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ABSTRACT Observing conditions at the geographic South Pole enable modes of global solar oscillations and theoretical models of the internal solar structure to be identified. Access through
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BEING VIEWED BY OTHERS HEIGHT-DEPENDENT DIFFERENTIAL ROTATION OF THE SOLAR ATMOSPHERE DETECTED BY CHASE Article 13 June 2024 THE SOLAR DYNAMO BEGINS NEAR THE SURFACE Article Open access 22
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CAS Google Scholar Download references AUTHOR INFORMATION AUTHORS AND AFFILIATIONS * Département d'Astrophysique de l'IMSP, ERA 669 du CNRS, Université de Nice, Parc Valrose,
Nice Cedex, F-06034, France Gérard Grec * Observatoire de Nice, BP 252, F-06007, Nice, Cedex 2, France Eric Fossat * Bartol Research Foundation of the Franklin Institute, University of
Delaware, Newark, Delaware, 19711 Martin Pomerantz Authors * Gérard Grec View author publications You can also search for this author inPubMed Google Scholar * Eric Fossat View author
publications You can also search for this author inPubMed Google Scholar * Martin Pomerantz View author publications You can also search for this author inPubMed Google Scholar RIGHTS AND
PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE Grec, G., Fossat, E. & Pomerantz, M. Solar oscillations: full disk observations from the geographic South Pole.
_Nature_ 288, 541–544 (1980). https://doi.org/10.1038/288541a0 Download citation * Received: 30 September 1980 * Accepted: 06 November 1980 * Issue Date: 11 December 1980 * DOI:
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