The acceleration and heating of the solar wind have been studied for decades using satellite observations and models. However, the exact mechanism that leads to solar wind heating and acceleration is poorly understood. In order to improve the understanding of the physical mechanisms that are involved in these processes a combination of modeling and observational analysis is required. Recent models constrained by satellite observations show that wave heating in the low-frequency (MHD), and high-frequency (ion-cyclotron) range may provide the necessary momentum and heat input to coronal plasma and produce the solar wind. This review is focused on the results of several recent solar modeling studies that include waves explicitly in the MHD and the kinetic regime. The current status of the understanding of the solar wind acceleration and heating by waves is reviewed.

中文翻译：

---

太阳风的波浪建模。

数十年来，使用卫星观测和模型研究了太阳风的加速和加热。但是，人们对导致太阳风加热和加速的确切机制知之甚少。为了更好地理解这些过程中涉及的物理机制，需要将建模和观察分析结合起来。受卫星观测约束的最新模型表明，在低频（MHD）和高频（离子回旋加速器）范围内的波加热可能会向日冕等离子体提供必要的动量和热量输入，并产生太阳风。这篇综述的重点是最近几项太阳建模研究的结果，这些研究包括MHD和动力学模式中明确包含的波浪。