Learning

Understanding the Basic Properties of the Solar Wind

Plasma: The Fourth State of Matter → Basic Plasma Physics

This learning path introduces high school students with basic physics to the fundamental properties of the solar wind, including its composition, speed, density, temperature, the Parker spiral, and the distinction between fast and slow wind. It begins with essential background in plasma physics and the Sun's atmosphere, then builds up to the detailed characteristics of the solar wind and its large-scale structure.