  Quantitative data on the solar wind, solar magnetic fields, solar eruptions,
solar neutrinos, and on the planetary material orbiting the Sun all indicate
the presence of an iron-rich solar interior and a neutron star at the core of
the Sun. Solar magnetic fields are deep-seated remnants from the core and/or
Bose-Einstein condensation of Fe-rich material into a rotating superconductor.
Neutron emission from the core triggers a series of reactions that produce
solar luminosity, the H carrier gas that maintains mass separation in the Sun,
and an outpouring of 3 E43 H+ ions per year in the solar wind.
