Ion Heating in Coronal Holes and the Fast Solar Wind: A Theoretical Model Based on Plasma Microinstabilities

将建立低β太阳冕洞中电子热流不稳定性的动力学理论，并研究其在快速太阳风加热和加速中的作用。 提出了一种新的范例，其中来自太阳的电子热通量由纳米耀斑产生，然后产生离子回旋波，随后加热覆盖的日冕。 因此，由离子回旋波驱动的太阳风直接耦合到纳米耀斑活动。 一个新的波阻尼机制，涉及参数共振的粒子与泵波驱动的交叉场电流的不稳定性，以及由不稳定性产生的波，将模拟分析和数值。 最后，离子加热的动力学理论在快速太阳风作为一个结果，这种交叉场电流不稳定性将进行调查。

A kinetic theory of the electron heat flux instability in low-beta solar coronal holes will be developed and its role in the heating and acceleration of the fast solar wind will be investigated. A new paradigm is advanced, wherein the electron heat flux coming from the sun is produced by nanoflares and then generates ion cyclotron waves, which subsequently heat the overlying corona. Thus the solar wind driven by ion cyclotron waves is directly coupled to the nanoflare activity. A new wave damping mechanism, involving the parametric resonance of particles with a pump wave which drives a cross-field current instability, and the waves generated by the instability, will be modeled analytically and numerically. Finally, a kinetic theory of ion heating in the fast solar wind as a result of this cross-field current instability will be investigated.