Instrument Data - Presently this reads the Instrument Data from the EIT GENX files on the SSW as provided by J. Lemen.
Data can be whole images, single pixels, or vectors.
These are both subfields contained in the same Level zero file. Response Curves in Solar Physics paper assume a constant emission measure with temperature. Therefore if input observed DN's you can invert the above equation to solve for the emission measure. Since EIT is sensitive to a narrow temperature range and of observations have 3 filters, the true temperature can have fairly good constraints. This page is still under construction.