天体磁场发电机理论新进展

全面阐述了宇宙发电机理论的发展。首先简介介绍了天体发电机的理论基础，在此基础上分别讨论了运动学和动力学两大类发电机理论，尤其对运动学中的α－ω发电机理论和动力学发电机中的参数法和直接数值模拟法作了详尽述评，并对其理论的最新发展如非线性、非对称、各向异性和混沌等情况都作了介绍。     

The heating of the solar corona

The heating of the solar corona has been a fundamental astrophysical issue for over sixty years. Over the last decade in particular, space-based solar observatories (Yohkoh, SOHO and TRACE) have revealed the complex and often subtle magnetic-field and plasma interactions throughout the solar atmosphere in unprecedented detail. It is now established that any energy release mechanism is magnetic in origin - the challenge posed is to determine what specific heat input is dominating in a given coronal feature throughout the solar cycle. This review outlines a range of possible magnetohydrodynamic (MHD) coronal heating theories, including MHD wave dissipation and MHD reconnection as well as the accumulating observational evidence for quasi-periodic oscillations and small-scale energy bursts occurring in the corona. Also, we describe current attempts to interpret plasma temperature, density and velocity diagnostics in the light of specific localised energy release. The progress in these investigations expected from future solar missions (Solar-B, STEREO, SDO and Solar Orbiter) is also assessed.Received: 6 February 2003, Published online: 14 November 2003 Correspondence to: R. W. Walsh     

Some Comments on the Magnetic Braking of CP Stars

The low rotation velocities of magnetic CP stars are discussed. Arguments against the involvement of the magnetic field in the loss of angular momentum are given: (1) the fields are not strong enough in young stars in the stage of evolution prior to the main sequence; (2) there is no significant statistical correlation between the magnetic field strength and the rotation period of CP stars; (3) stars with short periods have the highest fields; (4) a substantial number of stars with very low magnetic fields (B _e < 500 G) have rotation speeds that are typical of other CP stars; (5) simulations of the magnetic fields by Leroy and the author show that the orientation of dipoles inside rotating stars, both slow and fast, is consistent with an arbitrary orientation of the dipoles; and, (6) slow rotators with P>25 days, which form 12% of the total, probably lie at the edge of the velocity distribution for low mass stars. All of these properties conflict with the hypothesis of magnetic braking of CP stars.     

物探方法在谢坑矽卡岩型金铜矿勘查中的应用效果

在青海省循化县谢坑矽卡岩型金铜矿勘查中，利用激电异常结合高精度磁测异常确定了矿化体的位置、规模、产状，取得了显著的探矿效果。     

湘南骑田岭地区锡多金属矿的岩石磁学研究

湘南地区骑田岭芙蓉矿田存在众多航磁以及地面高精度磁力异常,正确认识磁异常与锡多金属矿异常的对应关系,直接涉及到对矿区找矿前景的评价与找矿工作部署。笔者从岩石磁学参数的统计特征来探讨磁法勘探的应用范围及其应注意的问题。     

利用核磁共振技术对丘陵油田低渗储层可动油的研究

为了定量评价储层可动油饱和度及渗流能力,应用核磁共振技术对丘陵油田40块岩心的可动油饱和度进行了定量测试.研究表明,丘陵油田低渗透储层可动油饱和度值的分布范围是4.8%~56.7%,平均值为33.4%.可动油饱和度高低与岩心孔隙度、渗透率及驱油效率呈正相关关系.各类储层可动油饱和度差异较大,储层沉积微相及物性决定了可动油饱和度和渗流能力的大小.     

高精度磁测技术在铬铁矿勘探中的应用效果——以仁布超基性岩体为例

西藏仁布县仁布超基性岩体的高精度磁测综合平面图显示，以△T=2000nT组成的等值线闭合圈清晰地反映出超基性岩体的范围，高精度磁测异常与超基性岩体吻合。该区物探推断成果已经得到工程验证，取得良好的效果，首期已采掘铬铁矿近10000t。     

Axial poloidal electromagnetic core-mantle coupling torque: A re-examination for different conductivity and satellite supported geomagnetic field models

We investigate the temporal behaviour of the axial component of the electromagnetic core-mantle coupling torque that is associated with the poloidal part of the geomagnetic field observable at the Earth surface. For its computation, we use different models of the geomagnetic field, expanded into spherical harmonics (Wardinski and Holme, 2006; Sabaka et al., 2004), and the mantle conductivity. The geomagnetic field, which we have to know at the core-mantle boundary for the associated computations, will be inferred from the field at the Earth surface by the non-harmonic field continuation through a conducting mantle shell. The aims of this investigation are (i) to check how sensitive is the computation of the torque with respect to the different geomagnetic field models, (ii) to check its dependence on the spherical harmonic degree n, and (iii) to determine the difference between the mechanical torque derived from the observed length-of-day variations (atmospheric influence subtracted) and the poloidal electromagnetic torque in dependence on the assumed conductivity. To use the non-harmonic field continuation for the torque calculation and to obtain an insight into the influence of the different geomagnetic field models on the EM torques are the major aspects of this paper. grm@gfz-potsdam.de