Delta Scuti stars are high amplitude, nonradial multiperiodic oscillators. The major problem is the identification of the observed frequencies as specific oscillation modes, however this step is important to provide constraints upon the internal structure of the star.

We show here that despite the complicated frequency distributions which can be expected from COROT space mission for a typical delta Scuti star, it will be possible to identify at least some modes or at least the degree for low-l modes from space data.