Acoustic waves in isothermal winds in the vicinity of the sonic point
Astron. and Astrophys., 322, p.659, 1997.
Roland Grappin, Etienne Cavillier and Marco Velli
Abstract
We study the propagation of acoustic waves incident on the base of a stellar
wind and the back-reaction on the mean flow, in the spherically symmetric,
isothermal case, both analytically and via direct simulations of the
Navier-Stokes equations. We consider successively the quasi-linear inviscid case
and the nonlinear dissipative case (shocks). We show that wave reflection is
small everywhere even when the WKB approximation breaks down, and conjecture
that the same result could hold for radial AlfveÚn waves in a spherically
symmetric wind. We show that, after a transient acceleration, outward
propagating waves lead to a lower mean wind velocity than in the unperturbed
wind, so that the average velocity may become negative below the sonic point,
the difference with the standard result that Lagrangian-mean velocities are
higher in presence of waves being explained by the drift between reference
frames. We propose that negative average velocities might provide a test for the
presence of compressive waves close to the sun. We conjecture that, for MHD
fluctuations, the net effect of the wave pressure on the wind velocity depends
on the importance of compressive components, and that this might play a role in
the observed correlation between the mean solar wind velocity and the level of
the compressive component in the wave spectrum.