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MeV Neutrino Sources: The Sun and the Supernovae

Published online by Cambridge University Press:  30 March 2016

Sylvaine Turck-Chièze
Sylvaine Turck-Chièze*
Affiliation:
SAp/DAPNIA/DSM/CEA CE Saclay, 91191 Gif sur Yvette, France

Abstract

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The two sources of MeV neutrinos, the Sun and the Supernovae are very interesting to study nowadays. Seismology aboard SoHO has properly constrained the solar emitted neutrino fluxes and consequently contributes to an unambiguous evidence of the solar neutrino oscillations. The main role of seismology stays nevertheless the description of the magneto-hydrodynamic processes and this progress provokes a renewal of the stellar discipline. Important results are noticed these three years, for the Sun. Future will be richer implying a large number of stars with an evident impact on supernovae and solar neutrino properties.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 9 - 12
Copyright
Copyright © Astronomical Society of Pacific 2005

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