In 1970 Elsworth graduated with honours from the Victoria University of Manchester with a Bachelor of Science degree in Physics. In 1976 she was awarded a Doctor of Philosophy degree[4][5] from the School of Physics at the Victoria University of Manchester.[2][6][7][8] Her thesis work was entitled "A field-compensated multiplex spectrometer for the visible region"[4] and was concerned with the design and implementation of a novel form of field-widened Michelson interferometer designed to study faint, extended sources like those coming from optical emission from the thermosphere.
Professor Elsworth's pioneering work in establishing and maintaining an important scientific investigation into the internal structure of the Sun using helioseismic data from the autonomous Birmingham network of observatories complemented by extant data from modes of intermediate degree has permitted an unprecedented investigation into the inner core of the Sun where the nuclear reactions are taking place. This has led to the conclusion that the deficiency of solar neutrinos detected on Earth was an issue of nuclear physics or particle physics, not of solar modelling; it also established that the very centre of the Sun rotates no more rapidly than the convective envelope, a matter of serious dynamical concern.
Furthermore, Professor Elsworth has led her group to study solar-cycle-related variations in the Sun's convective envelope, providing important structural information to theorists investigating the solar dynamo. Her current extension to seismic studies of stars other than the Sun is already contributing to a transformation in our understanding of stellar evolution.[1]
^"Archived copy". astro.phys.au.dk. Archived from the original on 11 June 2007. Retrieved 12 January 2022.{{cite web}}: CS1 maint: archived copy as title (link)
^Elsworth, Y; James, J F; Sternberg, R S (1974). "A field compensated interference spectrometer for the visible region: the optical design". Journal of Physics E: Scientific Instruments. 7 (10): 813–816. Bibcode:1974JPhE....7..813E. doi:10.1088/0022-3735/7/10/011.
^Chaplin, W. J.; Kjeldsen, H.; Christensen-Dalsgaard, J.; Basu, S.; Miglio, A.; Appourchaux, T.; Bedding, T. R.; Elsworth, Y.; Garcia, R. A.; Gilliland, R. L.; Girardi, L.; Houdek, G.; Karoff, C.; Kawaler, S. D.; Metcalfe, T. S.; Molenda-Zakowicz, J.; Monteiro, M. J. P. F. G.; Thompson, M. J.; Verner, G. A.; Ballot, J.; Bonanno, A.; Brandao, I. M.; Broomhall, A.- M.; Bruntt, H.; Campante, T. L.; Corsaro, E.; Creevey, O. L.; Dogan, G.; Esch, L.; Gai, N.; Gaulme, P.; Hale, S. J.; Handberg, R.; Hekker, S.; Huber, D.; Jimenez, A.; Mathur, S.; Mazumdar, A.; Mosser, B.; New, R.; Pinsonneault, M. H.; Pricopi, D.; Quirion, P.- O.; Regulo, C.; Salabert, D.; Serenelli, A. M.; Aguirre, V. S.; Sousa, S. G.; Stello, D.; Stevens, I. R.; Suran, M. D.; Uytterhoeven, K.; White, T. R.; Borucki, W. J.; Brown, T. M.; Jenkins, J. M.; Kinemuchi, K.; Van Cleve, J.; Klaus, T. C. (2011). "Ensemble Asteroseismology of Solar-Type Stars with the NASA Kepler Mission". Science. 332 (6026): 213–216. arXiv:1109.4723. Bibcode:2011Sci...332..213C. doi:10.1126/science.1201827. PMID21474754. S2CID33911883.
^Bedding, Timothy R.; Mosser, Benoit; Huber, Daniel; Montalbán, Josefina; Beck, Paul; Christensen-Dalsgaard, Jørgen; Elsworth, Yvonne P.; García, Rafael A.; Miglio, Andrea; Stello, Dennis; White, Timothy R.; De Ridder, Joris; Hekker, Saskia; Aerts, Conny; Barban, Caroline; Belkacem, Kevin; Broomhall, Anne-Marie; Brown, Timothy M.; Buzasi, Derek L.; Carrier, Fabien; Chaplin, William J.; Di Mauro, Maria Pia; Dupret, Marc-Antoine; Frandsen, Søren; Gilliland, Ronald L.; Goupil, Marie-Jo; Jenkins, Jon M.; Kallinger, Thomas; Kawaler, Steven; Kjeldsen, Hans; Mathur, Savita; Noels, Arlette; Aguirre, Victor Silva; Ventura, Paolo (2011). "Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars". Nature. 471 (7340): 608–611. arXiv:1103.5805. Bibcode:2011Natur.471..608B. doi:10.1038/nature09935. PMID21455175. S2CID4338871.