Final answer:
Solar flares, solar wind, and solar rotation can be explained by the interaction of gas and the Sun's magnetic field.
Step-by-step explanation:
The solar features that can be explained by the interaction of gas and the Sun's magnetic field are:
- Solar flares: Flares are intense bursts of energy on the Sun's surface that occur when magnetic fields in the Sun's atmosphere become twisted and release a tremendous amount of electromagnetic radiation.
- Solar wind: The flow of hot, charged particles leaving the Sun is driven by the Sun's magnetic field.
- Solar rotation: By observing sunspots move across the disk of the Sun, we can show that the Sun rotates on its axis.