This type of solar wind is characterized by rapid variations in the solar wind parameters, such as speed, density, and magnetic field. Transient solar wind is typically caused by coronal mass ejections and can cause geomagnetic storms.
This type of solar wind is characterized by rapid variations in the solar wind parameters, such as speed, density, and magnetic field. Transient solar wind is typically caused by coronal mass ejections and can cause geomagnetic storms.