Coronal Emission

    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 intergation requires knowledge of the plasma density and temperature in the corona, which we predict using our model.  The images below show the predicted coronal emission at the time of greatest eclipse (22:13 UTC on November 13, 2012).  Click on the images to see higher resolution versions.

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EUV 171Å Emission (AIA) Eclipse Time Full-resolution QuickTime movie (700 kbytes) Full-resolution GIF movie (21 Mbytes) Half-resolution GIF movie (7 Mbytes)	EUV 193Å Emission (AIA) Eclipse Time Full-resolution QuickTime movie (500 kbytes) Full-resolution GIF movie (17 Mbytes) Half-resolution GIF movie (6 Mbytes)	EUV 211Å Emission (AIA) Eclipse Time Full-resolution QuickTime movie (500 kbytes) Full-resolution GIF movie (15 Mbytes) Half-resolution GIF movie (5 Mbytes)	EUV 171Å Emission (EIT) Eclipse Time Full-resolution QuickTime movie (900 kbytes) Full-resolution GIF movie (21 Mbytes) Half-resolution GIF movie (7 Mbytes)
EUV 195Å Emission (EIT) Eclipse Time Full-resolution QuickTime movie (600 kbytes) Full-resolution GIF movie (19 Mbytes) Half-resolution GIF movie (6 Mbytes)	EUV 284Å Emission (EIT) Eclipse Time Full-resolution QuickTime movie 700 kbytes) Full-resolution GIF movie (19 Mbytes) Half-resolution GIF movie (6 Mbytes)	X-Ray Emission (XRT Al-mesh Filter) Eclipse Time Full-resolution QuickTime movie (600 kbytes) Full-resolution GIF movie (18 Mbytes) Half-resolution GIF movie (6 Mbytes)	X-Ray Emission (XRT Ti-poly Filter) Eclipse Time Full-resolution QuickTime movie (500 kbytes) Full-resolution GIF movie (18 Mbytes) Half-resolution GIF movie (6 Mbytes)