solar

SOLAR DYNAMICS

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 coronas of stars transform the kinetic energy of solar electric currents into photons, radiated outward as starlight and radiating the ferrite surface of the core 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.

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 mantle is cooled by transforming photons into protons and by evaporative cooling as mantle hydrogen sublimates at the surface, into the ionized plasma gas composing the solar wind which escapes from Coronal holes and sunspots and composes 95% of the interstellar medium of ionized plasma gas.

The solar core is a rotating array of close packed equal radius, ionized spheres, draped in ferrite boundary layers, which transforms the angular momentum of core moving charges into dipole moments.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 atmosphere and heliosphere sheet.