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

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dc.creatorManuel, O.
dc.creatorSingh, Y.
dc.date2004-11-06
dc.date.accessioned2026-07-07T02:15:41Z
dc.date.available2026-07-07T02:15:41Z
dc.descriptionQuantitative 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.
dc.description2 pages, 4 Equations, 14 references, 34th MidAmerican Regional Astrophysics Conference (MARAC), Kansas City, MO 16-17 April 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0411163
dc.identifierhttp://arxiv.org/abs/astro-ph/0411163
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8497
dc.subjectAstrophysics
dc.titleSurface Evidence of an Iron-Rich Solar Interior and a Neutron-Rich Solar Core
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