐ模的脊向高波数方向位移，功率的降低受频率调制，即声波在某些有限的频带中被吸收。这些观测表明，在磁场中ｐ模与磁声重力波（ＭＡＧ）产生了模式混合或耦合。模式混合的存在支持了模式转换作为ｐ模式被黑子吸收的机制的解释。此外，本文还分析了转换的ＭＡＧ波进入黑子磁流管（其中的磁场基本上是垂直的）后进一步被吸收，吸收的功率最高达ＭＡＧ波的２０％。在磁流管内没有进一步观测到模式的转换  相似文献   

全日面磁场观测资料的初步处理     

刘扬  宋国锋  王敬山  汪景琇 《中国天文和天体物理学报》1994,(2)

用口径为１０ｃｍ的全日面磁场望远镜，我们获得了光球的全日面视向磁场观测资料。与３５ｃｍ磁场望远镜的观测结果比对，发现日面上各活动区磁场的形态以及强度都吻合较好，说明全日面磁场望远镜得到的观测资料是可信的。  相似文献   

The characteristics of motion of thin magnetic tubes     

Cheng Jiu-heng 《Chinese Astronomy and Astrophysics》1994,18(4):374-382

Starting from the equations of motion of a thin magnetic tube, the characteristic curves and velocities and compatibility relations are derived as basis for investigating its motion and for correctly formulating the problem of stationary solution. It is shown that the characteristic velocity of transverse waves is related to the Alfvén Mach number of the flow in the tube. When the flow velocity exceeds the critical value for the Kelvin-Helmholtz instability, transverse waves cease to exist.  相似文献   

类星体光谱的Monte　Carlo模拟及高红移类星体颜色法巡天中的选择效应     

樊晓晖  陈建生 《中国天文和天体物理学报》1994,(2)

利用已知的统计结果对高红移类星体光谱进行ＭｏｎｔｅＣａｒｌｏ模拟，得到了ＵＢＶＲＩ五色测光的色指数，并利用模拟的选择判据计算了选择效应函数，当２．４＜ｚ＜３．０时，选择效应来自于与主序星的混淆；当ｚ＞３．０时，则是由于较暗的类星体与晚型矮星同时从Ｕ．Ｂ等颜色的图象上消失，导致可利用色指数的减少。  相似文献   

GPS在湖南1：20万区域重力调查中的应用     

羊春华 《湖南地质》2001,20(2):135-138

GPS是现代高科技，它采用微型接收机，可以实现快速定位并取得测量点的3维座标。这种新技术在数字化地质、提高找矿效果等方面，应用前景广阔，侧重介绍了ASHTECH GPS接收机在区域重力调查中，怎样建立基准站与流动观测站、数据的传输与预处理和测量点3维座标的换算，以及应用数据自动生成布格异常等值线图。这项新技术的使用完全可以满足1：20万区域重力调查的精度要求。  相似文献   

北京同步辐射装置准直测量控制网的设计与优化   总被引：1，自引：0，他引：1  

柯明  殷立新  董岚  黄开席  韩庆夫  盛伟繁 《测绘科学》2007,32(2):122-124

在北京同步辐射装置升级改造中,为提高元件的安装精度,同时兼顾未来新增光束线的建设需要,在实验大厅建立了准直测量控制网,作为设备定位、调校、安装和变形监测等工作的基础。本文重点介绍该控制网的设计、优化与观测结果分析,特别阐述了激光精密测量技术的应用,以及对点位密度、测量精度及可靠性的控制。  相似文献   

JX4系统处理数码相机影像方法研究     

张建霞  王留召  王宝山 《测绘科学》2007,32(3):160-161

非量测性的数码相机影像已成为摄影测量中应用研究的热点。本文提出了利用数字影像重采样实现数字摄影测量工作站(JX4)处理非量测性数码影像的理论与方法,并通过具体试验加以验证。试验结果表明,该方法可实现非量测数码影像的摄影测量一体化作业。  相似文献