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 (19:33 UT on
11, 2010). Click on
the images to see higher resolution versions.
If your movie player can continuously loop a movie
playing it, set this option to "on" for the best effect.
CAUTION: Some of the movies are
very large and are only appropriate for high-speed internet
connections. Please pay attention to the stated sizes of the