Predicted and Observed Coronal Emission:  November 4, 2012 

(Simulation using ADAPT maps)

    We compute emission of radiation from the corona by integrating the emission kernels for extreme ultraviolet (EUV) and X-ray radiation along a chosen line of sight.  This page shows a comparison of observed and simulated emission for SDO/AIA EUV channels on November 4, 2012 at 23:59UTC.   This integration requires knowledge of the plasma density and temperature in the corona, which we predict using our model.  Click on the images to see higher resolution versions.

EUV 94Å Emission (AIA) November 4, 2012  23:59 UTC Observed	EUV 131Å Emission (AIA) November 4, 2012  23:59 UTC Observed	EUV 171Å Emission (AIA) November 4, 2012  23:59 UTC Observed	EUV 193Å Emission (EIT) November 4, 2012  23:59 UTC Observed	EUV 211Å Emission (AIA) November 4, 2012  23:59 UTC Observed	EUV 335Å Emission (AIA) November 4, 2012  23:59 UTC Observed
EUV 94Å Emission (AIA) November 4, 2012  23:59 UTC Simulated	EUV 131Å Emission (AIA) November 4, 2012  23:59 UTC Simulated	EUV 171Å Emission (AIA) November 4, 2012  23:59 UTC Simulated	EUV 193Å Emission (EIT) November 4, 2012  23:59 UTC Simulated	EUV 211Å Emission (AIA) November 4, 2012  23:59 UTC Simulated	EUV 335Å Emission (AIA) November 4, 2012  23:59 UTC Simulated