stars

SOLAR DYNAMICS

UV radiation ionizes atoms in deep space which frees electrons and the ionized solar winds of stars induce a voltage potential between stars and deep spacel powering solar electric currents which transform thr voltage potential into kinetic energy until electrical resistance of the corona transforms kinetic energy into photons, radiated outwards as starlight and radiated downward, heating the ferrite surface of the 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.

For photons with high photon energy (MeV scale and higher), pair production is the dominant mode of photon interaction with matter. These interactions were 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 radiated by the corona transform into electron positron pairs at the surface of the core where electrons transform into field lines resulting in residual positrons which merge in trios, trios are trapped by transiting electrons and transform into protons, composing the liquid hydrogen mantle, and the corona, solar wind and interstellar medium of ionized plasma gas.

Temperatures in the corona are upwards of 2 million degrees Fahrenheit, 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.