磁尾宽频带静电噪声的一种新的激发机制

本文提出了磁尾宽频带静电噪声强谱段的一种新的激发机制。在等离子体片边界层中存在着瞬时的局域性的晨昏电场。电子和离子对该电场的响应不同:在电场存在的区域内,电子作回旋漂移运动,而离子轨道在的时间尺度内可视为直线。由于等离子体片边界层中等离子体是非均匀的,这就导致了电荷分离的产生,从而可激发静电不稳定性。本文通过求解含电场的Vlasov方程,计算了由此产生的不稳定波的频率和增长率,考察了波矢方向。上述计算结果均与强谱段静电噪声的观测特征一致。     

弱耗散作用下非线性Rossby波的调制不稳定

本文使用WKB方法对弱耗散作用下基本气流具有弱切变的行星大气中非线性Rossby波进行了研究,得到了弱耗散的非线性Rossby波振幅所满足的复系数非线性Schrdinger方程,并分别就无耗散和弱耗散的Rossby波的边带稳定性问题进行了讨论,得到了一些新结果.     

地球弓激波前的低频磁流体波

一、引言 在地球弓激波前存在着低频磁流体波。这种低频磁流体波是太阳风在地球弓激波上的反射粒子和太阳风粒子之间相互作用产生的。根据人造卫星的观测资料可以得到,在地球弓激波前,Pc3-4脉动频率范围内的低频磁流体波的主频率和行星际磁场强度     

由岩体失稳讨论地震前兆的复杂性

断层带应变弱化——失稳的地震模式表明,岩体失稳不仅取决于作用的应力水平,而且决定于应变弱化阶段中环境刚度和岩石刚度的相对大小。该模式可能被应用去解释实际观测中出现异常,而其后不发生地震活动的复杂情况。     

涡旋诱发重联模型（Ⅰ）——动力学特性

本文首先从理论上系统地研究了涡旋诱发重联的基本动力学特性.包括:涡旋诱发重联的物理机制;Kelvin-Helmholtz（K-H）不稳定性和撕裂模不稳定性耦合过程;磁流体涡管的基本特性;不同尺度涡旋间的相互作用,动能和磁能间的转化及准稳态时流线、磁力线、等涡度线和等电流密度线的相似性等.用二维MHD数值模拟方法研究了上述一些特性,并与理论分析结论进行了比较.结果表明,模拟结果证实了理论推论.涡旋诱发重联是产生局部磁场重联的重要机制之一,该模型在磁顶区的应用将另文发表.     

SEARCH FOR CORRELATIVITY OF LIGHTNING(STROKE)WITH ATMOSPHERIC STRATIFICATION FACTORS

In this paper the statistical analysis is carried out on the correlation between lightning strokes andatmospheric stratification factors.It is shown that the total number of strokes in lightning process is mainlydecided by environmental temperature at altitude with the residual instability of 5℃(T_r).The instabilityshould also affect the total number of strokc in lightning process.A forecasting equation of stroke in light-ning process has been deduced and two interesting preliminary conclusions have been obtained.     

A swallow-tail type catastrophic model of earthquake process

（殷有泉）（杜静）Ａｓｗａｌｌｏｗ－ｔａｉｌｔｙｐｅｃａｔａｓｔｒｏｐｈｉｃｍｏｄｅｌｏｆｅａｒｔｈｑｕａｋｅｐｒｏｃｅｓｓ￥Ｙｏｕ－ＱｕａｎＹＩＮａｎｄＪｉｎｇＤＵ（ＰｅｋｉｎｇＵｎｉｖｅｒｓｄｙ，Ｂｅｉｊｉｎｇ１００８７１，Ｃｈｉｎａ）（Ｎｏｒｔ...     

从地震模拟看匀阻段与大震的关系

运用滑块模型建立了一个地震活动的计算机模拟系统。对地震活动计算机模型进行反复试验，认识到断层失稳过程中摩擦强度分布的重要性。把在断层滑动中摩擦阻力分布比较均匀的段称为匀阻段。对大地震而言，断层摩擦阻力的大或小都不是决定因素，而具有较长的匀阻段才是发生大震的首要条件     

Baroclinic energetics and zonal plane distribution of monsoon disturbances

The adiabatic, quasi-geostraphic, 25-layer, numerical, linear model with Ekman boundary layer friction is utilised to perform the baroclinic stability analysis of the mean monsoon zonal wind profile. It is shown thec _i is a function of the resultant wavenumber alone. This relation is able to explain the effects of the lateral walls on the unstable waves.The energetics and zonal plane distribution of the short and long preferred viscous waves are computed. The upward motion of the short wave together with the warm (cold) core lies to the west of the surface trough position above (below) 850 mb. Further, it is shown that the main source of kinetic energy for the wave lies in the middle layer (850–700 mb) which is transported to the lower and upper layers. Computed is found to be in good agreement with observed values.