Explore the Sun’s hidden depths with ‘The Solar Tachocline.’ This essential astrophysics book delves into the groundbreaking field of helioseismology, revealing the surprising discovery of the tachocline – the abrupt transition zone between the Sun’s outer convection zone and its inner radiative interior. Featuring contributions from leading experts at the Isaac Newton Institute, this comprehensive volume examines the properties and dynamics of the tachocline, blending observational data with cutting-edge theoretical insights into hydrodynamic and magnetohydrodynamic behavior. A must-have reference for astrophysicists, heliospheric physicists, geophysicists, and fluid dynamics researchers seeking to understand solar interior dynamics.