Sun In Time:

Image Channels

304 | 1600 | 1700 | 304-211-171
094-335-193 | 094 | 335 | 131
211-193-171 | 211 | 193 | 171
HMI cont | HMI B(los) | 171-B(los)
Tip: Hover over the wavelength labels underneath the set of images to change the thumbnail image.

Movie links:

Other resources:


Light Curves

(Sorry, the light curve image is not available for this date.)


Images and movies from the Solar Dynamics Observatory (SDO) are not copyrighted unless explicitly noted. The use of SDO images for non-commercial purposes and public education and information efforts is strongly encouraged and requires no expressed authorization. It is requested, however, that any such use properly attributes the source of the images, movies, or derived data products (as appropriate) with a statement such as:
SDO images and movies displayed on this webpage are courtesy of NASA, and the respective AIA and HMI science teams at Lockheed Martin and at Stanford University. The coronal magnetic field visualizations are based on the models described in Schrijver & DeRosa, "Photospheric and Heliospheric Magnetic Fields", which was published in the journal Solar Physics in 2003. Emission measure data are based on the method described in Cheung et al., "Thermal Diagnostics with the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory: A Validated Method for Differential Emission Measure Inversions", which was published in The Astrophysical Journal in 2015.