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1 Introduction
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2 Model of the interstellar fast mode spectrum
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3 Approximate and exact calculations of dissipation rate
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4 Revised dissipation rate calculation
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5 Comparison of new expression for dissipation rate with previous expressions
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6 The dependence of the dissipation rate on the plasma 
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7 The magnitude of turbulent dissipation and the heating rate in the DIG
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8 The feasibility of highly anisotropic turbulence spectra
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9 Summary and conclusions
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References
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