How has the solar wind evolved to reach what it is today? In this review, I discuss the long-term evolution of the solar wind, including the evolution of observed properties that are intimately linked to the solar wind: rotation, magnetism and activity. Given that we cannot access data from the solar wind 4 billion years ago, this review relies on stellar data, in an effort to better place the Sun and the solar wind in a stellar context. I overview some clever detection methods of winds of solar-like stars, and derive from these an observed evolutionary sequence of solar wind mass-loss rates. I then link these observational properties (including, rotation, magnetism and activity) with stellar wind models. I conclude this review then by discussing implications of the evolution of the solar wind on the evolving Earth and other solar system planets. I argue that studying exoplanetary systems could open up new avenues for progress to be made in our understanding of the evolution of the solar wind.

太阳风是如何进化到今天的样子的？在这篇评论中，我讨论了太阳风的长期演化，包括与太阳风密切相关的观测到的特性的演化：旋转、磁性和活动。鉴于我们无法获取40亿年前太阳风的数据，本次回顾依赖于恒星数据，以期更好地将太阳和太阳风置于恒星背景下。我概述了一些类太阳恒星风的巧妙探测方法，并从中得出了观察到的太阳风质量损失率的演化序列。然后，我将这些观测特性（包括旋转、磁性和活动）与恒星风模型联系起来。然后，我通过讨论太阳风的演化对不断演化的地球和其他太阳系行星的影响来结束这篇评论。我认为，研究系外行星系统可以为我们理解太阳风的演化开辟新的途径。