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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.
Hendrix et al. (Thu,) studied this question.