Quote:
Originally Posted by oil pan 4
That went way over your head.
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That's probably true, however your response doesn't help me to focus more specifically.
The Parker Solar Probe would be investigating some of the 4% of mass we can sense/ detect in the corona. Electrons, protons, atomic nuclei, neutral hydrogen, ionized hydrogen, particles, magnetized plasma, flares, coronal mass ejection, magnetic sheets, Parker spirals, plages / faculae, irradiance, solar neutrinos, muon-type neutrinos, electron neutrinos, tau-type neutrinos, r-Modes, Rossby waves, inertial oscillations, Coriolis effect, vorticity, convection, ephemeral active regions, x-point magnetic-field topological annihilations, super-heated thin-filament ejection, magnetrohydrodynamics, moats, sunspots, ultraviolet photons, infrared photons, visible photons, X-ray photons, antipodal magnetic fields, synchrotron photons, solar radio photons, solar radio-burst, gamma-ray photons, gravity-lensing, Magnetic periodicies, wave superposition, rogue waves, Alfve'n waves, interplanetary magnetic field, magnetic field storm orientation, upper-atmospheric nitrates, solar wind, latitudinal photospheric rotation, coronal holes, bow- shock compressions, rarifactions, overtaking shockwaves, edge effects, Alfe'n MACH number, ram pressure, stationary draping pattern, wake, current sheets, whistler-type waves, MACH cones.......... the dark side of the Sun.
