论文标题
重力分层的两流体等离子体中的慢速磁性波在强烈离子的极限下
Slow magnetoacoustic waves in gravitationally stratified two-fluid plasmas in strongly ionised limit
论文作者
论文摘要
在多流体框架中必须描述与各种物种之间碰撞频率相当的频率的等离子体动力学,其中粒子之间的碰撞相互作用是重要的成分。在我们的研究中,我们将假设带电的颗粒是强烈耦合的,这意味着它们形成了与中性相互作用的单个流体,因此我们将采用两流体模型。在这里,我们旨在研究使用初始值分析在强烈离子的极限下,在两流体太阳大气中在重力分层的磁通管中传播的慢慢香波的进化方程。由于大量颗粒(离子和中性)之间的碰撞相互作用,管理方程是耦合的。在强烈离子的极限中寻求溶液,中性颗粒之间的密度比是一个小参数。该极限与染色体的上部有关。我们的结果表明,与带电颗粒相关的缓慢香肠波传播,因此由于重力分层而导致的截止频率受到临界的影响。对比,对于中性声波,截止值适用于其波长,只有小波长波才能传播。与中性相关的慢速模式是由与离子的碰撞耦合驱动的。
The plasma dynamics at frequencies comparable with collisional frequency between various species has to be described in multi-fluid framework, where collisional interaction between particles is an important ingredient. In our study we will assume that charged particles are strongly coupled, meaning that they form a single fluid that interacts with neutrals, therefore we will employ a two-fluid model. Here we aim to investigate the evolutionary equation of slow sausage waves propagating in a gravitationally stratified flux tube in the two-fluid solar atmosphere in a strongly ionised limit using an initial value analysis. Due to the collisional interaction between massive particles (ions and neutrals) the governing equations are coupled. Solutions are sought in the strongly ionised limit and the density ratio between neutrals and charged particles is a small parameter. This limit is relevant to the upper part of the chromosphere. Our results show that slow sausage waves associated with charged particles propagate such that their possible frequency is affected by a cut-off due to the gravitational stratification. contrast, for neutral acoustic waves the cut-off value applies on their wavelength and only small wavelength waves are able to propagate. Slow modes associated to neutrals are driven by the collisional coupling with ions.