After 30 years of investigation, the solar neutrino problem is still puzzling but the perspectives are extremely encouraging, due to the large improvements obtained on the experimental side including nuclear reaction rates, high statistics in neutrino detections, precise acoustic mode properties and hope to detect gravity modes. The present status, including the differences between neutrino predictions and neutrino flux detections, confirms the general features of solar modelling proposed in the sixties but reveals a rich field of Astrophysics and Particle Physics. The helioseismic investigation of the solar interior with the satellite SOHO begins to offer a complete verification of the solar structure, the introduction of dynamical effects will modify the neutrino emissions and the solar properties on rotation and magnetic field could appear important for the solution of the puzzle if the properties of the neutrinos (mass and magnetic moment) are revealed more complex than thought at the beginning.