CONTENTS

Introduction
  Morphology of the magnetic transition region, and wave transport and mode mixing through the TR
  Sketch of the Solar atmosphere
  Chromospheric issues
  Transition region issues
  Chromospheric oscillations
  Exceptions to the "rule"
  The role of the magnetic field
  Reflection due to the magnetic field
  Reflection due the temperature gradient
  Interaction with the Transition Region
  Transition region redshifts i
  Transition region redshifts ii
  Network vs Internetwork velocities
  Coronal driving
  Network line profiles
  A three component transition region?
Waves in a magnitized atmosphere
  Waves generated in the vicinity of "weak" and "strong" field
  "Intensity": radial driving, weak field
  Doppler velocity: radial driving, weak field
  Doppler velocity: radial driving, strong field
  "Intensity" and doppler velocity, above piston in radially driven weak field case
  Observational advice...