Energy source of the solar wind

• Published in: Astrophysics and space science Vol. 71; no. 1; pp. 203 - 209
• Main Authors: Carlqvist, P., Alfv n, H.
• Format: Journal Article
• Language: English
• Published: 01-01-1980
• ISSN: 0004-640X; 1572-946X; 1572-946X
• DOI: 10.1007/BF00646918

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 that occasionally erupt and give rise to expanding loop-like structures in the corona, as observed from Skylab. Because of expansion, the legs of the loops are transformed into coronal rays that 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 in the following ways: 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.