Intensity and Magnetic Field Distribution of Sunspots     

Trevor Leonard  Debi Prasad Choudhary 《Solar physics》2008,252(1):33-41

We study the relationship between the brightness (I) and magnetic field (B) distributions of sunspots using 272 samples observed at the San Fernando Observatory and the National Solar Observatory, Kitt Peak, whose characteristics varied widely. We find that the I – B relationship has a quadratic form for the spots with magnetic field less than about 2000 G. The slope of the linear part of the I – B curve varies by about a factor of three for different types of spots. In general the slope increases as the spot approaches disk center. The I – B slope does not have a clear dependency on the spot size but the lower limit appears to increase as a function of the ratio of umbra and penumbra area. The I – B slope changes as a function of age of the sunspots. We discuss various sunspot models using these results.  相似文献   

行星际磁通量绳尺度及能量研究     

冯恒强  韩运侠  吴德金  赵寄昆 《天文学进展》2008,26(4)

行星际磁通量绳是太阳风中一种重要的磁结构.从1995-2001年的Wind卫星的观测资料中认证了144个行星际磁通量绳.其时间尺度介于几十分钟到几十小时之间,其空间尺度呈现连续分布.通过估算磁通量绳单位长度的能量和总能量发现:磁通量绳的能量分布和耀斑的类似都呈现很好的幂率谱.通过讨论行星际磁通量绳和太阳活动爆发的关系,建议所有的小、中、大尺度通量绳都直接起源于太阳上的爆发,和磁云对应于通常的日冕物质抛射一样,中、小尺度的通量绳对应相对较小的日冕物质抛射.  相似文献   

Using the quasar VLBI network for the fundamental time—positioning service of the GLONASS space system     

A. M. Finkelstein  E. A. Skurikhina  I. F. Surkis  A. V. Ipatov  I. A. Rakhimov  S. G. Smolentsev 《Astronomy Letters》2008,34(1):59-68

Regular high-precision determinations of the Earth’s orientation parameters (EOPs) on the Quasar VLBI Network were begun in August 2006. The observations are performed within the framework of two national programs: daily sessions at three observatories of the Network to determine all five EOPs (the RU-E program) and 8-h sessions on the Zelenchukskaya-Badary and Svetloe-Badary baselines to determine the Universal Time (the RU-U program). The observations from August 2006 through May 2007 are analyzed. The rms deviations of the EOP values obtained in the RU-E program from the IERS C04 series are 1.1 mas for X _p and Y _p, 37 μs for UT1-UTC, and 0.7 and 0.6 mas for X _c and Y _c, respectively. These results closely match the prospective requirements of GLONASS. The rms deviations of the Universal Times obtained in the RU-U program from the IERS C04 series are 146 μs. We consider the immediate prospects for improving the accuracy of EOP determinations in daily sessions and for implementing the e-VLBI mode for an online determination of the Universal Time. Original Russian Text ? A.M. Finkelstein, E.A. Skurikhina, I.F. Surkis, A.V. Ipatov, I.A. Rakhimov, S.G. Smolentsev, 2008, published in Pis’ma v Astronomicheskiĭ Zhurnal, 2008, Vol. 34, No. 1, pp. 66–76.  相似文献   

Dynamo coefficients from local simulations of the turbulent ISM     

O. Gressel  U. Ziegler  D. Elstner  G. Rüdiger 《Astronomische Nachrichten》2008,329(6):619-624

Observations in polarized emission reveal the existence of large‐scale coherent magnetic fields in a wide range of spiral galaxies. Radio‐polarization data show that these fields are strongly inclined towards the radial direction, with pitch angles up to 35° and thus cannot be explained by differential rotation alone. Global dynamo models describe the generation of the radial magnetic field from the underlying turbulence via the so called α ‐effect. However, these global models still rely on crude assumptions about the small‐scale turbulence. To overcome these restrictions we perform fully dynamical MHD simulations of interstellar turbulence driven by supernova explosions. From our simulations we extract profiles of the contributing diagonal elements of the dynamo α ‐tensor as functions of galactic height. We also measure the coefficients describing vertical pumping and find that the ratio between these two effects has been overestimated in earlier analytical work, where dynamo action seemed impossible. In contradiction to these models based on isolated remnants we always find the pumping to be directed inward. In addition we observe that depends on whether clustering in terms of superbubbles is taken into account. Finally, we apply a test field method to derive a quantitative measure of the turbulent magnetic diffusivity which we determine to be ∼2 kpckms^–1. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Nonhelical mean‐field dynamos in a sheared turbulence     

I. Rogachevskii  N. Kleeorin 《Astronomische Nachrichten》2008,329(7):732-736

Mechanisms of nonhelical large‐scale dynamos (shear‐current dynamo and effect of homogeneous kinetic helicity fluctuations with zero mean) in a homogeneous turbulence with large‐scale shear are discussed. We have found that the shearcurrent dynamo can act even in random flows with small Reynolds numbers. However, in this case mean‐field dynamo requires small magnetic Prandtl numbers (i.e., when Pm < Pm^cr < 1). The threshold in the magnetic Prandtl number, Pm^cr = 0.24, is determined using second order correlation approximation (or first‐order smoothing approximation) for a background random flow with a scale‐dependent viscous correlation time τ_c = (νk 2)^–1 (where ν is the kinematic viscosity of the fluid and k is the wave number). For turbulent flows with large Reynolds numbers shear‐current dynamo occurs for arbitrary magnetic Prandtl numbers. This dynamo effect represents a very generic mechanism for generating large‐scale magnetic fields in a broad class of astrophysical turbulent systems with large‐scale shear. On the other hand, mean‐field dynamo due to homogeneous kinetic helicity fluctuations alone in a sheared turbulence is not realistic for a broad class of astrophysical systems because it requires a very specific random forcing of kinetic helicity fluctuations that contains, e.g., low‐frequency oscillations. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Meridional circulation and dynamo waves     

H. Popova  D. Sokoloff 《Astronomische Nachrichten》2008,329(7):766-768

The effect of meridional circulation on spherical shell dynamos is considered in the Parker approximation. We demonstrate that the type of the exited solution crucially depend on the intensity of the meridional circulation. If the circulation is equatorward or if it is polarward however do not exceed some critical value, an oscillating solution in form of an equatorward traveling wave is excited. If the polarward meridional circulation becomes too intensive the solution becomes steady growing. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

环境磁学理论、方法和研究进展   总被引：32，自引：1，他引：31  

姜月华  殷鸿福  王润华 《地球学报》2004,25(3):357-362

环境磁学是一门介于地球科学、环境科学和磁学之间的边缘科学。环境磁学可提供大量有关区域或全球环境变化及人类活动对环境影响等的重要信息,其研究范围迅速扩大,已成为当今地学前沿学科之一。本文在简述了环境磁学的理论和方法的基础上,介绍了环境磁学中几个主要研究领域如古气候与古环境变化、土壤学和环境污染研究等方面所取得的进展,指出了环境磁学研究中存在的不足之处,并提出了近年来环境磁学的一些新的发展趋势：①加强磁信息与地质记录之间的定量研究;②利用磁信息加强应用研究;③环境磁学与地球化学方法密切相结合;④建立全球磁数据  相似文献   

安徽拂晓地区地物化特征及找矿意义     

罗凡  许强平  严加永  付光明  侯照方 《地质与勘探》2019,55(4):925-938

拂晓地区位于苏鲁超高压变质带安徽段的张八岭地区,地质构造条件与山东段的胶东金矿矿集区类似,具有较好的成矿地质条件和找矿前景。为探索拂晓地区金矿找矿前景,我们系统的开展地物化工作,以面积性的磁法、化探异常为依据,圈定隐伏岩体范围,提供多目标的直接找矿信息,减小找矿范围,预测出两个重点找矿远景区。在重点找矿远景区内,部署了两条可控源音频大地电磁和频谱激电剖面对重点区域的深部纵向结构特征进行探索。综合研究拂晓地区的地物化资料,提出以“弱磁异常-化探异常中心-中等强度的电性异常”为特征的物化探找矿标志;“煌斑岩脉-闪长质脉岩”为特征的地质直接找矿标志;“次级断裂带-不同岩体间的接触带区域”为重点找矿区域的地物化综合找矿方法,有效的增强了找矿能力。为安徽拂晓地区及其邻区的矿产勘查工作提供一定的指示。  相似文献   

扬中金源时代购物中心基坑降水数值模拟分析          下载免费PDF全文

葛鹏  胡远  左新明 《探矿工程》2019,46(4):63-69

基坑降水的成功与否,将对基坑开挖和周边环境产生重要影响,因此有必要对基坑降水方案进行评估。针对扬中金源时代购物中心基坑降水问题,采用MIDAS/GTS对基坑降水效果进行研究。首先,依据地勘报告中提供的土体渗透系数,结合单井、双井抽水试验结果,反演出MIDAS/GTS中需要的土层渗流系数和边界函数;然后利用反演得到的参数,建立了考虑回灌井补水效应的三维基坑降水效果分析模型,模拟基坑内水位降深与时间的变化关系,并对基坑降水效果进行分析和评估,以期指导土方开挖工程的施工。  相似文献   

深部切顶沿空成巷关键参数研究及工程应用     

陈上元  赵菲  王洪建  袁广祥  郭志飚  杨军 《岩土力学》2019,40(1):332-342

传统充填沿空留巷工艺繁琐﹑留巷速度慢,与现代化高强度开采要求不相适应,由此提出了切顶沿空成巷无煤柱开采新技术,其中关键参数设计是该技术的核心问题之一,对留巷的稳定性具有较大影响。以城郊煤矿21304工作面为研究背景,采用理论分析、数值模拟和现场试验等方法,对切顶沿空成巷关键参数进行了系统研究。基于岩石碎胀自承特性和围岩结构“S-R”稳定原理,推导出切顶高度﹑切顶角度的理论计算公式;建立了聚能爆破力学模型,并结合数值模拟和现场试验,确定了聚能爆破装药量及钻孔间距。研究结果表明：合理的切顶参数能够切断巷道顶板与采空区岩层间的力学关系,使采空区顶板沿切缝顺利垮落,碎胀的矸石可有效支撑上覆顶板,限制其回转下沉,减弱覆岩运动对留巷的扰动作用,沿空巷道围岩变形量明显减小。根据理论计算﹑数值分析和现场试验研究成果,确定了城郊煤矿21304工作面切顶沿空成巷关键参数,并在现场进行了应用,回采后沿空巷道侧向顶板能够迅速切落形成巷帮,留巷稳定后各项指标均能满足现场使用要求。  相似文献