This image shows four separate images of the M5.3 class flare from the morning of July 4, 2012. In clockwise order starting at the top left, the wavelengths shown are: 131, 94, 193, and 171 Angstroms. Each wavelength shows a different temperature of material, which in turn corresponds to different levels of the sun’s atmosphere. By looking at images in several wavelengths, scientists can track how a solar eruption moves through the layers.
Credit for the composite is: NASA/SDO/AIA/Helioviewer/TheSunToday