The Structure of the Sun PDF
418 Pages·1996·8.127 MB·English
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In this timely volume, the editors present eight specially-written chapters by experts renowned for their teaching skills. The chapters show how astronomers can deduce the internal composition (density, helium abundance, etc.) and dynamical structure (rotation, sub-surface velocity fields, etc.) of the Sun through helioseismology, and how researchers can infer the central temperature from measurements of the flux of solar neutrinos.
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