Surface Evidence of an Iron-Rich Solar Interior and a Neutron-Rich Solar Core

Details Surface Evidence of an Iron-Rich Solar Interior and a Neutron-Rich Solar Core Surface Evidence of an Iron-Rich Solar Interior and a Neutron-Rich Solar Core

2004-11-06

arxiv.org/abs/astro-ph/0411163v1

Astronomy and Astrophysics

Astrophysics

2 pages, 4 Equations, 14 references, 34th MidAmerican Regional Astrophysics Conference (MARAC), Kansas City, MO 16-17 April 20

Scientific paper

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.

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