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Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 2.TURBULENCE AND CHEMICAL
INHOMOGENEITY
- 2.1.Metallicity Fluctuations:
Observations
- 2.2.How Large Should Metallicity
Fluctuations Be?
- 2.3.Methods of Analysis
- 2.4.How Do The Metals Enter
the Flow?
- 2.5.Turbulent Concentration of
Dust Grains
- 2.6.Turbulent Washout of Radial
Abundance Gradients
3.EFFECTS OF TURBULENCE ON
INTERSTELLAR CHEMISTRY
3.1.Turbulent Transport of Chemical Species
3.2.Turbulent Heating
4.COSMIC RAY SCATTERING AND
ACCELERATION IN A TURBULENT INTERSTELLAR MEDIUM
4.1.Cosmic Ray Scattering in
Magnetic Waves
4.2.Other Scattering
Mechanisms
4.3.Cosmic Ray Acceleration
4.4.Generation of Turbulence
by Cosmic Rays
5.RADIO WAVE SCINTILLATION AS A
DIAGNOSTIC FOR ISM TURBULENCE
5.1.Theory of Diffraction and
Refraction in the ISM
5.2.Observations
5.3.Summary of Scintillation
6.SUMMARY AND REFLECTIONS
REFERENCES