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A novel type of turbulence, which arises in 2D electron magnetohydrodynamics, is studied by numerical simulation. Energy dissipation rates are found to be independent of the dissipation coefficients. The energy spectrum E₊ follows the basic Kolmogorov-type predictions, k^-5/3 for kd₄>1 and k^-7/3 for kd₄<1 (d₄ is the electron inertial length) and is hence independent of the linear wave properties. Results are compared with other 2D turbulent systems.
Biskamp et al. (Mon,) studied this question.