NEW: THE SUN: AN ELECTRO-MAGNETIC PLASMA DIFFUSER THAT CONTROLS EARTH'S CLIMATE
http://www.omatumr.com/papers.html
There are a number of papers here, read them and let me know what you think
If this is true than our standard model of the sun will need to change.I. INTRODUCTION Hydrogen (H) and other lightweight elements are dominant on stellar surfaces and in the interstellar medium. Since the classical 1957 paper on element synthesis in stars by Burbidge et al. [1], it has been widely assumed that H-fusion is the main driving force for stellar luminosity and ordinary stellar evolution. The idea of a universe driven in one direction by H-fusion fits with the concept of H-production in an initial “Big Bang”. However, a recent analysis of the systematic properties of all 2,850 known nuclides [2] revealed an even larger source of energy from repulsive interactions between neutrons in condensed nuclear matter [3-5]. Those results [3-5] and the abundances of isotopes and elements in meteorites, planets, the solar wind, the solar photosphere, and solar flares [6-9] showed that:
a) The Sun and other stars act as plasma diffusers, sorting lighter ions to their surfaces.
b) The interior of the Sun is made of common elements in rocky planets and meteorites – Fe, Ni, O, Si, and S – although the lightest elements (H and He) cover its surface.
c) Neutron-emission from the solar core, a neutron star, is the first step in a series of reactions that has steadily generated luminosity, neutrinos, solar mass fractionation, and an out-pouring of solar-wind hydrogen from the Sun over the past 4-5 Gy.
d) Neutron-emission from a neutron star is a statistical process, like the radioactive decay of ordinary nuclei via α, β, γ, or spontaneous fission.
The Sun is an ordinary star, probably powered by the same processes as other stars. Prior to these recent papers [3-9], compact nuclear matter or black holes had been considered as the likely energy sources for the violent, more energetic events, like gamma ray bursts and quasars, but not as an energy source that might sustain luminosity in ordinary stars for billions of years.