Magnetohydrodynamic Turbulence and Implications for Solar Coronal Heating

Details Magnetohydrodynamic Turbulence and Implications for Solar Coronal Heating Magnetohydrodynamic Turbulence and Implications for Solar Coronal Heating

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...467..887h&link_type=abstract

Astrophysical Journal v.467, p.887

Astronomy and Astrophysics

Astronomy

54

Methods: Numerical, Magnetohydrodynamics: Mhd, Sun: Corona, Turbulence

Scientific paper

During the course of an investigation of coronal heating, we have performed three-dimensional numerical simulations using the model proposed by Parker (t972, 1994), and have studied its ultimate dynamic magnetic-reconnection dissipation mechanism. Our findings suggest that magnetohydrodynamic turbulence plays an important role in the form of the energy spectrum and, hence, in the ohmic heating.

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