Coronal heating by turbulent phase mixed MHD waves

Details Coronal heating by turbulent phase mixed MHD waves Coronal heating by turbulent phase mixed MHD waves

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220..249n&link_type=abstract

In ESA The Hydromagnetics of the Sun p 249-251 (SEE N85-25091 14-92)

Physics

1

Magnetohydrodynamic Waves, Plasma Turbulence, Solar Corona, Solar Heating, Energy Transfer, Solar Spectra

Scientific paper

The possibility of transferring mechanical and magnetic energy from MHD waves propagating in the solar corona to smaller and smaller scales via nonlinear effects, starting from a phase-mixed configuration is studied. The efficiency of this turbulent cascade and the turbulent spectra (in space and time) are worked out numerically. The time spectrum suggests the onset of chaotic behavior, The resulting heating rate meets the energetic requirements to heat the corona.

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