Energy source of the solar wind

Details Energy source of the solar wind Energy source of the solar wind

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stin...8025266c&link_type=abstract

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Physics

Electric Corona, Energy Transfer, Solar Flares, Solar Wind, Interplanetary Medium, Magnetohydrodynamic Waves, Photosphere, Skylab 3, Solar Corona, Solar Corpuscular Radiation, Theoretical Physics

Scientific paper

A direct transfer of energy from photospheric activity to the solar wind by means of electric currents is discussed. Currents are assumed to flow in quiescent prominences which occasionally erupt and give rise to expanding looplike structures in the corona as observed from Skylab. Due to the expansion the legs of the loops are transformed into coronal rays which carry currents from the photosphere to the outer parts of the corona or interplanetary medium and then back again to the photosphere. It is proposed that energy is transferred from photospheric activity to the solar wind (1) as kinetic energy of the ejected loop matter; (2) as electric power directly fed into the extended loops; and (3) as torsional waves produced by fluctuations in the loop currents.

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