Helioseismology: a fantastic tool to probe the interior of the Sun
M. P. Di Mauro

TL;DR
Helioseismology is a powerful technique that uses solar oscillation data to reveal the Sun's internal structure, rotation, and dynamics, providing insights consistent with models and enabling detailed surface and interior investigations.
Contribution
This paper reviews the development and application of helioseismology techniques to probe the Sun's interior, including recent advances in high-resolution surface and subsurface analysis.
Findings
Solar structure closely matches standard models
Near-surface region can be probed with high spatial resolution
Internal rotation profile of the Sun can be accurately deduced
Abstract
Helioseismology, the study of global solar oscillations, has proved to be an extremely powerful tool for the investigation of the internal structure and dynamics of the Sun. Studies of time changes in frequency observations of solar oscillations from helioseismology experiments on Earth and in space have shown, for example, that the Sun's shape varies over solar cycle timescales. In particular, far-reaching inferences about the Sun have been obtained by applying inversion techniques to observations of frequencies of oscillations. The results, so far, have shown that the solar structure is remarkably close to the predictions of the standard solar model and, recently, that the near-surface region can be probed with sufficiently high spatial resolution as to allow investigations of the equation of state and of the solar envelope helium abundance. The same helioseismic inversion methods can…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Solar Radiation and Photovoltaics
