How does helioseismology constrain solar neutrino properties?

This review summarizes the advances in solar modelling due to helioseismic measurements. One objective is the correct determination of the different neutrino fluxes and the establishment of the first neutrino properties. The two solar probes (acoustic modes and detected neutrinos) are today in excellent agreement after introduction of the LMA solution for the neutrino oscillations. This consistency is impressive and confirms the interest to look to neutrinos of the Universe. We note that the introduction of recent improvements on essential ingredients of solar modelling put in evidence the limitation of the “Solar Standard Model”. Discrepancies between its results and solar observations are rich of physics beyond this framework, with evident perspectives to look for other neutrino properties, in pursuing the investigation of different objects of the Universe including the Sun.