The Role of Abundances in the Solar Interior Models
Sensitivity of the predicted frequencies of l = 1 gravity modes to known physical processes
Procyon-A and etaBootis: observational frequencies analyzed by the local-wave formalism
Dynamical processes in the solar radiative interior
Dynamical processes in stellar radiation zones: secular magnetohydrodynamics of rotating stars
Detection of periodic signatures in the solar power spectrum On the track of l=1 gravity modes
Cyclic variability of the seismic solar radius from SOHO/MDI and related physics
Comparison of the solar velocity spectrum from MDI and GOLF during cycle 23