Bibcode
                                    
                            Mosser, B.; Fossat, E.; Schmider, F.-X.
    Referencia bibliográfica
                                    Astronomy and Astrophysics (ISSN 0004-6361), vol. 248, no. 1, Aug. 1991, p. 281-291.
Fecha de publicación:
    
                        8
            
                        1991
            
  Número de citas
                                    51
                            Número de citas referidas
                                    41
                            Descripción
                                    Observations of the Jupiter were carried out using a refined version of
the stellar seismometer with a sensitivity of better than 50 cm/s. The
observations revealed the existence of strong velocity variations of the
planets in the 10-20-min period range. It is concluded that the observed
variations can only be explained as global acoustic modes. The
frequencies of the modes are examined with reference to the internal
structure of the planet.