Robin van Spaandonk wrote:
Note that the determination of what the Sun is spewing out is probably based upon spectroscopic evidence, and as Mills has already pointed out, at least one Hydrino line is easily confused with an Fe line. Now which is more likely to be present on the Sun in large quantities, Fe or H?
But even Mills sez that the Hy formation is a coronal effect - and not a core effect.
The lines in question are seen only in flares erupting from the core, and are not in (abundant) evidence otherwise (apparently, or they would have been mentioned).
