The Active Sun from SDO: 4500 Ångstroms

The Solar Dynamics Observatory (SDO) observes the Sun with many different instruments, in many different wavelengths of light. Many of these capabilities are not possible for ground-based observatories - hence the need for a space-based observing platform.

This movie is generated for a wavelength of 4500 Ångstroms (450.0 nanometers) which corresponds to visible light, showing the Sun's visible surface, or photosphere. This wavelength can also be seen from the surface of the Earth, though not with the clarity possible from SDO. The dark regions on the left side are sunspots (Wikipedia) - essentially magnetic storms in the photosphere.

This visualization is one of a set of visualizations (others linked below) covering the same time span of 17 hours over the full wavelength range of the mission. They are setup to play synchronously on a Hyperwall, or can be run individually.

The images are sampled every 36 seconds, 1/3 of the standard time-cadence for SDO. This visualization is useful for illustrating how different solar phenomena, such as sunspots and active regions, look very different in different wavelengths of light. These differences enable scientists to study them more completely, with an eventual goal of improving Space Weather forecasting.