The physics in the auroral dynamo regions and auroral particle acceleration

Y. Song, R.L. Lysak
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引用次数: 30

Abstract

Auroral particle acceleration requires an energy flux flowing into the acceleration region and the subsequent development of parallel electric fields. Auroral arcs are often very dynamic, and even in cases when a quasi-steady arc is formed, the question arises of how the system evolved to this quasi-steady state. Existing theories of auroral current generation and the formation of parallel electric fields mostly consider such a steady situation, limiting their ability to describe the dynamics of the system. Since the energy necessary to power auroral particle acceleration is related to the auroral current system, the generation of field-aligned currents (FAC) and auroral particle acceleration are closely coupled. Thus, in order to understand the dynamics of auroral particle acceleration, the physics in the auroral dynamo region must also be considered. Construction of such a dynamical theory of the auroral current system requires that the time-dependent generation of field-aligned currents (∂J|/∂t) and the dynamics of the generation of parallel electric fields (∂E|/∂t) and parallel potential drops must be the primary considerations.

The time-dependent generation of FAC filaments can occur as a result of the interaction of the MHD fast mode wave packets and a current sheet, either at the magnetopause or in the plasma sheet. In this process, a shear Alfvén wave can be generated in a discrete form as shear Alfvén wave packets. Although a single shear Alfvén wave packet can propagate without distortion or nonlinear interaction, the interaction of incident and reflected shear mode wave packets in the auroral acceleration region can release the kinetic and/or magnetic energy carried by the wave packets. Either solitary waves accompanied by a charge condensation (charge hole) or a net parallel potential drop may be formed, depending on the polarizations of the interacting wave packets. In order to produce FAC filaments and parallel electric fields by the wave packet interaction, a localized breakdown of the frozen-in condition is necessary. The electron inertial term is a natural candidate to break the frozen-in condition locally.

极光发电机区和极光粒子加速中的物理现象
极光粒子加速需要能量流进入加速区域,并随后发展平行电场。极光弧通常是非常动态的,即使在形成准稳定弧的情况下,也会出现系统如何演变到这种准稳定状态的问题。现有的极光电流产生和平行电场形成的理论大多考虑这种稳定的情况,限制了它们描述系统动力学的能力。由于驱动极光粒子加速所需的能量与极光电流系统有关,因此场向电流(FAC)的产生与极光粒子加速密切相关。因此,为了理解极光粒子加速的动力学,还必须考虑极光发电机区域的物理。构建这样一个极光电流系统的动力学理论,首先需要考虑的是场向电流(∂J|/∂t)的时变产生,以及平行电场(∂E|/∂t)和平行电位降的动态产生。在磁层顶或等离子体层中,由于MHD快模波包和电流片的相互作用,FAC细丝的时间依赖性产生可能发生。在此过程中,可以产生一个离散形式的剪切alfv录影带波,即剪切alfv录影带波包。虽然单个剪切alfv录影带波包可以在没有畸变或非线性相互作用的情况下传播,但在极光加速区入射和反射剪切波包的相互作用可以释放波包携带的动能和/或磁能。根据相互作用波包的极化情况,可能形成带有电荷凝聚(电荷空穴)或净平行电位下降的孤立波。为了通过波包相互作用产生FAC细丝和平行电场,必须局部击穿冻结条件。电子惯性项是打破局部冻结状态的自然候选项。
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