P. Gouttebroze et T. Toutain, AN EULERIAN APPROACH FOR THE COMPUTATION OF OSCILLATION MODE VISIBILITY, Astronomy and astrophysics, 287(2), 1994, pp. 535-542
We propose a method to compute the visibility of nonradial oscillation
modes for a star observed in the continuum. This method, based on the
use of Eulerian coordinates, remains valid whenever the geometrical t
hickness of the emitting layer cannot be neglected. Some numerical tes
ts are performed for comparison with the previous formulation of Dziem
bowski (1977), based on the use of Lagrangean coordinates.