Images and Spectra of a solar flare taken from the Solar Dynamics Observatory (SDO) Mission launched in February 2010. Top three panels (l to r): Images showing magnetic loops of the solar flare taken at 9.4 nm, 33.5 nm, and 17.1 nm, respectively, taken by the Atmospheric Imaging Assembly (AIA) aboard the SDO; Fourth panel: graphic related to magnetic field strength at the flare taken by the Helioseismic and Magnetic Imager (HMI). Bottom: Time history of flare emission at 9.4 nm and 33.5 nm taken by the Extreme-Ultraviolet Variability Experiment (EVE) instrument. The initial calibration of EVE and the periodic recalibrations through a duplicate EVE on rocket underflights were done at SURF III. The AIA is periodically cross calibrated against EVE.