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- W1681018768 abstract "The Sun has been aptly described as the Rosetta Stone of astronomy. Even though the interior of the Sun is not directly accessible to observations, it has been possible to unravel its internal structure with the help of equations governing the mechanical and thermal equilibrium along with the boundary conditions provided by observations of its mass, radius, luminosity and surface chemical composition. The external layers of the Sun display astonishingly rich dynamics with a host of energetic phenomena occurring at the surface and in the outer atmosphere. An interaction between solar differential rotation, turbulent convection and magnetic field seems to provide an effective mechanism that maintains the solar dynamo and drives the cyclic activity seen at the surface in the form of sunspots. The magnetic field appears to be the guiding force that can effectively supply the energy required for heating the chromospheric and coronal regions. The Sun thus turns out to be an ideal cosmic laboratory for testing atomic and nuclear physics, high-temperature plasma physics and magnetohydrodynamics, neutrino physics and general relativity." @default.
- W1681018768 created "2016-06-24" @default.
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- W1681018768 date "2003-01-01" @default.
- W1681018768 modified "2023-09-24" @default.
- W1681018768 title "Overview of Solar Physics" @default.
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- W1681018768 doi "https://doi.org/10.1007/3-540-36963-5_1" @default.
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