Why Different Wavelengths?

The left panel indicates that the Sun is being studied at many wavelengths. Different wavelengths are sensitive to different portions of the solar surface and atmosphere, and to different processes.

For example, light passed through a filter to select frequencies near the H-alpha line of the hydrogen Balmer series can't have come from very deep in the atmosphere because hydrogen absorbs this frequency strongly. As a second example, X-rays are produced by high energy particles and image regions of very high temperature or of violent collisions.

Thus, imaging of the Sun at a range of specific wavelengths provides a much greater variety of information than that obtained from simply observing the Sun in white light.