CONTENTS

Introduction
  Overview
  The radial, single fluid, isothermal wind
  ... a pocket history
Solar Wind Energetics
  The energy budget
  The mass flux
  Implications for coronal heating
UVCS observations
  Hydrogen and Oxygen
  Line profiles
  Outflow velocities
  Line widths
Gyrotropic model
  Mass and momentum conservation
  Energy equations
  Heat flux equations
  Momenttum collision terms
  Energy collision terms
  Heat flux collision terms
  Gyrotropic capabilities
  qperp and the mirror force
  The 16 (6) moment code
Initial results and conclusions
  A (new) reference model
  Implications of transition region heating