Wavelength-dependent 4D model of solar eclipses using images of the Sun. Currently supporting annotated images from SDO AIA, SOHO EIT, GOES SUVI, Hinode XRT. Can be used for eclipse predictions and scientific analysis.
This is the main repository for the CLEDB code distribution. CLEDB is utilized to infer vector magnetic fields in the solar corona.
Computation of the Thomson scattering of the K-Corona
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