• Corpus ID: 117227378

Solar Energy, Wind, Eruptions, Magnetic Fields, Neutrinos, and Planetary Material: Surface Evidence of an Iron-Rich Solar Interior and a Neutron-Rich Solar Core

@inproceedings{Manuel2004SolarEW,
  title={Solar Energy, Wind, Eruptions, Magnetic Fields, Neutrinos, and Planetary Material: Surface Evidence of an Iron-Rich Solar Interior and a Neutron-Rich Solar Core},
  author={Oliver K. Manuel and Y. Singh},
  year={2004}
}

• O. Manuel, Y. Singh
• Published 6 November 2004
• Physics, Geology

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.