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

2004/11/06 by O. Manuel, Manuel, O., Y. Singh +1
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0411163

2 pages, 4 Equations, 14 references, 34th MidAmerican Regional Astrophysics Conference (MARAC), Kansas City, MO 16-17 April 2004

arxiv created 2004/11/06 · arxiv updated 2009/12/01

Abstract

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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