stars

SOLAR DYNAMICS

Protons compose the solar winds of stars and induce monopole charge in the same instant, as 2 electrons cycle through singularity with a positron trio and like charges induced in the same instant are electrically repelled powering the solar wind and filling the heliosphere with solar ions.

Starlight ionizes atoms in deep space, freeing electrons which induce monopole charge in the same instant as solar ions, and opposite charges induced in the same instant are attracted powering solar electric currents which transform potential into kinetic energy until electrical resistance of the solar corona transforms kinetic energy into photons, radiated as starlight and radiating the ferrite core below the corona.

The Solid Solar Surface Model is based upon observations from the YOHKOH, SOHO and TRACE satellite programs, from spectral analysis data compiled by the SERTS program. This “running Difference” image of the sun’s surface was captured by SOHO. This NASA image was taken on May 27th 2005 at 19:13 using the 195A filter that is sensitive to iron ion emissions.

At high photon energy, electron positron pair production is the dominant mode of photon interaction with matter. First observed in Patrick Blackett’s cloud chamber, leading to the 1948 Nobel Prize in Physics. If the photon is near an atomic nucleus, the energy of a photon can be converted into an electron–positron pair:

Photons transforms into electron positron pairs at the core surface where electrons transform into field lines, resulting in residual positrons. Positrons merge in trios, 3 trios are trapped by 4 transiting electrons and transform into protons, and protons deionize into liquid hydrogen, composing the mantle, cooled at the surface by the change of state from H2 into ionized plasma gas composing the solar wind.

Temperatures in the corona are upwards of 2 million degrees Fahrenheeit, while just 1,000 miles below, the underlying surface simmers at a balmy 10,000 F. How the Sun manages this feat remains one of the greatest unanswered questions in astrophysics; scientists call it the coronal heating problem.

The cores of stars are rotating arrays of equal radius ionized spheres of protons, draped in ferrite boundary layers which transform the momentum of moving charges into moments and the sum of moments is captured by the solar field which increases the momentum of orbiting ions in the direction of core rotation, powering super-rotation of the solar atmosphere and solar wind.

The solar field captures repelling forces between core ions. When gravitational collapse disrupts the fields of first generation stars repelling forces between core ions are restored and the star goes supernova.