stars

SOLAR DYNAMICS

Protons compose the solar winds of stars and induce like charge in the same instant as two electrons cycle a positron trio through singularity and like charges induced in the same instant are electrically repelled, powering the solar wind. Starlight ionizes atoms in deep space freeing electrons which cycle in the same instant as solar ions. Opposite charges induced in the same instant are electrically attracted, inducing a voltage potential between stars and deep space.

The voltage potential powers solar electric currents, increasing current kinetic energy until coronal electrical resistance transforms kinetic energy into photons, heating the corona which radiates photons outward, as starlight, and downward, radiating the ferrite core where photons transform into electron positron pairs and electrons transform into field lines resulting in residual positrons.

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 radiating the solar core transform into electron positron pairs where electrons transform into solar field lines resulting in residual positrons which merge in trios, 3 trios are trapped by 4 transiting electrons and transform into protons.

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.

Protons transformed from photons deionize into metallic hydrogen composing the mantle, cooled from below by transformation of photons into protons and cooled at the surface by evaporative cooling, as liquid hydrogen transforms into the 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 ionized rotating cores of stars transform momentum of moving charges into dipole moments. The sum of moments induced by core ions is captured by the solar field, a vector force which increases the momentum of orbiting ions in the direction of rotation powering super-rotation of the ionized atmosphere and solar wind.