Visibilities with an observer coordinate frame (d_sun)
Reorder vis so for each (u,v) as a function of energy
Rescale spectra by fitting a single, broken or sum power laws pick by lowest chi-square (divide by fit to have similar magnitude number to make inversion possible/faster)
Reject low energy bins if error too large (magic number)
Need the SRM for vis energies (attenuator)
get bremsstrahlung cross section
estimate electron flux simple multiplication -> 1st estimate of electron vis
SVD on matrix SRM cross section energy (cm^2 keV-1) [ for photon could do on SRM * energy (cm^2 keV-1)]
regaulisation using SVD, with both discrepancy and 3-sigman -> reg electron vis
confidence strip - perturb the count spectra repeat above to obtain an estimate of confidence