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

List of tables
List of figures

Copyright ESO 2003
Published by EDP Sciences