Morphology of the magnetic transition region, and wave transport and mode mixing through the TR Waves in a magnitized atmosphere(2.5)


"Intensity" and doppler velocity, above piston in radially driven weak field case

left panel: space vs time plots of delta rho/rho (e.g. Intensity), right panel: space vs time plots of uz/cs

 993km two interfering wave-trains: low-beta fast and slow modes

 Chromosphere is not well connected to the driving piston at the photosphere