冷水坑银矿田成矿条件及矿床特征

冷水坑中生代陆相火山-次火山岩型银矿田的成矿地质条件,着重论述矿田层控叠加型、斑岩型矿床的分布规律、物质组分、矿化分带等基本地质特征。     

日食一厄尔尼诺系数及其应用

通过比较本世纪以来的厄尔尼诺年和日食资料,发现了高纬（包括极区）日食与厄尔尼诺年之间存在着一定的因果关系。通过定义年日食一厄尔厄诺系数Ｒ１和累积日食一厄尔尼诺系数Ｒ２后,可以发现当某年的Ｒ１≥９或Ｒ２≥１０．５级时,则当年必为厄尔尼诺年,反之亦然．本文还提出了日食诱发厄尔尼诺现象的热一动力机制,并预测２０００年将是一个强厄尔尼诺年．     

太平煤矿深厚土层的水文地质工程地质性质

依据对太平煤矿3号煤区深厚土层的水文地质与工程地质勘测及室内外实验结果,分析了主要的水文地质与工程地质特征及其对3号煤开采的影响,对矿区防水煤岩柱留设高度进行了合理确定。      

Post-noon two-minute period pulsating aurora and their relationship to the dayside convection pattern

Poleward-moving auroral forms, as observed by meridian-scanning photometers, in the vicinity of the cusp region are generally assumed to be the optical signature of flux transfer events. Another class of quasi-continuous, short period (1–2 min) wave-like auroral emission has been identified, closely co-located with the convection reversal boundary in the post-noon sector, which is similar in appearance to such cusp aurora. It is suggested that these short period wave-like auroral emissions, the optical signature of boundary plasma sheet precipitation in the region 1 field-aligned current system, are associated with ULF magnetohydrodynamic wave activity, which is observed simultaneously by ground magnetometer stations. This association with ULF wave activity is strengthened by the observation of several harmonic frequencies in the pulsation spectrum, each an overtone of the fundamental standing wave resonance frequency.     

广州气温与厄尔尼诺的多尺度相互联系

通过对广州气温距平和Ｎｉｎｏ　３、Ｎｉｎｏ　１＋２区ＳＳＴＡ序列做小波变换,研究了广州气温变化与ＥＮＳＯ振荡过程之间的多尺度联系,发现它们都存在着强的十年际振荡。年际尺度的振荡为正相关,十年际风度为负相关。由于ＳＳＴＡ的十年际变率是由强厄尔尼诺事件的韵律产生的,因此;广州气温对强烈厄尔尼诺的响应性质上不同于对普通厄尔尼诺的响应．     

应用水化多层次跟踪预报方法研究闽台地区地震的映震特征

本文针对1990年至1999年福建及沿海中强以上地震和台湾7.0级以上地震,利用“八五”攻关的水化多层次跟踪预报方法,研究福建水氡台网观测资料的异常频次变化特征和演化过程,总结其相应的映震特征。     

Possible configurations of the magnetic field in the outer magnetosphere during geomagnetic polarity reversals

Possible configurations of the magnetic field in the outer magnetosphere during geomagnetic polarity reversals are investigated by considering the idealized problem of a magnetic multipole of order m and degree n located at the centre of a spherical cavity surrounded by a boundless perfect diamagnetic medium. In this illustrative idealization, the fixed spherical (magnetopause) boundary layer behaves as a perfectly conducting surface that shields the external diamagnetic medium from the compressed multipole magnetic field, which is therefore confined within the spherical cavity. For a general magnetic multipole of degree n, the non-radial components of magnetic induction just inside the magnetopause are increased by the factor 1 + [(n + 1)/n] relative to their corresponding values in the absence of the perfectly conducting spherical magnetopause. An exact equation is derived for the magnetic field lines of an individual zonal (m = 0), or axisymmetric, magnetic multipole of arbitrary degree n located at the centre of the magnetospheric cavity. For such a zonal magnetic multipole, there are always two neutral points and n – 1 neutral rings on the spherical magnetopause surface. The two neutral points are located at the poles of the spherical magnetopause. If n is even, one of the neutral rings is coincident with the equator; otherwise, the neutral rings are located symmetrically with respect to the equator. The actual existence of idealized higher-degree (n > 1) axisymmetric magnetospheres would necessarily imply multiple (n + 1) magnetospheric cusps and multiple (n) ring currents. Exact equations are also derived for the magnetic field lines of an individual non-axisymmetric magnetic multipole, confined by a perfectly conducting spherical magnetopause, in two special cases; namely, a symmetric sectorial multipole (m = n) and an antisymmetric sectorial multipole (m = n – 1). For both these non-axisymmetric magnetic multipoles, there exists on the spherical magnetopause surface a set of neutral points linked by a network of magnetic field lines. Novel magnetospheric processes are likely to arise from the existence of magnetic neutral lines that extend from the magnetopause to the surface of the Earth. Finally, magnetic field lines that are confined to, or perpendicular to, either special meridional planes or the equatorial plane, when the multipole is in free space, continue to be confined to, or perpendicular to, these same planes when the perfectly conducting magnetopause is present.Also Honorary Research Associate, Rutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 0QX, UK and Visiting Reader in Physics. University of Sussex, Falmer, Brighton BN1 9QH, UK