A. Cacciani

Are Standard Solar Models Reliable?

parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code

Solar neutrinos

Standard Solar Models in the Light of New Helioseismic Constraints. II. Mixing below the Convective Zone

Solar System Abundances and Condensation Temperatures of the Elements

The ‘Standard’ Sun Modelling and Helioseismology

Helioseismology

How Much Do Helioseismological Inferences Depend on the Assumed Reference Model?

FRESH INSIGHTS ON THE STRUCTURE OF THE SOLAR CORE

The Chemical Composition of the Sun

The Internal Rotation of the Sun

MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): PLANETS, OSCILLATIONS, ROTATION, AND MASSIVE STARS

Evidence for Neutrino Oscillations I: Solar and Reactor Neutrinos

The Sudbury Neutrino Observatory

Confirmation of solar cycle-dependent intermediate-degree p-mode frequency shifts

An instrument to observe low-degree solar oscillations

Depth and latitude dependence of the solar internal angular velocity

The magneto-optical filter