Inverse modelling; Sun; Sun—helioseismology; Sun—interior; Astronomy and Astrophysics; Space and Planetary Science
Abstract :
[en] Helioseismology and solar modelling have enjoyed a golden era thanks to decades-long surveys from ground-based networks such as for example GONG, BiSON, IRIS and the SOHO and SDO space missions which have provided high-quality helioseismic observations that supplemented photometric, gravitational, size and shape, limb-darkening and spectroscopic constraints as well as measurements of neutrino fluxes. However, the success of solar models is also deeply rooted in progress in fundamental physics (equation of state of the solar plasma, high-quality atomic physics computations and opacities, description of convection and the role of macroscopic transport processes of angular momentum and chemicals, such as for example meridional circulation, internal gravity waves, shear-induced turbulence or even convection. In this paper, we briefly outline some key areas of research that deserve particular attention in solar modelling. We discuss the current uncertainties that need to be addressed, how these limit our predictions from solar models and their impact on stellar evolution in general. We outline potential strategies to mitigate them and how multidisciplinary approaches will be needed in the future to tackle them.
Research Center/Unit :
STAR - Space sciences, Technologies and Astrophysics Research - ULiège
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Buldgen, Gaël ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Canocchi, Gloria ; Department of Astronomy, Stockholm University, Stockholm, Sweden
Le Saux, Arthur ; AIM, Université Paris Cité, Université Paris-Saclay, CEA, CNRS, Gif-sur-Yvette, France
Baturin, Vladimir A. ; Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, Russian Federation
Trampedach, Regner ; Space Science Institute, Boulder, United States
Oreshina, Anna V. ; Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, Russian Federation
Ayukov, Sergey V. ; Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, Russian Federation
Pradhan, Anil; Dept. Astronomy, Ohio State University, Columbus, United States
Pain, Jean-Christophe; DIF, CEA, DAM, Arpajon, France ; LMCE, Université Paris-Saclay, CEA, Bruyères le Châtel, France
Kunitomo, Masanobu ; Department of Physics, Kurume University, Kurume, Japan ; Laboratoire Lagrange, Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Nice, France
Appourchaux, Thierry; Institut d’Astrophysique Spatiale, UMR 8617, Université Paris-Saclay, CNRS, Orsay Cedex, France
García, Rafael A. ; AIM, Université Paris Cité, Université Paris-Saclay, CEA, CNRS, Gif-sur-Yvette, France
Deal, Morgan ; LUPM, Université de Montpellier, CNRS, Montpellier, France
Grevesse, Nicolas ; Université de Liège - ULiège > Centres généraux > CSL (Centre Spatial de Liège)
Noels, Arlette; STAR Institute, Université de Liège, Liège, Belgium
Christensen-Dalsgaard, Jørgen ; Stellar Astrophysics Centre, and Department of Physics and Astronomy, Aarhus University, Aarhus C, Denmark
Guillot, Tristan ; Laboratoire Lagrange, Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Nice, France
Nandal, Devesh; University of Virginia, Charlottesville, United States
Bétrisey, Jérôme ; Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden
Blancard, Christophe; DIF, CEA, DAM, Arpajon, France
Colgan, James; Los Alamos National Laboratory, Los Alamos, United States
Cossé, Philippe; DIF, CEA, DAM, Arpajon, France
Fontes, Christopher J.; Los Alamos National Laboratory, Los Alamos, United States
Petitdemange, Ludovic; LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Université, Paris, France
Pinçon, Charly; Institut d’Astrophysique Spatiale, UMR 8617, Université Paris-Saclay, CNRS, Orsay Cedex, France
GB acknowledges fundings from the Fonds National de la Recherche Scientifique (FNRS) as a postdoctoral researcher. GC acknowledges funds from the Knut and Alice Wallenberg Foundation. RT acknowledges support from NASA grants 80NSSC20K0543 and 80NSSC-22K0829. The study by V.A.B., A.V.O , and S.V.A. is conducted under the state assignment of Lomonosov Moscow State University. R.A.G. acknowledges the support from the GOLF and PLATO Centre National D\u2019\u00C9tudes Spatiales grants. J.B. acknowledges funding from the SNF Postdoc.Mobility grant no. P (Impact of magnetic activity on the characterization of FGKM main-sequence host-stars). M.K. was supported by the JSPS KAKENHI (grant nos. 24K00654 and 24K07099). AP acknowledges partial support from US National Science Foundation (Astronomy). Los Alamos National Laboratory is operated by Triad National Security, LLC, for the National Nuclear Security Administration of US Department of Energy (Contract No. 89233218NCA000001). This research has made use of the Astrophysics Data System, funded by NASA under Cooperative Agreement 80NSSC21M00561.
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