solar

SOLAR DYNAMICS

Starlight ionizes atoms in deep space, freeing electrons and electrons are electrically attracted to the solar winds of stars, inducing a voltage potential between stars and deep space powering solar electric currents which transform the voltage potential into kinetic energy until electrical resistance of the solar corona, transforms, kinetic energy into photons.

The corona radiates photons outward as starlight, and downward radiating the ferrite surface below the mantle where photons transform into electron positron pairs and electrons transform into field lines resulting in residual positrons which merge in trios, trios are trapped by transiting electrons and transform into protons.

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:

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 surface was captured by SOHO. This image was taken on May 27th 2005 at 19:13 using the 195A filter that is sensitive to iron ion emissions.

The corona transforms the kinetic energy of the solar electric currents into photons heating the corona, which radiates photons outward as starlight and radiates the core, which transforms photons into protons composing the mantle of liquid hydrogen, which is cooled at the surface as hydrogen sublimates into ionized plasma gas composing the solar wind which escapes from sunspots and coronal holes.

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.