Coronal Mass Ejections
Coronal Mass Ejections (CMEs) are large expulsions of plasma and magnetic field from the Sun’s corona.
Coronal Mass Ejections (CMEs) are large expulsions of plasma and magnetic field from the Sun’s corona.
Solar flares are large eruptions of electromagnetic radiation from the Sun lasting from minutes to hours.
The solar radio flux at 10.7 cm (2800 MHz) is an excellent indicator of solar activity.
Solar Extreme Ultraviolet (EUV) is solar radiation that covers the wavelengths 10 – 120 nm of the electromagnetic spectrum.