The Future of Solar modelling: requirements for a new generation of solar models

Anil Pradhan; Anna V. Oreshina; Arlette Noels; Arthur. Le Saux; Charly Pincon; Christophe Blancard; Devesh Nandal; Gael Buldgen; Gloria. Canocchi; James Colgan

REVIEW 2 major objections 4 minor 242 references

The Future of Solar modelling: requirements for a new generation of solar models

T0 review · 2 major / 4 minor · reviewed 2026-08-07 · deepseek-v4-flash

Challenge this review Re-run · record.json Download PDF Read on arXiv ↗

Pith's one-line read The paper argues that the persistent mismatch between standard solar models and helioseismic and neutrino constraints is not a single missing ingredient but a set of well-identified uncertainties, and that a new generation of solar models…

desk verdict A broad, expert roadmap for solar modelling—valuable as a synthesis, less so as a technical reference; the main weakness is that its prioritized list leans on EOS-dependent helioseismic metallicity determinations while declaring the EOS an open problem. read the letter →

arxiv 2506.14514 v1 pith:QZ5UN52N submitted 2025-06-17 astro-ph.SR

Gael Buldgen , Gloria. Canocchi , Arthur. Le Saux , Vladimir A. Baturin , Regner Trampedach , Anna V. Oreshina , Sergey V. Ayukov , Anil Pradhan

show 17 more authors

Jean-Christophe Pain Masanobu Kunitomo Thierry Appourchaux Rafael A. Garcia Morgan Deal Nicolas Grevesse Arlette Noels Joergen Christensen-Dalsgaard Tristan Guillot Devesh Nandal Jérôme Bétrisey Christophe Blancard James Colgan Philippe Cossé Christopher J. Fontes Ludovic Petitdemange Charly Pincon

This is my paper

classification astro-ph.SR

keywords solarmodellinghelioseismologyabundancesradiativeopacitiesequationofstateangularmomentumtransportneutrinosprotosolaraccretion

verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

Standard solar models reproduce thousands of acoustic oscillation frequencies and measured neutrino fluxes, yet they still disagree with the Sun at the base of the convective zone and in the core. This review argues that the disagreement is not one missing ingredient but a set of named uncertainties: spectroscopic abundances, convective boundary mixing and angular-momentum transport, radiative opacities and the equation of state, and the Sun's accretion and mass-loss history. The paper's central claim is that progress on these fronts, not a single clever fix, is what a new generation of solar models requires. A sympathetic reader should care because the Sun is the calibration anchor for all stellar evolution, so each of these fixes would propagate to asteroseismology and exoplanet host-star characterisation.

What carries the argument

The central object is the standard solar model, a one-dimensional, spherically symmetric stellar evolution calculation calibrated to the Sun's luminosity, radius, and surface composition, and validated against helioseismic frequencies, neutrino fluxes, and spectroscopic abundances. The review's organising mechanism is the comparison between the standard solar model's predicted sound-speed profile, adiabatic exponent profile, helium abundance, and neutrino fluxes and the seismically inferred values. Around that comparison the paper builds a diagnostic map: each discrepancy, such as the sound-speed deviation at the base of the convective zone, the too-low helium abundance with new opacities, or the missing CNO flux, is traced backward to a specific physical ingredient or early-evolution assumption, which then becomes a wish for future work.

What would settle it

A decisive test would be an independent, high-precision CNO neutrino flux measurement from a detector different from Borexino, combined with a laboratory opacity measurement at solar-core conditions: if the CNO flux came out lower than current values while opacity discrepancies persisted, the early-accretion and opacity fixes would both be weakened and the assumption that the listed ingredients are the culprit would fail.

Watch

Extended reading notes

Core claim

The paper's central claim, on its own terms, is that the current solar modelling crisis, the persistent mismatch between standard solar models and helioseismic and neutrino constraints, is unlikely to be resolved by any single revised ingredient. Instead it identifies four interacting fronts: (i) better spectroscopic abundances and atomic data, especially for oxygen and neon; (ii) macroscopic transport processes, including convective overshoot, rotation-induced mixing and internal gravity waves; (iii) microscopic physics, above all radiative opacities, the equation of state of the solar plasma, and microscopic diffusion; and (iv) the early evolution of the Sun, where metal-rich accretion followed by metal-poor accretion can leave a metal-rich core that raises CNO neutrino fluxes. It also argues that the inference techniques used to compare models with data, linear inversions, radius uncertainties, surface effects and activity, need hardening before these physics improvements can be trusted. The authors frame the paper explicitly as a wish-list of key areas of research that deserve particular attention rather than as a solved model.

Load-bearing premise

The load-bearing premise is that the gap between standard solar models and helioseismic and neutrino data is caused by the physical ingredients the review discusses, rather than by a systematic error in the model framework or in the observations themselves.

Editorial extensions

If this is right

If opacities and the equation of state are improved to helioseismic accuracy, standard solar models could simultaneously reproduce the sound-speed profile and the seismically inferred helium abundance, resolving the abundance problem.
If the protosolar accretion scenario of metal-rich early accretion followed by metal-poor late accretion is confirmed, the solar core is more metal-rich than the photosphere, which would raise CNO neutrino fluxes toward the measured values and link solar modelling to planet formation.
If rotation-induced mixing is responsible for lithium depletion, the near-solar beryllium abundance constrains that mixing to be mild, ruling out strong transport at the base of the convective zone.
If solar gravity modes are unambiguously detected, they would directly probe the rotation profile of the inner core and discriminate among angular-momentum transport candidates.
If inversion techniques are extended to nonlinear, sharp-transition schemes, overshoot prescriptions can be constrained locally at the convective boundary instead of being calibrated globally.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

Beyond the paper's explicit list, the same prioritisation implies that near-future laboratory opacity experiments at solar interior conditions would directly test the abundance problem, because a quantified mismatch between theory and experiment at iron or oxygen edges would pinpoint the ingredient at fault.
An implication the authors leave implicit is that if the early-accretion scenario is right, the solar metallicity inferred from photospheric spectroscopy would systematically underestimate the core metallicity, so solar composition should be separated into envelope and core values in future model comparisons.
A testable extension would be to build standard solar models with simultaneous, correlated variations of opacity, diffusion, and accretion history and compare them against a joint helioseismic and neutrino likelihood; the paper lists these ingredients separately, so a joint-inversion framework is the natural next step not described there.

Share X Bluesky LinkedIn Reddit HN

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Desk Editor's Note

read the letter

This is a review/perspective, not a research paper. It presents no new data, equations, or methods. Its contribution is a structured, expert consensus view of where solar modelling needs to go. The author list is deep, and the section-by-section coverage of observational constraints, macroscopic transport, microscopic physics, early evolution, and inference techniques is genuinely useful. The 'wishes' bullets in each section are concrete enough to guide grant proposals and PhD projects.

The synthesis itself is the product—organizing known crises (abundance problem, EOS mismatch, convective boundary, CNO flux confirmation, g-mode detection) into a ranked agenda. There is also a useful discussion of accretion history and pebble formation as a potential solution, which is often left out of solar-model reviews. The paper is honest about uncertainties, e.g. noting that no opacity table provides a global improvement and that all available EOS disagree with Γ1 inversions.

The main concern, which the stress-test note identifies, is the paper's reliance on helioseismic determinations of low metallicity (Buldgen et al. 2017, 2024a; Baturin et al. 2024) as if they were independent of the EOS problem. Those inversions use a chosen EOS, and the same section says the EOS is an open problem. So the list of priorities is partly circular: if a different EOS shifted the inferred envelope Z, the 'abundance problem' could shrink and the ranking would change. The authors do acknowledge the high-Z side (Caffau, Magg) and the degeneracy is well known in the field, so this is not a fatal flaw for a review, but it deserves an explicit caveat.

There are also unfinished editorial artifacts: a citation placeholder '?' in Section 6 and at least one placeholder reference ('In: ???' for Trampedach & Däppen). Those should be fixed before publication.

Who is this for: graduate students and researchers entering solar modelling, and anyone writing a proposal in helioseismology or neutrino astronomy. It is less useful as a technical reference because it is a roadmap, not a derivation.

I would send it to peer review. The author list carries weight, the coverage is broad and mostly balanced, and the field benefits from a written consensus on priorities. The referee should ask for the circularity caveat and the placeholder cleanup, not for new science.

Referee Report

2 major / 4 minor

Summary. This review paper, authored by a broad group of solar and stellar physicists, assesses the current limitations of standard solar models and proposes a research agenda for the next generation of models. After summarizing observational constraints from spectroscopy, helioseismology, and neutrinos, it discusses macroscopic processes (convection, rotation, overshoot), microscopic physics (diffusion, equation of state, opacities), early evolution (accretion, mass loss), and inference techniques. The central claim is that the remaining discrepancies between solar models and observations are attributable to a set of identifiable uncertainties, particularly low solar metallicity, opacities, and the equation of state, and that targeted, multidisciplinary progress in these areas is required. The paper concludes with a list of concrete 'wishes,' including renewed opacity calculations, improved equations of state, independent CNO neutrino confirmation, g-mode detection, and constraints on protosolar disk evolution.

Significance. If accurate, the paper provides a useful roadmap for the solar modelling community and connects solar physics to atomic physics, planet formation, and asteroseismology. Its strengths include the breadth of expert coverage, the clear and actionable summary lists at the end of each section, the up-to-date inclusion of laboratory opacity experiments and neutrino results, and the explicit links to PLATO and future measurements. The paper is also honest about uncertainties, for example in the protosolar disk lifetime and the mass-loss history. However, because the review's prioritization is built on the premise that the solar metallicity is low, the internal tension between the EOS-based helioseismic Z determinations and the paper's own statement that the equation of state is an open problem must be addressed before the roadmap can be considered robust.

major comments (2)

[§1, §2.1, §4] The review treats the helioseismic determinations of low solar metallicity (Buldgen et al. 2017, 2024a; Baturin et al. 2024) as independent confirmation of the low-Z abundance scale, but these determinations are inferred from the adiabatic exponent Γ1 using a chosen equation of state, as the paper itself notes when describing the Baturin et al. (2022) method as an 'EOS-based abundance estimate.' The same section states that all available EOS lie well outside the uncertainties of helioseismic Γ1 inversions and that the equation of state is 'still an open problem.' This creates a circularity: the diagnostic used to select the low-Z premise depends on the very ingredient the review later identifies as a source of the discrepancy. The authors should either quantify the sensitivity of the inferred envelope Z to the choice of EOS (FreeEOS, ChemEOS, OPAL, SAHA-S) or explicitly frame the helioseismic Z results as provisional and model-dependent. As written, the ordering of research priorities in the conclusion is not robust to this potential systematic error.
[§4, opacity paragraph] The claim that 'none of them provide a global improvement to the agreement of standard solar models with helioseismic data' and that OPAS/OPLIB improve the sound-speed profile at the expense of a lower helium abundance is central to the review's conclusion that opacity revisions are not a sufficient fix. However, no quantitative comparison is shown; Figure 1 compares OP and OPLIB opacities at the same thermodynamical coordinates, not the resulting solar model agreement or the helium abundance. Please provide a reference to a direct side-by-side model comparison or show the relevant helioseismic diagnostics; otherwise this strong negative claim is difficult to evaluate.

minor comments (4)

[§6] The sentence 'Recent findings also indicate that the inferred solar age determined through helioseismology varies significantly with the solar activity cycle ( ?)' contains an unresolved placeholder '?'; please add the appropriate citation or remove the claim.
[§5, mass-loss paragraph] The sentence 'These empirical laws lead to the solar initial mass Minitial > 1.01 M⊙ and Minitial ∼ 1.0005 M⊙, respectively' is unclear because the two values are not explicitly tied to the named studies in that sentence; please spell out which power law gives which mass.
[§2.2] The statement that 'the most recent review of paths to g-mode detection can be found in Appourchaux and Pallé (2013)' is more than a decade old; please update with any newer review or state explicitly that no newer comprehensive review exists.
[References] The reference 'Trampedach, R., Däppen, W.: 2024, Various Modifications to Debye-Hückel Interactions in Solar Equations of State. In: ???, 1.' contains a placeholder '???'; the actual volume and publisher must be supplied.

Circularity Check

0 steps flagged · score 1.0 of 10

No circular derivation: the paper is a review/roadmap whose low-Z premise has independent spectroscopic support, with only minor self-citation and an acknowledged EOS-dependence caveat.

full rationale

This is a review paper, not a derivation: its central claim is the abstract's statement that 'we briefly outline some key areas of research that deserve particular attention in solar modelling'. There is no fitted parameter renamed as a prediction and no equation whose output is its input by construction. The closest candidate for circularity is the use of the authors' own helioseismic metallicity determinations, e.g. 'recent helioseismic determinations of the solar metallicity (Vorontsov et al., 2013; Buldgen et al., 2017, 2024a; Baturin et al., 2024) ... confirm the lower abundance of oxygen as well as the lower solar metallicity' (Section 1). These are self-citations, but they are not the only load-bearing support: the same sentence also cites the external 3D-NLTE spectroscopic analysis Asplund, Amarsi, and Grevesse (2021), and the paper explicitly acknowledges the opposing view that 'some groups claiming a higher solar metallicity (Caffau et al., 2011; Magg et al., 2022)'. The skeptical concern about EOS dependence is real but is stated in the paper itself: Section 4 notes that 'all available EOS lie well outside the uncertainties of helioseismic inversions of Γ1' and calls the equation of state 'still an open problem', while also describing how the Baturin et al. (2022) method can be used 'to obtain an EOS-based abundance estimate of metals, against a seismic determination of the Sun's Γ1 profile'. That is a model-dependent inference from seismic data, not a circular identity: the seismic Γ1 profile is an external observable, and the paper openly identifies the EOS as the ingredient needing improvement rather than treating it as a verified input. The manuscript also contains an editorial gap, an unresolved citation '( ?)' in Section 6 regarding the solar-age variation with the activity cycle; this is a missing reference, not a circular step. Overall, the review's recommendations are grounded in an acknowledged, well-documented open problem rather than in a self-referential reduction, so the circularity score is low.

Assumptions & free parameters 0 free parameters · 3 assumptions · 0 invented entities

As a review, the paper introduces no new entities or free parameters. It relies on the standard assumptions of solar and stellar modelling and on the reliability of prior observations and computations, including helioseismic inversions, neutrino flux measurements, and theoretical opacity tables.

assumptions (3)

domain assumption The standard solar model framework, with 1D spherically symmetric structure and calibrated mixing-length parameter, is a valid baseline.
Invoked throughout the paper, e.g., Section 3 discusses improvements to this framework rather than replacing it.
domain assumption Helioseismic inversions provide reliable estimates of solar structure and the adiabatic exponent.
Section 2.2 treats helioseismology as the backbone of model validation, and Section 4 uses inversions of Gamma_1 to constrain the equation of state.
domain assumption Neutrino fluxes, particularly the CNO flux, are sensitive to the core composition and temperature and can constrain the early evolution of the Sun.
Section 2.3 and Section 5 discuss accretion scenarios that alter the core metallicity and would be tested via neutrino fluxes.

how reviews work

0 comments

Cite this review

Pith. "Pith review of The Future of Solar modelling: requirements for a new generation of solar models." pith.science (2026). https://pith.science/paper/QZ5UN52N

@misc{pith2026250614514,
  author       = {Pith},
  title        = {Pith review of: The Future of Solar modelling: requirements for a new generation of solar models},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/QZ5UN52N}},
  note         = {Machine review of arXiv:2506.14514}
}

read the original abstract

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.

Figures

Figures reproduced from arXiv: 2506.14514 by the authors.

**Figure 1.** Comparison between the OP and OPLIB opacities in the solar radiative zone, on the same thermodynamical coordinates (ρ, T, X, Z). Whether one uses OPAS or OPLIB, the sound speed profile is improved at the expense of a lower helium abundance in the convective zone (well outside the helioseismic uncertainty) and, for the OPLIB opacities, a significant disagreement in neutrino fluxes. These effects are due to differenc… view at source ↗

**Figure 2.** Contribution of chemical various elements to the Rosseland mean opacity in three characteristic regions of the radiative interior of the Sun. The Z-pinch experiments at Sandia, together with the solar oxygen abundance problem, have focused theoretical efforts on iron L-shell 2p-nd (n = 3 and 4) transitions. It would be worth investigating the ∆n = 0 (3s-3p and 3p-3d) transitions (Da Silva et al., 1992), which are lo… view at source ↗

**Figure 3.** Relative differences in squared adiabatic sound speed for models built with various abundances and opacity tables (namely AAG21, AGSS09 and MB22 for abundances and OPAS, OPLIB and OPAL for opacities). illustrates this issue, whose origin has been linked to multiple causes. Most notably, these include the chemical composition of the solar radiative zone, the opacity of the solar plasma, the effects of the thermalizat… view at source ↗

Discussion (0). Sign in to comment.

Reference graph

Works this paper leans on

242 extracted references · 62 canonical work pages

[1]

, Aliotta , M

botherref Acharya , B. , Aliotta , M. , Balantekin , A.B. , Bemmerer , D. , Bertulani , C.A. , Best , A. , Brune , C.R. , Buompane , R. , Cavanna , F. , Chen , J.W. , Colgan , J. , Czarnecki , A. , Davids , B. , deBoer , R.J. , Delahaye , F. , Depalo , R. , Garc \' a , A. , Gatu Johnson , M. , Gazit , D. , Gialanella , L. , Greife , U. , Guffanti , D. , G...

work page doi:10.48550/arxiv.2405.06470 2024
[2]

, Mathis , S

barticle Aerts , C. , Mathis , S. , Rogers , T.M. : 2019 , Angular Momentum Transport in Stellar Interiors . 57 , 35 . https://doi.org/10.1146/annurev-astro-091918-104359 . 2019ARA&A..57...35A . barticle

doi:10.1146/annurev-astro-091918-104359 2019
[3]

, Barklem , P.S

barticle Amarsi , A.M. , Barklem , P.S. , Asplund , M. , Collet , R. , Zatsarinny , O. : 2018 , Inelastic O+H collisions and the O I 777 nm solar centre-to-limb variation . 616 , A89 . https://doi.org/10.1051/0004-6361/201832770 . 2018A&A...616A..89A . barticle

doi:10.1051/0004-6361/201832770 2018
[4]

, Grevesse , N

barticle Amarsi , A.M. , Grevesse , N. , Asplund , M. , Collet , R. : 2021 , The solar carbon, nitrogen, and oxygen abundances from a 3D LTE analysis of molecular lines . 656 , A113 . https://doi.org/10.1051/0004-6361/202141384 . 2021A&A...656A.113A . barticle

doi:10.1051/0004-6361/202141384 2021
[5]

, Ogneva , D

barticle Amarsi , A.M. , Ogneva , D. , Buldgen , G. , Grevesse , N. , Zhou , Y. , Barklem , P.S. : 2024 , The solar beryllium abundance revisited with 3D non-LTE models . 690 , A128 . https://doi.org/10.1051/0004-6361/202451778 . 2024A&A...690A.128A . barticle

doi:10.1051/0004-6361/202451778 2024
[6]

, Lecoanet , D

barticle Anders , E.H. , Lecoanet , D. , Brown , B.P. : 2019 , Entropy Rain: Dilution and Compression of Thermals in Stratified Domains . 884 , 65 . https://doi.org/10.3847/1538-4357/ab3644 . 2019ApJ...884...65A . barticle

doi:10.3847/1538-4357/ab3644 2019
[7]

O . , Pietrofaccia , L. , Pilipenko , N. , Pocar , A. , Raikov , G. , Ranalli , M.T. , Ranucci , G. , Razeto , A. , Re , A. , Redchuk , M. , Rossi , N. , Sch \

barticle Appel , S. , Bagdasarian , Z. , Basilico , D. , Bellini , G. , Benziger , J. , Biondi , R. , Caccianiga , B. , Calaprice , F. , Caminata , A. , Cavalcante , P. , Chepurnov , A. , D'Angelo , D. , Derbin , A. , Di Giacinto , A. , Di Marcello , V. , Ding , X.F. , Di Ludovico , A. , Di Noto , L. , Drachnev , I. , Franco , D. , Galbiati , C. , Ghiano ...

2022
[8]

, Corbard , T

barticle Appourchaux , T. , Corbard , T. : 2019 , Searching for g modes. II. Unconfirmed g-mode detection in the power spectrum of the time series of round-trip travel time . 624 , A106 . https://doi.org/10.1051/0004-6361/201935196 . 2019A&A...624A.106A . barticle

doi:10.1051/0004-6361/201935196 2019

Show all 242 references

[9]

, Pall \'e , P.L

bchapter Appourchaux , T. , Pall \'e , P.L. : 2013 , The History of the g-mode Quest . In: Jain , K. , Tripathy , S.C. , Hill , F. , Leibacher , J.W. , Pevtsov , A.A. (eds.) Fifty Years of Seismology of the Sun and Stars , Astronomical Society of the Pacific Conference Series ...

2013 doi arXiv
[10]

u ger , H. , L \

barticle Appourchaux , T. , Burston , R. , Chen , Y. , Cruise , M. , Dittus , H. , Foulon , B. , Gill , P. , Gizon , L. , Klein , H. , Klioner , S. , Kopeikin , S. , Kr \"u ger , H. , L \"a mmerzahl , C. , Lobo , A. , Luo , X. , Margolis , H. , Ni , W.-T. , Pat \'o n , A.P. , ...

2009
[11]

, Amarsi , A.M

barticle Asplund , M. , Amarsi , A.M. , Grevesse , N. : 2021 , The chemical make-up of the Sun: A 2020 vision . 653 , A141 . https://doi.org/10.1051/0004-6361/202140445 . 2021A&A...653A.141A . barticle

2021 doi
[12]

, Grevesse , N

bchapter Asplund , M. , Grevesse , N. , Sauval , A.J. : 2005 , The Solar Chemical Composition . In: Barnes , I. Thomas G. , Bash , F.N. (eds.) Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis , Astronomical Society of the Pacific Conference Series 336 , 25...

2005
[13]

, Wiedemann , G.R

barticle Ayres , T.R. , Wiedemann , G.R. : 1989 , Non--LTE CO Revisited . 338 , 1033 . https://doi.org/10.1086/167256 . 1989ApJ...338.1033A . barticle

1989 doi
[14]

, Gilbert , F

barticle Backus , G. , Gilbert , F. : 1968 , The Resolving Power of Gross Earth Data . Geophysical Journal 16 , 169 . https://doi.org/10.1111/j.1365-246X.1968.tb00216.x . 1968GeoJ...16..169B . barticle

1968 doi
[15]

, Gilbert , F

barticle Backus , G. , Gilbert , F. : 1970 , Uniqueness in the Inversion of Inaccurate Gross Earth Data . Philosophical Transactions of the Royal Society of London Series A 266 , 123 . https://doi.org/10.1098/rsta.1970.0005 . 1970RSPTA.266..123B . barticle

1970
[16]

, Nagayama , T

barticle Bailey , J.E. , Nagayama , T. , Loisel , G.P. , Rochau , G.A. , Blancard , C. , Colgan , J. , Coss \'e , P. , Faussurier , G. , Fontes , C.J. , Gilleron , F. , Golovkin , I. , Hansen , S.B. , Iglesias , C.A. , Kilcrease , D.P. , MacFarlane , J.J. , Mancini , R.C. , Na...

2015
[17]

, Beeck , B

barticle Ball , W.H. , Beeck , B. , Cameron , R.H. , Gizon , L. : 2016 , MESA meets MURaM: Surface effects in main-sequence solar-like oscillators computed using three-dimensional radiation hydrodynamics simulations . A&A 592 , A159:1 . http://cdsads.u-strasbg.fr/abs/2016arXiv...

2016
[18]

, Pratt , J

barticle Baraffe , I. , Pratt , J. , Vlaykov , D.G. , Guillet , T. , Goffrey , T. , Le Saux , A. , Constantino , T. : 2021 , Two-dimensional simulations of solar-like models with artificially enhanced luminosity. I. Impact on convective penetration . 654 , A126 . https://doi.o...

2021 doi
[19]

, Constantino , T

barticle Baraffe , I. , Constantino , T. , Clarke , J. , Le Saux , A. , Goffrey , T. , Guillet , T. , Pratt , J. , Vlaykov , D.G. : 2022 , Local heating due to convective overshooting and the solar modelling problem . 659 , A53 . https://doi.org/10.1051/0004-6361/202142666 . 2...

2022 doi
[20]

, Amarsi , A.M

botherref Barklem , P.S. , Amarsi , A.M. : 2024, Revisiting the statistical equilibrium of H ^- in stellar atmospheres . arXiv e-prints, arXiv:2407.19833. https://doi.org/10.48550/arXiv.2407.19833 . 2024arXiv240719833B . botherref

2024 doi arXiv
[21]

O . , Pietrofaccia , L. , Pilipenko , N. , Pocar , A. , Raikov , G. , Ranalli , M.T. , Ranucci , G. , Razeto , A. , Re , A. , Rossi , N. , Sch \

barticle Basilico , D. , Bellini , G. , Benziger , J. , Biondi , R. , Caccianiga , B. , Calaprice , F. , Caminata , A. , Chepurnov , A. , D'Angelo , D. , Derbin , A. , Di Giacinto , A. , Di Marcello , V. , Ding , X.F. , Di Ludovico , A. , Di Noto , L. , Drachnev , I. , Franco ...

2023
[22]

, Pinsonneault , M

barticle Basinger , C. , Pinsonneault , M. , Bastelberger , S.T. , Gaudi , B.S. , Domagal-Goldman , S.D. : 2024 , Constraints on the early luminosity history of the Sun: applications to the Faint Young Sun problem . 534 , 2968 . https://doi.org/10.1093/mnras/stae2280 . 2024MNR...

2024 doi
[23]

, Christensen-Dalsgaard , J

barticle Basu , S. , Christensen-Dalsgaard , J. : 1997 , Equation of state and helioseismic inversions. 322 , L5 . https://doi.org/10.48550/arXiv.astro-ph/9702162 . 1997A&A...322L...5B . barticle

1997 doi arXiv
[24]

, D \"a ppen , W

barticle Baturin , V.A. , D \"a ppen , W. , Morel , P. , Oreshina , A.V. , Th \'e venin , F. , Gryaznov , V.K. , Iosilevskiy , I.L. , Starostin , A.N. , Fortov , V.E. : 2017 , Equation of state SAHA-S meets stellar evolution code CESAM2k . 606 , A129 . https://doi.org/10.1051/...

2017 doi
[25]

, Oreshina , A.V

barticle Baturin , V.A. , Oreshina , A.V. , D \"a ppen , W. , Ayukov , S.V. , Gorshkov , A.B. , Gryaznov , V.K. , Iosilevskiy , I.L. : 2022 , Ionization of heavy elements and the adiabatic exponent in the solar plasma . 660 , A125 . https://doi.org/10.1051/0004-6361/202141873 ...

2022 doi
[26]

, Oreshina , A.V

barticle Baturin , V.A. , Oreshina , A.V. , Buldgen , G. , Ayukov , S.V. , Gryaznov , V.K. , Iosilevskiy , I.L. , Noels , A. , Scuflaire , R. : 2024 , Heavy Elements Abundances Inferred from the First Adiabatic Exponent in the Solar Envelope . 299 , 142 . https://doi.org/10.10...

2024 doi
[27]

, Ayukov , S.V

barticle Baturin , V.A. , Ayukov , S.V. , Oreshina , A.V. , Gorshkov , A.B. , Gryaznov , V.K. , Iosilevskiy , I.L. , D \"a ppen , W. : 2025 , Hydrogen Ionization Inside the Sun . 300 , 3 . https://doi.org/10.1007/s11207-024-02413-9 . 2025SoPh..300....3B . barticle

2025 doi
[28]

, Mosser , B

barticle Bedding , T.R. , Mosser , B. , Huber , D. , Montalb \'a n , J. , Beck , P. , Christensen-Dalsgaard , J. , Elsworth , Y.P. , Garc \' a , R.A. , Miglio , A. , Stello , D. , White , T.R. , De Ridder , J. , Hekker , S. , Aerts , C. , Barban , C. , Belkacem , K. , Broomhal...

2011
[29]

, Gonzalez-Garcia , M.C

barticle Bergstr \"o m , J. , Gonzalez-Garcia , M.C. , Maltoni , M. , Pe \ n a-Garay , C. , Serenelli , A.M. , Song , N. : 2016 , Updated determination of the solar neutrino fluxes from solar neutrino data . Journal of High Energy Physics 2016 , 132 . https://doi.org/10.1007/J...

2016 doi
[30]

, Hu , H

barticle B \"o ning , V.G.A. , Hu , H. , Gizon , L. : 2019 , Signature of solar g modes in first-order p-mode frequency shifts . 629 , A26 . https://doi.org/10.1051/0004-6361/201935434 . 2019A&A...629A..26B . barticle

2019 doi
[31]

, Sackmann , I.-J

barticle Boothroyd , A.I. , Sackmann , I.-J. : 2003 , Our Sun. IV. The Standard Model and Helioseismology: Consequences of Uncertainties in Input Physics and in Observed Solar Parameters . 583 , 1004 . https://doi.org/10.1086/345407 . 2003ApJ...583.1004B . barticle

2003 doi
[32]

O . , Pilipenko , N. , Pocar , A. , Porcelli , A. , Raikov , G. , Ranucci , G. , Razeto , A. , Re , A. , Redchuk , M. , Romani , A. , Roncin , R. , Rossi , N. , Sch \

barticle Borexino Collaboration , Agostini , M. , Altenm \"u ller , K. , Appel , S. , Atroshchenko , V. , Bagdasarian , Z. , Basilico , D. , Bellini , G. , Benziger , J. , Bick , D. , Bonfini , G. , Bravo , D. , Caccianiga , B. , Calaprice , F. , Caminata , A. , Caprioli , S. ...

2018
[33]

O . , Pietrofaccia , L. , Pilipenko , N. , Pocar , A. , Raikov , G. , Ranalli , M.T. , Ranucci , G. , Razeto , A. , Re , A. , Redchuk , M. , Romani , A. , Rossi , N. , Sch \

barticle Borexino Collaboration , M. Agostini , Altenm \"u ller , K. , Appel , S. , Atroshchenko , V. , Bagdasarian , Z. , Basilico , D. , Bellini , G. , Benziger , J. , Biondi , R. , Bravo , D. , Caccianiga , B. , Calaprice , F. , Caminata , A. , Cavalcante , P. , Chepurnov ,...

2020
[34]

, Matt , S.P

botherref Bouvier , J. , Matt , S.P. , Mohanty , S. , Scholz , A. , Stassun , K.G. , Zanni , C. : 2014, Angular Momentum Evolution of Young Low-Mass Stars and Brown Dwarfs: Observations and Theory . Protostars and Planets VI, 433. https://doi.org/10.2458/azu_uapress_9780816531...

2014 doi
[35]

: 2016 , Stellar Mixing Length Theory with Entropy Rain

barticle Brandenburg , A. : 2016 , Stellar Mixing Length Theory with Entropy Rain . 832 , 6 . https://doi.org/10.3847/0004-637X/832/1/6 . 2016ApJ...832....6B . barticle

2016 doi
[36]

, Nakariakov , V.M

barticle Broomhall , A.-M. , Nakariakov , V.M. : 2015 , A Comparison Between Global Proxies of the Sun's Magnetic Activity Cycle: Inferences from Helioseismology . 290 , 3095 . https://doi.org/10.1007/s11207-015-0728-6 . 2015SoPh..290.3095B . barticle

2015 doi
[38]

, Miesch , M.S

barticle Brun , A.S. , Miesch , M.S. , Toomre , J. : 2011 , Modeling the Dynamical Coupling of Solar Convection with the Radiative Interior . 742 , 79 . https://doi.org/10.1088/0004-637X/742/2/79 . 2011ApJ...742...79B . barticle

2011 doi
[39]

, Salmon , S.J.A.J

barticle Buldgen , G. , Salmon , S.J.A.J. , Noels , A. , Scuflaire , R. , Dupret , M.A. , Reese , D.R. : 2017 , Determining the metallicity of the solar envelope using seismic inversion techniques . 472 , 751 . https://doi.org/10.1093/mnras/stx2057 . 2017MNRAS.472..751B . barticle

2017 doi
[40]

, B \'e trisey , J

barticle Buldgen , G. , B \'e trisey , J. , Roxburgh , I.W. , Vorontsov , S.V. , Reese , D.R. : 2022 , Inversions of Stellar Structure From Asteroseismic Data . Frontiers in Astronomy and Space Sciences 9 , 942373 . https://doi.org/10.3389/fspas.2022.942373 . 2022FrASS...9.237...

2022
[41]

, Noels , A

barticle Buldgen , G. , Noels , A. , Baturin , V.A. , Oreshina , A.V. , Ayukov , S.V. , Scuflaire , R. , Amarsi , A.M. , Grevesse , N. : 2024 a, Helioseismic determination of the solar metal mass fraction . 681 , A57 . https://doi.org/10.1051/0004-6361/202346928 . 2024A&A...68...

2024 doi
[42]

, Fellay , L

barticle Buldgen , G. , Fellay , L. , B \'e trisey , J. , Deheuvels , S. , Farnir , M. , Farrell , E. : 2024 b, Markov chain Monte Carlo inversions of the internal rotation of Kepler subgiants . 689 , A307 . https://doi.org/10.1051/0004-6361/202450315 . 2024A&A...689A.307B . barticle

2024 doi
[43]

, Jurewicz , A.J.G

barticle Burnett , D.S. , Jurewicz , A.J.G. , Woolum , D.S. : 2019 , The future of Genesis science . Meteorit. Planet. Sci. 54 , 1092 . https://doi.org/10.1111/maps.13266 . 2019M&PS...54.1092B . barticle

2019 doi
[44]

, Ludwig , H.-G

barticle Caffau , E. , Ludwig , H.-G. , Steffen , M. , Freytag , B. , Bonifacio , P. : 2011 , Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere . 268 , 255 . https://doi.org/10.1007/s11207-010-9541-4 . 2011SoPh..268..255C . barticle

2011 doi
[45]

, Ludwig , H.-G

barticle Caffau , E. , Ludwig , H.-G. , Malherbe , J.-M. , Bonifacio , P. , Steffen , M. , Monaco , L. : 2013 , The photospheric solar oxygen project. II. Non-concordance of the oxygen abundance derived from two forbidden lines . 554 , A126 . https://doi.org/10.1051/0004-6361/...

2013 doi
[46]

, Grumer , J

barticle Caliskan , S. , Grumer , J. , Amarsi , A.M. : 2024 , Targeted optimization in small-scale atomic structure calculations: application to Au I . Journal of Physics B Atomic Molecular Physics 57 , 055003 . https://doi.org/10.1088/1361-6455/ad2b71 . 2024JPhB...57e5003C . barticle

2024 doi
[47]

, Lind , K

barticle Canocchi , G. , Lind , K. , Lagae , C. , Pietrow , A.G.M. , Amarsi , A.M. , Kiselman , D. , Andriienko , O. , Hoeijmakers , H.J. : 2024 , 3D non-LTE modeling of the stellar center-to-limb variation for transmission spectroscopy studies. Na I D and K I resonance lines ...

2024 doi
[48]

, Mankovich , C

barticle Cantiello , M. , Mankovich , C. , Bildsten , L. , Christensen-Dalsgaard , J. , Paxton , B. : 2014 , Angular Momentum Transport within Evolved Low-mass Stars . 788 , 93 . https://doi.org/10.1088/0004-637X/788/1/93 . 2014ApJ...788...93C . barticle

2014 doi
[49]

, Miglio , A

barticle Chaplin , W.J. , Miglio , A. : 2013 , Asteroseismology of Solar-Type and Red-Giant Stars . 51 , 353 . https://doi.org/10.1146/annurev-astro-082812-140938 . 2013ARA&A..51..353C . barticle

2013 doi
[50]

, Elsworth , Y

barticle Chaplin , W.J. , Elsworth , Y. , Howe , R. , Isaak , G.R. , McLeod , C.P. , Miller , B.A. , van der Raay , H.B. , Wheeler , S.J. , New , R. : 1996 , BiSON Performance . 168 , 1 . https://doi.org/10.1007/BF00145821 . 1996SoPh..168....1C . barticle

1996 doi
[51]

, Talon , S

barticle Charbonnel , C. , Talon , S. : 2005 , Influence of Gravity Waves on the Internal Rotation and Li Abundance of Solar-Type Stars . Science 309 , 2189 . https://doi.org/10.1126/science.1116849 . 2005Sci...309.2189C . barticle

2005 doi
[52]

: 2009 , On the opacity change required to compensate for the revised solar composition

barticle Christensen-Dalsgaard , J. : 2009 , On the opacity change required to compensate for the revised solar composition . A&A 494 , 205 . barticle

2009
[53]

: 2021 , Solar structure and evolution

barticle Christensen-Dalsgaard , J. : 2021 , Solar structure and evolution . Living Reviews in Solar Physics 18 , 2 . https://doi.org/10.1007/s41116-020-00028-3 . 2021LRSP...18....2C . barticle

2021 doi
[54]

, Daeppen , W

barticle Christensen-Dalsgaard , J. , Daeppen , W. : 1992 , Solar oscillations and the equation of state . 4 , 267 . https://doi.org/10.1007/BF00872687 . 1992A&ARv...4..267C . barticle

1992 doi
[55]

, Proffitt , C.R

barticle Christensen-Dalsgaard , J. , Proffitt , C.R. , Thompson , M.J. : 1993 , Effects of Diffusion on Solar Models and Their Oscillation Frequencies . 403 , L75 . https://doi.org/10.1086/186725 . 1993ApJ...403L..75C . barticle

1993 doi
[56]

, Schou , J

barticle Christensen-Dalsgaard , J. , Schou , J. , Thompson , M.J. : 1990 , A comparison of methods for inverting helioseismic data . 242 , 353 . https://doi.org/10.1093/mnras/242.3.353 . 1990MNRAS.242..353C . barticle

1990 doi
[57]

, Dappen , W

barticle Christensen-Dalsgaard , J. , Dappen , W. , Ajukov , S.V. , Anderson , E.R. , Antia , H.M. , Basu , S. , Baturin , V.A. , Berthomieu , G. , Chaboyer , B. , Chitre , S.M. , Cox , A.N. , Demarque , P. , Donatowicz , J. , Dziembowski , W.A. , Gabriel , M. , Gough , D.O. ,...

1996
[58]

, Monteiro , M.J.P.F.G

barticle Christensen-Dalsgaard , J. , Monteiro , M.J.P.F.G. , Rempel , M. , Thompson , M.J. : 2011 , A more realistic representation of overshoot at the base of the solar convective envelope as seen by helioseismology . 414 , 1158 . https://doi.org/10.1111/j.1365-2966.2011.184...

2011
[59]

, Kilcrease , D.P

barticle Colgan , J. , Kilcrease , D.P. , Magee , N.H. , Sherrill , M.E. , Abdallah , J. Jr. , Hakel , P. , Fontes , C.J. , Guzik , J.A. , Mussack , K.A. : 2016 , A New Generation of Los Alamos Opacity Tables . ApJ 817 , 116 . barticle

2016
[60]

, Blanc-F \'e raud , L

barticle Corbard , T. , Blanc-F \'e raud , L. , Berthomieu , G. , Provost , J. : 1999 , Non linear regularization for helioseismic inversions. Application for the study of the solar tachocline . 344 , 696 . https://doi.org/10.48550/arXiv.astro-ph/9901112 . 1999A&A...344..696C ...

1999 doi arXiv
[61]

: 2017 , Mass-loss Rates from Coronal Mass Ejections: A Predictive Theoretical Model for Solar-type Stars

barticle Cranmer , S.R. : 2017 , Mass-loss Rates from Coronal Mass Ejections: A Predictive Theoretical Model for Solar-type Stars . 840 , 114 . https://doi.org/10.3847/1538-4357/aa6f0e . 2017ApJ...840..114C . barticle

2017 doi
[62]

, Saar , S.H

barticle Cranmer , S.R. , Saar , S.H. : 2011 , Testing a Predictive Theoretical Model for the Mass Loss Rates of Cool Stars . 741 , 54 . https://doi.org/10.1088/0004-637X/741/1/54 . 2011ApJ...741...54C . barticle

2011 doi
[63]

, Aerts , C

barticle Cunha , M.S. , Aerts , C. , Christensen-Dalsgaard , J. , Baglin , A. , Bigot , L. , Brown , T.M. , Catala , C. , Creevey , O.L. , Domiciano de Souza , A. , Eggenberger , P. , Garcia , P.J.V. , Grundahl , F. , Kervella , P. , Kurtz , D.W. , Mathias , P. , Miglio , A. ,...

2007
[64]

, MacGowan , B.J

barticle Da Silva , L.B. , MacGowan , B.J. , Kania , D.R. , Hammel , B.A. , Back , C.A. , Hsieh , E. , Doyas , R. , Iglesias , C.A. , Rogers , F.J. , Lee , R.W. : 1992 , Absorption measurements demonstrating the importance of n=0 transitions in the opacity of iron . Phys. Rev....

1992 doi
[65]

, Do g an , G

barticle Deheuvels , S. , Do g an , G. , Goupil , M.J. , Appourchaux , T. , Benomar , O. , Bruntt , H. , Campante , T.L. , Casagrande , L. , Ceillier , T. , Davies , G.R. , De Cat , P. , Fu , J.N. , Garc \' a , R.A. , Lobel , A. , Mosser , B. , Reese , D.R. , Regulo , C. , Sch...

2014
[66]

, Ballot , J

barticle Deheuvels , S. , Ballot , J. , Eggenberger , P. , Spada , F. , Noll , A. , den Hartogh , J.W. : 2020 , Seismic evidence for near solid-body rotation in two Kepler subgiants and implications for angular momentum transport . 641 , A117 . https://doi.org/10.1051/0004-636...

2020 doi
[67]

, Roland , G

bbook Delbouille , L. , Roland , G. , Neven , L. : 1973 , Atlas photometrique du spectre solaire de [lambda] 3000 a [lambda] 10000 . 1973apds.book.....D . bbook

1973
[68]

, Chakraborty , H.S

barticle Dias , E.W.B. , Chakraborty , H.S. , Deshmukh , P.C. , Manson , S.T. , Hemmers , O. , Glans , P. , Hansen , D.L. , Wang , H. , Whitfield , S.B. , Lindle , D.W. , Wehlitz , R. , Levin , J.C. , Sellin , I.A. , Perera , R.C.C. : 1997 , Breakdown of the Independent Partic...

1997 doi
[69]

, Bitsch , B

bchapter Dr a \.z kowska , J. , Bitsch , B. , Lambrechts , M. , Mulders , G.D. , Harsono , D. , Vazan , A. , Liu , B. , Ormel , C.W. , Kretke , K. , Morbidelli , A. : 2023 , Planet Formation Theory in the Era of ALMA and Kepler: from Pebbles to Exoplanets . In: Inutsuka , S. ,...

2023 doi arXiv
[70]

, Buldgen , G

barticle Eggenberger , P. , Buldgen , G. , Salmon , S.J.A.J. , Noels , A. , Grevesse , N. , Asplund , M. : 2022 , The internal rotation of the Sun and its link to the solar Li and He surface abundances . Nature Astronomy 6 , 788 . https://doi.org/10.1038/s41550-022-01677-0 . 2...

2022 doi
[71]

: 1996 , Equation of state in the solar convection zone and the implications of helioseismology

barticle Elliott , J.R. : 1996 , Equation of state in the solar convection zone and the implications of helioseismology . 280 , 1244 . https://doi.org/10.1093/mnras/280.4.1244 . 1996MNRAS.280.1244E . barticle

1996 doi
[72]

, Kosovichev , A.G

barticle Elliott , J.R. , Kosovichev , A.G. : 1998 , The Adiabatic Exponent in the Solar Core . 500 , L199 . https://doi.org/10.1086/311417 . 1998ApJ...500L.199E . barticle

1998 doi
[73]

, Ehmann , B

barticle Ellwarth , M. , Ehmann , B. , Sch \"a fer , S. , Reiners , A. : 2023 , Convective characteristics of Fe I lines across the solar disc . 680 , A62 . https://doi.org/10.1051/0004-6361/202347615 . 2023A&A...680A..62E . barticle

2023 doi
[74]

, Khomenko , E

barticle Fabbian , D. , Khomenko , E. , Moreno-Insertis , F. , Nordlund , . : 2010 , Solar Abundance Corrections Derived Through Three-dimensional Magnetoconvection Simulations . ApJ 724 , 1536 . barticle

2010
[75]

, Buldgen , G

barticle Fellay , L. , Buldgen , G. , Eggenberger , P. , Khan , S. , Salmon , S.J.A.J. , Miglio , A. , Montalb \'a n , J. : 2021 , Asteroseismology of evolved stars to constrain the internal transport of angular momentum. IV. Internal rotation of Kepler-56 from an MCMC analysi...

2021 doi
[76]

: 1991 , The IRIS Network for Full Disk Helioseismology - Present Status of the Programme

barticle Fossat , E. : 1991 , The IRIS Network for Full Disk Helioseismology - Present Status of the Programme . 133 , 1 . https://doi.org/10.1007/BF00149818 . 1991SoPh..133....1F . barticle

1991 doi
[77]

, Boumier , P

barticle Fossat , E. , Boumier , P. , Corbard , T. , Provost , J. , Salabert , D. , Schmider , F.X. , Gabriel , A.H. , Grec , G. , Renaud , C. , Robillot , J.M. , Roca-Cort \'e s , T. , Turck-Chi \`e ze , S. , Ulrich , R.K. , Lazrek , M. : 2017 , Asymptotic g modes: Evidence f...

2017 doi
[78]

, Ludwig , H.-G

barticle Freytag , B. , Ludwig , H.-G. , Steffen , M. : 1996 , Hydrodynamical models of stellar convection. The role of overshoot in DA white dwarfs, A-type stars, and the Sun. 313 , 497 . 1996A&A...313..497F . barticle

1996
[79]

, Steffen , M

barticle Freytag , B. , Steffen , M. , Ludwig , H.-G. , Wedemeyer-B \"o hm , S. , Schaffenberger , W. , Steiner , O. : 2012 , Simulations of stellar convection with CO5BOLD . Journal of Computational Physics 231 , 919 . https://doi.org/10.1016/j.jcp.2011.09.026 . 2012JCoPh.231...

2012 doi
[80]

, Romero , J

barticle Fr \"o hlich , C. , Romero , J. , Roth , H. , Wehrli , C. , Andersen , B.N. , Appourchaux , T. , Domingo , V. , Telljohann , U. , Berthomieu , G. , Delache , P. , Provost , J. , Toutain , T. , Crommelynck , D.A. , Chevalier , A. , Fichot , A. , D \"a ppen , W. , Gough...

1995
[81]

, Piro , A.L

barticle Fuller , J. , Piro , A.L. , Jermyn , A.S. : 2019 , Slowing the spins of stellar cores . 485 , 3661 . https://doi.org/10.1093/mnras/stz514 . 2019MNRAS.485.3661F . barticle

2019 doi
[82]

, Charra , J

barticle Gabriel , A.H. , Charra , J. , Grec , G. , Robillot , J.-M. , Roca Cort \'e s , T. , Turck-Chi \`e ze , S. , Ulrich , R. , Basu , S. , Baudin , F. , Bertello , L. , Boumier , P. , Charra , M. , Christensen-Dalsgaard , J. , Decaudin , M. , Dzitko , H. , Foglizzo , T. ,...

1997
[83]

, Zanni , C

barticle Gallet , F. , Zanni , C. , Amard , L. : 2019 , Rotational evolution of solar-type protostars during the star-disk interaction phase . 632 , A6 . https://doi.org/10.1051/0004-6361/201935432 . 2019A&A...632A...6G . barticle

2019 doi
[84]

, Nordlund , A

botherref Galsgaard , K. , Nordlund , A. : 1995, A 3D MHD Code for Parallel Computers, preparation. botherref

1995
[85]

, Ballot , J

barticle Garc \' a , R.A. , Ballot , J. : 2019 , Asteroseismology of solar-type stars . Living Reviews in Solar Physics 16 , 4 . https://doi.org/10.1007/s41116-019-0020-1 . 2019LRSP...16....4G . barticle

2019 doi
[86]

, Turck-Chi \`e ze , S

barticle Garc \' a , R.A. , Turck-Chi \`e ze , S. , Jim \'e nez-Reyes , S.J. , Ballot , J. , Pall \'e , P.L. , Eff-Darwich , A. , Mathur , S. , Provost , J. : 2007 , Tracking Solar Gravity Modes: The Dynamics of the Solar Core . Science 316 , 1591 . https://doi.org/10.1126/sci...

2007 doi
[87]

, McIntyre , M.E

barticle Gough , D.O. , McIntyre , M.E. : 1998 , Inevitability of a magnetic field in the Sun's radiative interior . 394 , 755 . https://doi.org/10.1038/29472 . 1998Natur.394..755G . barticle

1998 doi
[88]

, Catala , C

barticle Goupil , M.J. , Catala , C. , Samadi , R. , Belkacem , K. , Ouazzani , R.M. , Reese , D.R. , Appourchaux , T. , Mathur , S. , Cabrera , J. , B \"o rner , A. , Paproth , C. , Moedas , N. , Verma , K. , Lebreton , Y. , Deal , M. , Ballot , J. , Chaplin , W.J. , Christen...

2024
[89]

, Harwood , D.J

barticle Graboske , H.C. , Harwood , D.J. , Rogers , F.J. : 1969 , Thermodynamic Properties of Nonideal gases. I. F ree-Energy Minimization Method . Physical Review 186 , 210 . http://cdsads.u-strasbg.fr/abs/1969PhRv..186..210G . barticle

1969
[90]

, Eklund , G

barticle Grumer , J. , Eklund , G. , Amarsi , A.M. , Barklem , P.S. , Ros \'e n , S. , Ji , M. , Simonsson , A. , Cederquist , H. , Zettergren , H. , Schmidt , H.T. : 2022 , State-Resolved Mutual Neutralization of Mg ^ + and D ^ - . 128 , 033401 . https://doi.org/10.1103/PhysR...

2022 doi
[91]

, Ayukov , S.V

bchapter Gryaznov , V.K. , Ayukov , S.V. , Baturin , V.A. , Iosilevskiy , I.L. , Starostin , A.N. , Fortov , V.E. : 2004 , SAHA-S model: Equation of State and Thermodynamic Functions of Solar Plasma . In: Celebonovic , V. , Gough , D. , D \"a ppen , W. (eds.) Equation-of-State...

2004 doi
[92]

, Ayukov , S.V

barticle Gryaznov , V.K. , Ayukov , S.V. , Baturin , V.A. , Iosilevskiy , I.L. , Starostin , A.N. , Fortov , V.E. : 2006 , Solar plasma: calculation of thermodynamic functions and equation of state . Journal of Physics A Mathematical General 39 , 4459 . https://doi.org/10.1088...

2006 doi
[93]

, Hueso , R

barticle Guillot , T. , Hueso , R. : 2006 , The composition of Jupiter: sign of a (relatively) late formation in a chemically evolved protosolar disc . 367 , L47 . https://doi.org/10.1111/j.1745-3933.2006.00137.x . https://doi.org/10.1111/j.1745-3933.2006.00137.x . barticle

2006
[94]

, Ida , S

barticle Guillot , T. , Ida , S. , Ormel , C.W. : 2014 , On the filtering and processing of dust by planetesimals. I. Derivation of collision probabilities for non-drifting planetesimals . 572 , A72 . https://doi.org/10.1051/0004-6361/201323021 . 2014A\ barticle

2014 doi
[95]

, Mussack , K

barticle Guzik , J.A. , Mussack , K. : 2010 , Exploring Mass Loss, Low-Z Accretion, and Convective Overshoot in Solar Models to Mitigate the Solar Abundance Problem . 713 , 1108 . https://doi.org/10.1088/0004-637X/713/2/1108 . 2010ApJ...713.1108G . barticle

2010 doi
[96]

, Kilcrease , D.P

bchapter Hakel , P. , Kilcrease , D.P. : 2004 , CHEMEOS: A New Chemical-Picture-Based Model for Plasma Equation-of-State Calculations . In: AIP Conference Proceedings 730 , 190 . American Institute of Physics . bchapter

2004
[97]

, Howe , R

barticle Hale , S.J. , Howe , R. , Chaplin , W.J. , Davies , G.R. , Elsworth , Y.P. : 2016 , Performance of the Birmingham Solar-Oscillations Network (BiSON) . 291 , 1 . https://doi.org/10.1007/s11207-015-0810-0 . 2016SoPh..291....1H . barticle

2016 doi
[98]

, More , R

bchapter Hansen , S.B. , More , R. , Bailey , J. , Pain , J.-C. , Nagayama , T. : 2020 , Two-photon absorption in plasmas. In: APS Division of Plasma Physics Meeting Abstracts , APS Meeting Abstracts 2020 , GO08.010 . 2020APS..DPPG08010H . bchapter

2020
[99]

, Hill , F

barticle Harvey , J.W. , Hill , F. , Hubbard , R.P. , Kennedy , J.R. , Leibacher , J.W. , Pintar , J.A. , Gilman , P.A. , Noyes , R.W. , Title , A.M. , Toomre , J. , Ulrich , R.K. , Bhatnagar , A. , Kennewell , J.A. , Marquette , W. , Patron , J. , Saa , O. , Yasukawa , E. : 1...

1996
[100]

, Wieler , R

barticle Heber , V.S. , Wieler , R. , Baur , H. , Olinger , C. , Friedmann , T.A. , Burnett , D.S. : 2009 , Noble gas composition of the solar wind as collected by the Genesis mission . Geochim. Cosmochim. Acta 73 , 7414 . https://doi.org/10.1016/j.gca.2009.09.013 . 2009GeCoA....

2009 doi
[101]

, Lambert , D.L

barticle Hinkle , K.H. , Lambert , D.L. : 1975 , Formation of molecular lines in stellar atmospheres. 170 , 447 . https://doi.org/10.1093/mnras/170.3.447 . 1975MNRAS.170..447H . barticle

1975 doi
[102]

, Morton , J

barticle Hoarty , D.J. , Morton , J. , Rougier , J.C. , Rubery , M. , Opachich , Y.P. , Swatton , D. , Richardson , S. , Heeter , R.F. , McLean , K. , Rose , S.J. , Perry , T.S. , Remington , B. : 2023 , Radiation burnthrough measurements to infer opacity at conditions close t...

2023 doi
[103]

, Baldner , C.S

barticle Hoeksema , J.T. , Baldner , C.S. , Bush , R.I. , Schou , J. , Scherrer , P.H. : 2018 , On-Orbit Performance of the Helioseismic and Magnetic Imager Instrument onboard the Solar Dynamics Observatory . 293 , 45 . https://doi.org/10.1007/s11207-018-1259-8 . 2018SoPh..293...

2018 doi
[104]

, Kusano , K

barticle Hotta , H. , Kusano , K. , Shimada , R. : 2022 , Generation of Solar-like Differential Rotation . 933 , 199 . https://doi.org/10.3847/1538-4357/ac7395 . 2022ApJ...933..199H . barticle

2022 doi
[105]

, Bekki , Y

barticle Hotta , H. , Bekki , Y. , Gizon , L. , Noraz , Q. , Rast , M. : 2023 , Dynamics of Large-Scale Solar Flows . 219 , 77 . https://doi.org/10.1007/s11214-023-01021-6 . 2023SSRv..219...77H . barticle

2023 doi
[106]

, Trampedach , R

barticle Houdek , G. , Trampedach , R. , Aarslev , M.J. , Christensen-Dalsgaard , J. : 2017 , On the surface physics affecting solar oscillation frequencies . 464 , L124 . https://doi.org/10.1093/mnrasl/slw193 . 2017MNRAS.464L.124H . barticle

2017 doi
[107]

, Chaplin , W.J

barticle Howe , R. , Chaplin , W.J. , Basu , S. , Ball , W.H. , Davies , G.R. , Elsworth , Y. , Hale , S.J. , Miglio , A. , Nielsen , M.B. , Viani , L.S. : 2020 , Solar cycle variation of _ max in helioseismic data and its implications for asteroseismology . 493 , L49 . https:...

2020 doi
[108]

, Mihalas , D

barticle Hummer , D.G. , Mihalas , D. : 1988 , The equation of state for stellar envelopes. I . A n occupation probability formalism for the truncation of internal partitition functions . ApJ 331 , 794 . http://cdsads.u-strasbg.fr/abs/1988ApJ...331..794H . barticle

1988
[109]

, Rogers , F.J

barticle Iglesias , C.A. , Rogers , F.J. : 1996 , Updated Opal Opacities . ApJ 464 , 943 . barticle

1996
[110]

: 2012 , Present-day star formation: From molecular cloud cores to protostars and protoplanetary disks

barticle Inutsuka , S.-i. : 2012 , Present-day star formation: From molecular cloud cores to protostars and protoplanetary disks . Progress of Theoretical and Experimental Physics 2012 , 01A307 . https://doi.org/10.1093/ptep/pts024 . 2012PTEP.2012aA307I . barticle

2012 doi
[111]

: 2012, FreeEOS: Equation of State for stellar interiors calculations , Astrophysics Source Code Library

botherref Irwin , A.W. : 2012, FreeEOS: Equation of State for stellar interiors calculations , Astrophysics Source Code Library. botherref

2012
[112]

, Andrassy , R

barticle Jones , S. , Andrassy , R. , Sandalski , S. , Davis , A. , Woodward , P. , Herwig , F. : 2017 , Idealized hydrodynamic simulations of turbulent oxygen-burning shell convection in 4 geometry . 465 , 2991 . https://doi.org/10.1093/mnras/stw2783 . 2017MNRAS.465.2991J . barticle

2017 doi
[113]

, Mosumgaard , J.R

barticle J rgensen , A.C.S. , Mosumgaard , J.R. , Weiss , A. , Silva Aguirre , V. , Christensen-Dalsgaard , J. : 2018 , Coupling 1D stellar evolution with 3D-hydrodynamical simulations on the fly - I. A new standard solar model . 481 , L35 . https://doi.org/10.1093/mnrasl/sly1...

2018 doi
[114]

, Colgan , J

barticle Kilcrease , D.P. , Colgan , J. , Hakel , P. , Fontes , C.J. , Sherrill , M.E. : 2015 , An equation of state for partially ionized plasmas: The Coulomb contribution to the free energy . High Energy Density Phys. 16 , 36 . http://www.sciencedirect.com/science/article/pi...

2015
[115]

, Garaud , P

barticle Korre , L. , Garaud , P. , Brummell , N.H. : 2019 , Convective overshooting and penetration in a Boussinesq spherical shell . 484 , 1220 . https://doi.org/10.1093/mnras/stz047 . 2019MNRAS.484.1220K . barticle

2019 doi
[116]

: 2005 , A Mode-Fitting Methodology Optimized for Very Long Helioseismic Time Series

barticle Korzennik , S.G. : 2005 , A Mode-Fitting Methodology Optimized for Very Long Helioseismic Time Series . 626 , 585 . https://doi.org/10.1086/429748 . 2005ApJ...626..585K . barticle

2005 doi
[117]

: 2008 a, YAOPBM - yet another peak bagging method

barticle Korzennik , S.G. : 2008 a, YAOPBM - yet another peak bagging method . Astronomische Nachrichten 329 , 453 . https://doi.org/10.1002/asna.200710979 . 2008AN....329..453K . barticle

2008 doi
[118]

: 2008 b, YAOPBM II: extension to higher degrees and to shorter time series

bchapter Korzennik , S.G. : 2008 b, YAOPBM II: extension to higher degrees and to shorter time series . In: Journal of Physics Conference Series , Journal of Physics Conference Series 118 , 012082 . https://doi.org/10.1088/1742-6596/118/1/012082 . 2008JPhCS.118a2082K . bchapter

2008 doi
[119]

: 1999 , Inversion methods in helioseismology and solar tomography

barticle Kosovichev , A.G. : 1999 , Inversion methods in helioseismology and solar tomography. Journal of Computational and Applied Mathematics 109 , 1 . 1999JCoAM.109....1K . barticle

1999
[120]

, Shapiro , A.I

barticle Kostogryz , N.M. , Shapiro , A.I. , Witzke , V. , Cameron , R.H. , Gizon , L. , Krivova , N.A. , Ludwig , H.-G. , Maxted , P.F.L. , Seager , S. , Solanki , S.K. , Valenti , J. : 2024 , Magnetic origin of the discrepancy between stellar limb-darkening models and observ...

2024 doi
[121]

, Kleine , T

barticle Kruijer , T.S. , Kleine , T. , Borg , L.E. : 2020 , The great isotopic dichotomy of the early Solar System . Nature Astronomy 4 , 32 . https://doi.org/10.1038/s41550-019-0959-9 . 2020NatAs...4...32K . barticle

2020 doi
[122]

, Iglesias , C.A

barticle Kruse , M.K.G. , Iglesias , C.A. : 2019 , Two-photon absorption framework for plasma transmission experiments . High Energy Density Physics 31 , 38 . https://doi.org/10.1016/j.hedp.2019.02.004 . https://www.sciencedirect.com/science/article/pii/S1574181818300600 . barticle

2019 doi
[123]

, Iglesias , C.A

barticle Kruse , M.K.G. , Iglesias , C.A. : 2021 , Two-photon ionization in solar opacity experiments . High Energy Density Physics 41 , 100976 . https://doi.org/10.1016/j.hedp.2022.100976 . https://www.sciencedirect.com/science/article/pii/S1574181822000027 . barticle

2021
[124]

, Guillot , T

barticle Kunitomo , M. , Guillot , T. : 2021 , Imprint of planet formation in the deep interior of the Sun . 655 , A51 . https://doi.org/10.1051/0004-6361/202141256 . 2021A&A...655A..51K . barticle

2021 doi
[125]

, Guillot , T

barticle Kunitomo , M. , Guillot , T. , Buldgen , G. : 2022 , Evidence of a signature of planet formation processes from solar neutrino fluxes . 667 , L2 . https://doi.org/10.1051/0004-6361/202244169 . 2022A&A...667L...2K . barticle

2022 doi
[126]

, Suzuki , T.K

barticle Kunitomo , M. , Suzuki , T.K. , Inutsuka , S.-i. : 2020 , Dispersal of protoplanetary discs by the combination of magnetically driven and photoevaporative winds . 492 , 3849 . https://doi.org/10.1093/mnras/staa087 . 2020MNRAS.492.3849K . barticle

2020 doi
[127]

, Guillot , T

barticle Kunitomo , M. , Guillot , T. , Takeuchi , T. , Ida , S. : 2017 , Revisiting the pre-main-sequence evolution of stars. I. Importance of accretion efficiency and deuterium abundance . 599 , A49 . https://doi.org/10.1051/0004-6361/201628260 . 2017A\ barticle

2017 doi
[128]

, Muthsam , H.J

barticle Kupka , F. , Muthsam , H.J. : 2017 , Modelling of stellar convection . Living Reviews in Computational Astrophysics 3 , 1 . https://doi.org/10.1007/s41115-017-0001-9 . 2017LRCA....3....1K . barticle

2017 doi
[129]

: 2005 , New atlases for solar flux, irradiance, central intensity, and limb intensity

barticle Kurucz , R.L. : 2005 , New atlases for solar flux, irradiance, central intensity, and limb intensity . Memorie della Societa Astronomica Italiana Supplementi 8 , 189 . 2005MSAIS...8..189K . barticle

2005
[130]

, Furenlid , I

bbook Kurucz , R.L. , Furenlid , I. , Brault , J. , Testerman , L. : 1984 , Solar flux atlas from 296 to 1300 nm . 1984sfat.book.....K . bbook

1984
[131]

: 2015 , The FIP and Inverse FIP Effects in Solar and Stellar Coronae

barticle Laming , J.M. : 2015 , The FIP and Inverse FIP Effects in Solar and Stellar Coronae . Living Reviews in Solar Physics 12 , 2 . https://doi.org/10.1007/lrsp-2015-2 . 2015LRSP...12....2L . barticle

2015 doi
[132]

, Testa , P

barticle Landi , E. , Testa , P. : 2015 , Neon and Oxygen Abundances and Abundance Ratio in the Solar Corona . 800 , 110 . https://doi.org/10.1088/0004-637X/800/2/110 . 2015ApJ...800..110L . barticle

2015 doi
[133]

: 1969 , Numerical calculations of the dynamics of collapsing proto-star

barticle Larson , R.B. : 1969 , Numerical calculations of the dynamics of collapsing proto-star . 145 , 271 . http://ads.nao.ac.jp/abs/1969MNRAS.145..271L . barticle

1969
[134]

, Schou , J

barticle Larson , T.P. , Schou , J. : 2015 , Improved Helioseismic Analysis of Medium- Data from the Michelson Doppler Imager . 290 , 3221 . https://doi.org/10.1007/s11207-015-0792-y . 2015SoPh..290.3221L . barticle

2015 doi
[135]

, Guillet , T

barticle Le Saux , A. , Guillet , T. , Baraffe , I. , Vlaykov , D.G. , Constantino , T. , Pratt , J. , Goffrey , T. , Sylvain , M. , R \'e ville , V. , Brun , A.S. : 2022 , Two-dimensional simulations of solar-like models with artificially enhanced luminosity. II. Impact on in...

2022 doi
[136]

, Schwab , J

barticle Lecoanet , D. , Schwab , J. , Quataert , E. , Bildsten , L. , Timmes , F.X. , Burns , K.J. , Vasil , G.M. , Oishi , J.S. , Brown , B.P. : 2016 , Turbulent Chemical Diffusion in Convectively Bounded Carbon Flames . 832 , 71 . https://doi.org/10.3847/0004-637X/832/1/71 ...

2016 doi
[137]

, Gordon , I.E

barticle Li , G. , Gordon , I.E. , Rothman , L.S. , Tan , Y. , Hu , S.-M. , Kassi , S. , Campargue , A. , Medvedev , E.S. : 2015 , Rovibrational Line Lists for Nine Isotopologues of the CO Molecule in the X ^ 1 ^ + Ground Electronic State . ApJS 216 , 15 . https://doi.org/10.1...

2015 doi
[138]

, J \"o nsson , P

barticle Li , W. , J \"o nsson , P. , Amarsi , A.M. , Li , M.C. , Grumer , J. : 2023 , Extended atomic data for oxygen abundance analyses . 674 , A54 . https://doi.org/10.1051/0004-6361/202245645 . 2023A&A...674A..54L . barticle

2023 doi
[139]

: 1969 , Interaction of Atoms with Electrons and Ions in a Plasma

barticle Likalter , A.A. : 1969 , Interaction of Atoms with Electrons and Ions in a Plasma . JETP 29 , 133 . barticle

1969
[140]

, Amarsi , A.M

botherref Lind , K. , Amarsi , A.M. : 2024, 3D non-LTE abundance analyses of late-type stars . arXiv e-prints, arXiv:2401.00697. https://doi.org/10.48550/arXiv.2401.00697 . 2024arXiv240100697L . botherref

2024 doi arXiv
[141]

, Ku c inskas , A

barticle Ludwig , H.-G. , Ku c inskas , A. : 2012 , Three-dimensional hydrodynamical CO ^ 5 BOLD model atmospheres of red giant stars. I. Atmospheric structure of a giant located near the RGB tip . 547 , A118 . https://doi.org/10.1051/0004-6361/201220264 . 2012A&A...547A.118L ...

2012 doi
[142]

, Steffen , M

barticle Ludwig , H.-G. , Steffen , M. , Freytag , B. : 2023 , Effects of magnetic fields on the center-to-limb variation in solar-type stars . 679 , A65 . https://doi.org/10.1051/0004-6361/202346783 . 2023A&A...679A..65L . barticle

2023 doi
[143]

, Li , Y

barticle Ma , M. , Li , Y. , Godefroid , M. , Gaigalas , G. , Li , J. , Bieroń , J. , Chen , C. , Wang , J. , Jönsson , P. : 2024 , Natural Orbitals and Targeted Non-Orthogonal Orbital Sets for Atomic Hyperfine Structure Multiconfiguration Calculations . Atoms 12 . https://doi...

2024 doi
[144]

, Bergemann , M

barticle Magg , E. , Bergemann , M. , Serenelli , A. , Bautista , M. , Plez , B. , Heiter , U. , Gerber , J.M. , Ludwig , H.-G. , Basu , S. , Ferguson , J.W. , Gallego , H.C. , Gamrath , S. , Palmeri , P. , Quinet , P. : 2022 , Observational constraints on the origin of the el...

2022 doi
[145]

, Collet , R

barticle Magic , Z. , Collet , R. , Asplund , M. , Trampedach , R. , Hayek , W. , Chiavassa , A. , Stein , R.F. , Nordlund , A . : 2013 , The Stagger-grid: A grid of 3D stellar atmosphere models. I. Methods and general properties . 557 , A26 . https://doi.org/10.1051/0004-6361...

2013 doi
[146]

, Deal , M

barticle Manchon , L. , Deal , M. , Goupil , M.-J. , Serenelli , A. , Lebreton , Y. , Klevas , J. , Ku c inskas , A. , Ludwig , H.-G. , Montalb \'a n , J. , Gizon , L. : 2024 , Entropy-calibrated stellar modeling: Testing and improving the use of prescriptions for the entropy ...

2024 doi
[147]

, Hobbs , B.A

barticle Mayes , D.C. , Hobbs , B.A. , Heeter , R.F. , Perry , T.S. , Johns , H.M. , Opachich , Y.P. , Hohenberger , M. , Bradley , P.A. , Dutra , E.C. , Fontes , C.J. , Gallardo-Diaz , E. , Montgomery , M.H. , Robey , H.F. , Wallace , M.S. , Winget , D.E. : 2025 , Overview of...

2025
[148]

: 2016 , Nobel Lecture: The Sudbury Neutrino Observatory: Observation of flavor change for solar neutrinos*

barticle McDonald , A.B. : 2016 , Nobel Lecture: The Sudbury Neutrino Observatory: Observation of flavor change for solar neutrinos* . Reviews of Modern Physics 88 , 030502 . https://doi.org/10.1103/RevModPhys.88.030502 . 2016RvMP...88c0502M . barticle

2016 doi
[149]

, Dappen , W

barticle Mihalas , D. , Dappen , W. , Hummer , D.G. : 1988 , The Equation of State for Stellar Envelopes. II. Algorithm and Selected Results . 331 , 815 . https://doi.org/10.1086/166601 . 1988ApJ...331..815M . barticle

1988 doi
[150]

, Blancard , C

barticle Mondet , G. , Blancard , C. , Coss \'e , P. , Faussurier , G. : 2015 , Opacity Calculations for Solar Mixtures . ApJS 220 , 2 . barticle

2015
[151]

, Christensen-Dalsgaard , J

barticle Monteiro , M.J.P.F.G. , Christensen-Dalsgaard , J. , Thompson , M.J. : 1994 , Seismic study of overshoot at the base of the solar convective envelope . 283 , 247 . 1994A&A...283..247M . barticle

1994
[152]

, Hansen , S.B

barticle More , R.M. , Hansen , S.B. , Nagayama , T. : 2017 , Opacity from two-photon processes . High Energy Density Physics 24 , 44 . https://doi.org/10.1016/j.hedp.2017.07.003 . https://www.sciencedirect.com/science/article/pii/S1574181817300654 . barticle

2017 doi
[153]

, Pain , J.-C

barticle More , R. , Pain , J.-C. , Hansen , S.B. , Nagayama , T. , Bailey , J.E. : 2020 , Free-free matrix-elements for two-photon opacity . High Energy Density Physics 34 , 100717 . https://doi.org/10.1016/j.hedp.2019.100717 . https://www.sciencedirect.com/science/article/pi...

2020
[154]

, Ball , W.H

barticle Mosumgaard , J.R. , Ball , W.H. , Silva Aguirre , V. , Weiss , A. , Christensen-Dalsgaard , J. : 2018 , Stellar models with calibrated convection and temperature stratification from 3D hydrodynamics simulations . 478 , 5650 . https://doi.org/10.1093/mnras/sty1442 . 20...

2018 doi
[155]

, Bailey , J.E

barticle Nagayama , T. , Bailey , J.E. , Loisel , G.P. , Dunham , G.S. , Rochau , G.A. , Blancard , C. , Colgan , J. , Coss \'e , P. , Faussurier , G. , Fontes , C.J. , Gilleron , F. , Hansen , S.B. , Iglesias , C.A. , Golovkin , I.E. , Kilcrease , D.P. , MacFarlane , J.J. , M...

2019 doi
[156]

, Zhao , L

barticle Nahar , S.N. , Zhao , L. , Eissner , W. , Pradhan , A.K. : 2024 , R-Matrix calculations for opacities: II. Photoionization and oscillator strengths of iron ions Fe XVII, Fe XVIII and Fe XIX . Journal of Physics B Atomic Molecular Physics 57 , 125002 . https://doi.org/...

2024 doi
[157]

, Maehara , H

barticle Namekata , K. , Maehara , H. , Honda , S. , Notsu , Y. , Okamoto , S. , Takahashi , J. , Takayama , M. , Ohshima , T. , Saito , T. , Katoh , N. , Tozuka , M. , Murata , K.L. , Ogawa , F. , Niwano , M. , Adachi , R. , Oeda , M. , Shiraishi , K. , Isogai , K. , Seki , D...

2022 doi
[158]

, Labs , D

barticle Neckel , H. , Labs , D. : 1984 , The solar radiation between 3300 and 12500 A . 90 , 205 . https://doi.org/10.1007/BF00173953 . 1984SoPh...90..205N . barticle

1984 doi
[159]

: 2013 , ASTROD-GW: OVERVIEW AND PROGRESS

barticle Ni , W.-T. : 2013 , ASTROD-GW: OVERVIEW AND PROGRESS . International Journal of Modern Physics D 22 , 1341004 . https://doi.org/10.1142/S0218271813410046 . https://doi.org/10.1142/S0218271813410046 . barticle

2013 doi
[160]

: 2024 , Space gravitational wave detection: Progress and outlook

barticle Ni , W.-T. : 2024 , Space gravitational wave detection: Progress and outlook . Scientia Sinica Physica, Mechanica & Astronomica 54 , 270402 . https://doi.org/10.1360/SSPMA-2024-0186 . 2024SSPMA..54A0402N . barticle

2024 doi
[161]

, Vidotto , A.A

barticle \'O Fionnag \'a in , D. , Vidotto , A.A. : 2018 , The solar wind in time: a change in the behaviour of older winds? 476 , 2465 . https://doi.org/10.1093/mnras/sty394 . 2018MNRAS.476.2465O . barticle

2018 doi
[162]

, Zuber , K

barticle Orebi Gann , G.D. , Zuber , K. , Bemmerer , D. , Serenelli , A. : 2021 , The Future of Solar Neutrinos . Annual Review of Nuclear and Particle Science 71 , 491 . https://doi.org/10.1146/annurev-nucl-011921-061243 . 2021ARNPS..71..491O . barticle

2021 doi
[163]

: 2018 , A note on the contribution of multi-photon processes to radiative opacity

barticle Pain , J.-C. : 2018 , A note on the contribution of multi-photon processes to radiative opacity . High Energy Density Physics 26 , 23 . https://doi.org/10.1016/j.hedp.2017.11.004 . https://www.sciencedirect.com/science/article/pii/S1574181817300885 . barticle

2018 doi
[164]

, Asplund , M

barticle Pereira , T.M.D. , Asplund , M. , Collet , R. , Thaler , I. , Trampedach , R. , Leenaarts , J. : 2013 , How realistic are solar model atmospheres? 554 , A118 . https://doi.org/10.1051/0004-6361/201321227 . 2013A&A...554A.118P . barticle

2013 doi
[165]

, Marcotte , F

barticle Petitdemange , L. , Marcotte , F. , Gissinger , C. : 2023 , Spin-down by dynamo action in simulated radiative stellar layers . Science 379 , 300 . https://doi.org/10.1126/science.abk2169 . 2023Sci...379..300P . barticle

2023 doi
[166]

, Marcotte , F

barticle Petitdemange , L. , Marcotte , F. , Gissinger , C. , Daniel , F. : 2024 , Tayler-Spruit dynamo simulations for the modeling of radiative stellar layers . 681 , A75 . https://doi.org/10.1051/0004-6361/202347241 . 2024A&A...681A..75P . barticle

2024 doi
[167]

: 1962 , A Technique for the Numerical Solution of Certain Integral Equations of the First Kind

barticle Phillips , D.L. : 1962 , A Technique for the Numerical Solution of Certain Integral Equations of the First Kind . J. ACM 9 , 84–97 . https://doi.org/10.1145/321105.321114 . https://doi.org/10.1145/321105.321114 . barticle

1962
[168]

, Thompson , M.J

barticle Pijpers , F.P. , Thompson , M.J. : 1992 , Faster formulations of the optimally localized averages method for helioseismic inversions . 262 , L33 . 1992A&A...262L..33P . barticle

1992
[169]

, Thompson , M.J

barticle Pijpers , F.P. , Thompson , M.J. : 1994 , The SOLA method for helioseismic inversion . 281 , 231 . 1994A\ barticle

1994
[170]

, Belkacem , K

barticle Pin c on , C. , Belkacem , K. , Goupil , M.J. : 2016 , Generation of internal gravity waves by penetrative convection . 588 , A122 . https://doi.org/10.1051/0004-6361/201527663 . 2016A&A...588A.122P . barticle

2016 doi
[171]

: 2024 a, Interface of equation of state, atomic data, and opacities in the solar problem

barticle Pradhan , A.K. : 2024 a, Interface of equation of state, atomic data, and opacities in the solar problem . 527 , L179 . https://doi.org/10.1093/mnrasl/slad154 . 2024MNRAS.527L.179P . barticle

2024 doi
[172]

: 2024 b, R-matrix calculations for opacities: III

barticle Pradhan , A.K. : 2024 b, R-matrix calculations for opacities: III. Plasma broadening of autoionizing resonances . Journal of Physics B Atomic Molecular Physics 57 , 125003 . https://doi.org/10.1088/1361-6455/ad421d . 2024JPhB...57l5003P . barticle

2024 doi
[173]

, Nahar , S.N

barticle Pradhan , A.K. , Nahar , S.N. , Eissner , W. : 2024 , R-matrix calculations for opacities: I. Methodology and computations . Journal of Physics B Atomic Molecular Physics 57 , 125001 . https://doi.org/10.1088/1361-6455/ad421c . 2024JPhB...57l5001P . barticle

2024 doi
[174]

, Baraffe , I

barticle Pratt , J. , Baraffe , I. , Goffrey , T. , Constantino , T. , Viallet , M. , Popov , M.V. , Walder , R. , Folini , D. : 2017 , Extreme value statistics for two-dimensional convective penetration in a pre-main sequence star . 604 , A125 . https://doi.org/10.1051/0004-6...

2017 doi
[175]

: 2021, Observations of large-scale solar flows

botherref Proxauf , B. : 2021, Observations of large-scale solar flows . PhD thesis, Georg August University of Gottingen, Germany. 2021PhDT........26P . botherref

2021
[176]

, Setzer , M

botherref Ramelli , R. , Setzer , M. , Engelhard , M. , Bianda , M. , Paglia , F. , Stenflo , J.O. , K \"u veler , G. , Plewe , R. : 2017, Atlas of the solar intensity spectrum and its center to limb variation . arXiv e-prints, arXiv:1708.03284. 2017arXiv170803284R . botherref

2017 arXiv
[177]

, Bianda , M

bchapter Ramelli , R. , Bianda , M. , Setzer , M. , Enegelhard , M. , Paglia , F. , Stenflo , J.O. , K \"u veler , G. , Plewe , R. : 2019 , Atlas of the Solar Intensity Spectrum and its Center-to-Limb Variation . In: Belluzzi , L. , Casini , R. , Romoli , M. , Trujillo Bueno ,...

2019
[178]

a fer , M. , Schlafly , E. , Schmider , F.-X. , Schneider , J. , Schou , J. , Schunker , H. , J \

botherref Rauer , H. , Aerts , C. , Cabrera , J. , Deleuil , M. , Erikson , A. , Gizon , L. , Goupil , M. , Heras , A. , Lorenzo-Alvarez , J. , Marliani , F. , Martin-Garcia , C. , Mas-Hesse , J.M. , O'Rourke , L. , Osborn , H. , Pagano , I. , Piotto , G. , Pollacco , D. , Rag...

2024 doi arXiv
[179]

, Mrotzek , N

barticle Reiners , A. , Mrotzek , N. , Lemke , U. , Hinrichs , J. , Reinsch , K. : 2016 , The IAG solar flux atlas: Accurate wavelengths and absolute convective blueshift in standard solar spectra . 587 , A65 . https://doi.org/10.1051/0004-6361/201527530 . 2016A&A...587A..65R ...

2016 doi
[180]

, Rhodes , J

barticle Reiter , J. , Rhodes , J. E. J. , Kosovichev , A.G. , Scherrer , P.H. , Larson , T.P. , , I. S. F. Pinkerton : 2020 , A Method for the Estimation of f- and p-mode Parameters and Rotational Splitting Coefficients from Un-averaged Solar Oscillation Power Spectra . 894 ,...

2020 doi
[181]

barticle Rhodes , J. E. J. , Kosovichev , A.G. , Schou , J. , Scherrer , P.H. , Reiter , J. : 1997 , Measurements of Frequencies of Solar Oscillations from the MDI Medium-l Program . 175 , 287 . https://doi.org/10.1023/A:1004963425123 . 1997SoPh..175..287R . barticle

1997 doi
[182]

, Dziembowski , W.A

barticle Richard , O. , Dziembowski , W.A. , Sienkiewicz , R. , Goode , P.R. : 1998 , On the accuracy of helioseismic determination of solar helium abundance . 338 , 756 . 1998A&A...338..756R . barticle

1998
[183]

, Lagae , C

botherref Rodr \' guez D \' az , L.F. , Lagae , C. , Amarsi , A.M. , Bigot , L. , Zhou , Y. , Aguirre B rsen-Koch , V. , Lind , K. , Trampedach , R. , Collet , R. : 2024, An extended and refined grid of 3D STAGGER model atmospheres. Processed snapshots for stellar spectroscopy...

2024 doi arXiv
[184]

, DeWitt , H.E

barticle Rogers , F.J. , DeWitt , H.E. : 1973 , Statistical Mechanics of Reacting Coulomb Gases . Phys. Rev. A 8 , 1061 . https://doi.org/10.1103/PhysRevA.8.1061 . https://link.aps.org/doi/10.1103/PhysRevA.8.1061 . barticle

1973 doi
[185]

, Nayfonov , A

barticle Rogers , F.J. , Nayfonov , A. : 2002 , Updated and Expanded OPAL Equation-of-State Tables: Implications for Helioseismology . 576 , 1064 . https://doi.org/10.1086/341894 . 2002ApJ...576.1064R . barticle

2002 doi
[186]

, Christensen-Dalsgaard , J

barticle Rosenthal , C.S. , Christensen-Dalsgaard , J. , Nordlund , . , Stein , R.F. , Trampedach , R. : 1999 , Convective Contributions to the Frequencies of Solar Oscillations . A&A 351 , 689 . 1999A\ barticle

1999
[187]

, Boothroyd , A.I

barticle Sackmann , I.-J. , Boothroyd , A.I. : 2003 , Our Sun. V. A Bright Young Sun Consistent with Helioseismology and Warm Temperatures on Ancient Earth and Mars . 583 , 1024 . https://doi.org/10.1086/345408 . 2003ApJ...583.1024S . barticle

2003 doi
[188]

, Buldgen , G

barticle Salmon , S.J.A.J. , Buldgen , G. , Noels , A. , Eggenberger , P. , Scuflaire , R. , Meynet , G. : 2021 , Standard solar models: Perspectives from updated solar neutrino fluxes and gravity-mode period spacing . 651 , A106 . https://doi.org/10.1051/0004-6361/202140769 ....

2021 doi
[189]

, Gough , D.O

barticle Scherrer , P.H. , Gough , D.O. : 2019 , A Critical Evaluation of Recent Claims Concerning Solar Rotation . 877 , 42 . https://doi.org/10.3847/1538-4357/ab13ad . 2019ApJ...877...42S . barticle

2019 doi
[190]

, Bogart , R.S

barticle Scherrer , P.H. , Bogart , R.S. , Bush , R.I. , Hoeksema , J.T. , Kosovichev , A.G. , Schou , J. , Rosenberg , W. , Springer , L. , Tarbell , T.D. , Title , A. , Wolfson , C.J. , Zayer , I. , MDI Engineering Team : 1995 , The Solar Oscillations Investigation - Michels...

1995 doi
[191]

, Reames , D.V

barticle Schmelz , J.T. , Reames , D.V. , von Steiger , R. , Basu , S. : 2012 , Composition of the Solar Corona, Solar Wind, and Solar Energetic Particles . 755 , 33 . https://doi.org/10.1088/0004-637X/755/1/33 . 2012ApJ...755...33S . barticle

2012 doi
[192]

, Barklem , P.S

barticle Schmidt-May , A.F. , Barklem , P.S. , Grumer , J. , Amarsi , A.M. , Bj \"o rkhage , M. , Blom , M. , Dochain , A. , Ji , M. , Martini , P. , Reinhed , P. , Ros \'e n , S. , Simonsson , A. , Zettergren , H. , Cederquist , H. , Schmidt , H.T. : 2024 , State-resolved mut...

2024 doi
[193]

, Birch , A

barticle Schou , J. , Birch , A. : 2020 , Estimating the nonstructural component of the helioseismic surface term using hydrodynamic simulations . 638 , A51 . 2020A&A...638A..51S/abstract . barticle

2020
[194]

, Schou , J

barticle Schunker , H. , Schou , J. , Gaulme , P. , Gizon , L. : 2018 , Fragile Detection of Solar g -Modes by Fossat et al. 293 , 95 . https://doi.org/10.1007/s11207-018-1313-6 . 2018SoPh..293...95S . barticle

2018 doi
[195]

, Yan , Y

barticle Seaton , M.J. , Yan , Y. , Mihalas , D. , Pradhan , A.K. : 1994 , Opacities for stellar envelopes . 266 , 805 . https://doi.org/10.1093/mnras/266.4.805 . 1994MNRAS.266..805S . barticle

1994 doi
[196]

, L \"a mmerzahl , C

barticle Selig , H. , L \"a mmerzahl , C. , Ni , W.-T. : 2013 , Astrodynamical Space Test of Relativity Using Optical Devices i (astrod i) Mission Overview . International Journal of Modern Physics D 22 , 1341003 . https://doi.org/10.1142/S0218271813410034 . 2013IJMPD..2241003...

2013 doi
[197]

, Haxton , W.C

barticle Serenelli , A.M. , Haxton , W.C. , Pe \ n a-Garay , C. : 2011 , Solar Models with Accretion. I. Application to the Solar Abundance Problem . 743 , 24 . https://doi.org/10.1088/0004-637X/743/1/24 . 2011ApJ...743...24S . barticle

2011 doi
[198]

, Basu , S

barticle Serenelli , A.M. , Basu , S. , Ferguson , J.W. , Asplund , M. : 2009 , New Solar Composition: The Problem with Solar Models Revisited . ApJ 705 , L123 . 2009ApJ...705L.123S . barticle

2009
[199]

, Trujillo Bueno , J

barticle Shchukina , N. , Trujillo Bueno , J. : 2015 , The impact of surface dynamo magnetic fields on the solar iron abundance . 579 , A112 . https://doi.org/10.1051/0004-6361/201425569 . 2015A&A...579A.112S . barticle

2015 doi
[200]

, Sukhorukov , A

barticle Shchukina , N. , Sukhorukov , A. , Trujillo Bueno , J. : 2016 , Impact of surface dynamo magnetic fields on the solar abundance of the CNO elements . 586 , A145 . https://doi.org/10.1051/0004-6361/201526452 . 2016A&A...586A.145S . barticle

2016 doi
[201]

, Cranmer , S.R

barticle Shoda , M. , Cranmer , S.R. , Toriumi , S. : 2023 , Formulating Mass-loss Rates for Sun-like Stars: A Hybrid Model Approach . 957 , 71 . https://doi.org/10.3847/1538-4357/acfa72 . 2023ApJ...957...71S . barticle

2023 doi
[202]

, Demarque , P

barticle Spada , F. , Demarque , P. , Basu , S. , Tanner , J.D. : 2018 , Improved Calibration of the Radii of Cool Stars Based on 3D Simulations of Convection: Implications for the Solar Model . 869 , 135 . https://doi.org/10.3847/1538-4357/aaee75 . 2018ApJ...869..135S . barticle

2018 doi
[203]

: 1997 , Convection in stellar envelopes: a changing paradigm

barticle Spruit , H.C. : 1997 , Convection in stellar envelopes: a changing paradigm. MmSAI 68 , 397 . https://doi.org/10.48550/arXiv.astro-ph/9605020 . 1997MmSAI..68..397S . barticle

1997 doi arXiv
[204]

: 2002 , Dynamo action by differential rotation in a stably stratified stellar interior

barticle Spruit , H.C. : 2002 , Dynamo action by differential rotation in a stably stratified stellar interior . 381 , 923 . https://doi.org/10.1051/0004-6361:20011465 . http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2002A\ barticle

2002 doi
[205]

, Roerich , V.C

barticle Starostin , A.N. , Roerich , V.C. : 2006 , Equation of state of weakly nonideal plasmas and electroneutrality condition . Journal of Physics A: Mathematical and General 39 , 4431 . https://doi.org/10.1088/0305-4470/39/17/S18 . https://dx.doi.org/10.1088/0305-4470/39/1...

2006 doi
[206]

, Nordlund , A

barticle Stein , R.F. , Nordlund , A . , Collet , R. , Trampedach , R. : 2024 , The Stagger Code for Accurate and Efficient, Radiation-coupled Magnetohydrodynamic Simulations . 970 , 24 . https://doi.org/10.3847/1538-4357/ad4706 . 2024ApJ...970...24S . barticle

2024 doi
[207]

: 2015 , FTS atlas of the Sun's spectrally resolved center-to-limb variation

barticle Stenflo , J.O. : 2015 , FTS atlas of the Sun's spectrally resolved center-to-limb variation . 573 , A74 . https://doi.org/10.1051/0004-6361/201424685 . 2015A&A...573A..74S . barticle

2015 doi
[208]

, Imada , S

barticle Suzuki , T.K. , Imada , S. , Kataoka , R. , Kato , Y. , Matsumoto , T. , Miyahara , H. , Tsuneta , S. : 2013 , Saturation of Stellar Winds from Young Suns . 65 , 98 . https://doi.org/10.1093/pasj/65.5.98 . http://ads.nao.ac.jp/abs/2013PASJ...65...98S . barticle

2013 doi
[209]

, Gough , D.O

barticle Takata , M. , Gough , D.O. : 2024 , The acoustic size of the Sun . 527 , 1283 . https://doi.org/10.1093/mnras/stad3206 . 2024MNRAS.527.1283T . barticle

2024 doi
[210]

, Birnstiel , T

bchapter Testi , L. , Birnstiel , T. , Ricci , L. , Andrews , S. , Blum , J. , Carpenter , J. , Dominik , C. , Isella , A. , Natta , A. , Williams , J.P. , Wilner , D.J. : 2014 , Dust Evolution in Protoplanetary Disks . In: Beuther , H. , Klessen , R.S. , Dullemond , C.P. , He...

2014 doi
[211]

1 , Institute Of Physics Publishing , Bristol

bbook The Opacity Project Team : 1995 , The Opacity Project Vol. 1 , Institute Of Physics Publishing , Bristol . bbook

1995
[212]

: 1963 , Solution of incorrectly formulated problems and the regularization method

barticle Tikhonov , A.N. : 1963 , Solution of incorrectly formulated problems and the regularization method . Soviet Math. Dokl. 4 , 1035 . barticle

1963
[213]

, Streander , K

barticle Tomczyk , S. , Streander , K. , Card , G. , Elmore , D. , Hull , H. , Cacciani , A. : 1995 , An Instrument to Observe Low-Degree Solar Oscillations . 159 , 1 . https://doi.org/10.1007/BF00733027 . 1995SoPh..159....1T . barticle

1995 doi
[214]

: 2017 , An opaque Sun ? The potential for future, higher opacities to solve the solar abundance problem

bchapter Trampedach , R. : 2017 , An opaque Sun ? The potential for future, higher opacities to solve the solar abundance problem . In: Monteiro , M.J.P.F.G. , Cunha , M.S. , Ferreira , J.M.T. (eds.) Seismology of the Sun and the Distant Stars 2016 - J oint TASC2 & KASC9 Works...

2017
[215]

: 2020 , Non-adiabatic Helioseismology via 3D Convection Simulations

bchapter Trampedach , R. : 2020 , Non-adiabatic Helioseismology via 3D Convection Simulations . In: Monteiro , M. , Garc \' a , R. , Christensen-Dalsgaard , J. , McIntosh , S.W. (eds.) Dynamics of the Sun and Stars , Astrophysics and Space Science Proceedings 57 , Springer , N...

2020
[216]

a ppen , W. : 2024 , Various Modifications to Debye-H \

bchapter Trampedach , R. , D \"a ppen , W. : 2024 , Various Modifications to Debye-H \"u ckel Interactions in Solar Equations of State . In: ??? , 1 . bchapter

2024
[217]

a ppen , W. , Baturin , V.A. : 2006 , A synoptic comparison of the M ihalas- H ummer- D \

barticle Trampedach , R. , D \"a ppen , W. , Baturin , V.A. : 2006 , A synoptic comparison of the M ihalas- H ummer- D \"a ppen and OPAL equations of state . ApJ 646 , 560 . http://cdsads.u-strasbg.fr/abs/2006ApJ...646..560T . barticle

2006
[218]

, Christensen-Dalsgaard , J

barticle Trampedach , R. , Christensen-Dalsgaard , J. , Nordlund , . , Asplund , M. , Stein , R.F. : 2014 a, Improvements to Stellar Structure Models, Based on a Grid of 3D Convection Simulations. I . T - Relations . MNRAS 442 , 805 . http://cdsads.u-strasbg.fr/abs/2014MNRAS.4...

2014
[219]

, Christensen-Dalsgaard , J

barticle Trampedach , R. , Christensen-Dalsgaard , J. , Nordlund , . , Asplund , M. , Stein , R.F. : 2014 b, Improvements to stellar structure models, based on a grid of 3D convection simulations. II . C alibrating the mixing-length . MNRAS 445 , 4366 . 2014MNRAS.445.4366T . barticle

2014
[220]

, Aarslev , M.J

barticle Trampedach , R. , Aarslev , M.J. , Houdek , G. , Christensen-Dalsgaard , J. , Stein , R.F. , Collet , R. , Asplund , M. : 2017 , The asteroseismic surface effect from a grid of 3D convection simulations. I. F requency shifts from convective expansion of stellar atmosp...

2017
[221]

, Carton , P.-H

barticle Turck-Chi \`e ze , S. , Carton , P.-H. , Ballot , J. , Barri \`e re , J.-C. , Daniel-Thomas , P. , Delbart , A. , Desforges , D. , Garcia , R.A. , Granelli , R. , Mathur , S. , Nunio , F. , Piret , Y. , Pall \'e , P.L. , Jim \'e nez , A.J. , Jim \'e nez-Reyes , S.J. ,...

2006
[222]

, Le Pennec , M

barticle Turck-Chi \`e ze , S. , Le Pennec , M. , Ducret , J.E. , Colgan , J. , Kilcrease , D.P. , Fontes , C.J. , Magee , N. , Gilleron , F. , Pain , J.C. : 2016 , Detailed Opacity Comparison for an Improved Stellar Modeling of the Envelopes of Massive Stars . ApJ 823 , 78 . ...

2016 doi
[223]

, Richer , J

barticle Turcotte , S. , Richer , J. , Michaud , G. , Iglesias , C.A. , Rogers , F.J. : 1998 , Consistent Solar Evolution Model Including Diffusion and Radiative Acceleration Effects . 504 , 539 . https://doi.org/10.1086/306055 . 1998ApJ...504..539T . barticle

1998 doi
[224]

, Julien , K

barticle Vasil , G.M. , Julien , K. , Featherstone , N.A. : 2021 , Rotation suppresses giant-scale solar convection . Proceedings of the National Academy of Science 118 , e2022518118 . https://doi.org/10.1073/pnas.2022518118 . 2021PNAS..11822518V . barticle

2021 doi
[225]

, Lecoanet , D

barticle Vasil , G.M. , Lecoanet , D. , Augustson , K. , Burns , K.J. , Oishi , J.S. , Brown , B.P. , Brummell , N. , Julien , K. : 2024 , The solar dynamo begins near the surface . 629 , 769 . https://doi.org/10.1038/s41586-024-07315-1 . 2024Natur.629..769V . barticle

2024 doi
[226]

, Haugb lle , T

barticle Vaytet , N. , Haugb lle , T. : 2017 , A grid of one-dimensional low-mass star formation collapse models . 598 , A116 . https://doi.org/10.1051/0004-6361/201628194 . 2017A&A...598A.116V . barticle

2017 doi
[227]

: 2021 , The evolution of the solar wind

barticle Vidotto , A.A. : 2021 , The evolution of the solar wind . Living Reviews in Solar Physics 18 , 3 . https://doi.org/10.1007/s41116-021-00029-w . 2021LRSP...18....3V . barticle

2021 doi
[228]

, Ricci , B

barticle Villante , F.L. , Ricci , B. : 2010 , Linear Solar Models . 714 , 944 . https://doi.org/10.1088/0004-637X/714/1/944 . 2010ApJ...714..944V . barticle

2010 doi
[229]

, Serenelli , A

barticle Villante , F.L. , Serenelli , A. : 2021 , The relevance of nuclear reactions for Standard Solar Models construction . Frontiers in Astronomy and Space Sciences 7 , 112 . https://doi.org/10.3389/fspas.2020.618356 . 2021FrASS...7..112V . barticle

2021
[230]

, Baraffe , I

barticle Vlaykov , D.G. , Baraffe , I. , Constantino , T. , Goffrey , T. , Guillet , T. , Le Saux , A. , Morison , A. , Pratt , J. : 2022 , Impact of radial truncation on global 2D hydrodynamic simulations for a Sun-like model . 514 , 715 . https://doi.org/10.1093/mnras/stac12...

2022 doi
[231]

, Baturin , V.A

barticle Vorontsov , S.V. , Baturin , V.A. , Pamiatnykh , A.A. : 1991 , Seismological measurement of solar helium abundance . 349 , 49 . https://doi.org/10.1038/349049a0 . 1991Natur.349...49V . barticle

1991 doi
[232]

, Baturin , V.A

barticle Vorontsov , S.V. , Baturin , V.A. , Ayukov , S.V. , Gryaznov , V.K. : 2013 , Helioseismic calibration of the equation of state and chemical composition in the solar convective envelope . 430 , 1636 . https://doi.org/10.1093/mnras/sts701 . 2013MNRAS.430.1636V . barticle

2013 doi
[233]

, Baturin , V.A

barticle Vorontsov , S.V. , Baturin , V.A. , Ayukov , S.V. , Gryaznov , V.K. : 2014 a, Helioseismic measurements in the solar envelope using group velocities of surface waves . MNRAS 441 , 3296 . barticle

2014
[234]

, Baturin , V.A

barticle Vorontsov , S.V. , Baturin , V.A. , Ayukov , S.V. , Gryaznov , V.K. : 2014 b, Helioseismic measurements in the solar envelope using group velocities of surface waves . 441 , 3296 . https://doi.org/10.1093/mnras/stu813 . 2014MNRAS.441.3296V . barticle

2014 doi
[235]

, Freytag , B

barticle Wedemeyer , S. , Freytag , B. , Steffen , M. , Ludwig , H.-G. , Holweger , H. : 2004 , Numerical simulation of the three-dimensional structure and dynamics of the non-magnetic solar chromosphere . 414 , 1121 . https://doi.org/10.1051/0004-6361:20031682 . 2004A&A...414...

2004 doi
[236]

, Bai , X.-N

barticle Weiss , B.P. , Bai , X.-N. , Fu , R.R. : 2021 , History of the solar nebula from meteorite paleomagnetism . Science Advances 7 , eaba5967 . https://doi.org/10.1126/sciadv.aba5967 . 2021SciA....7.5967W . barticle

2021 doi
[237]

, M \"u ller , H.-R

barticle Wood , B.E. , M \"u ller , H.-R. , Zank , G.P. , Linsky , J.L. , Redfield , S. : 2005 , New Mass-Loss Measurements from Astrospheric Ly Absorption . 628 , L143 . https://doi.org/10.1086/432716 . 2005ApJ...628L.143W . barticle

2005 doi
[238]

, Noyes , R.W

barticle Woodard , M.F. , Noyes , R.W. : 1985 , Change of solar oscillation eigenfrequencies with the solar cycle . 318 , 449 . https://doi.org/10.1038/318449a0 . 1985Natur.318..449W . barticle

1985 doi
[239]

: 2018 , Element Abundance Ratios in the Quiet Sun Transition Region

barticle Young , P.R. : 2018 , Element Abundance Ratios in the Quiet Sun Transition Region . 855 , 15 . https://doi.org/10.3847/1538-4357/aaab48 . 2018ApJ...855...15Y . barticle

2018 doi
[240]

, Soven , P

barticle Zangwill , A. , Soven , P. : 1980 , Density-functional approach to local-field effects in finite systems: Photoabsorption in the rare gases . Phys. Rev. A 21 , 1561 . https://doi.org/10.1103/PhysRevA.21.1561 . https://link.aps.org/doi/10.1103/PhysRevA.21.1561 . barticle

1980 doi
[241]

, Li , Y

barticle Zhang , Q.-S. , Li , Y. , Christensen-Dalsgaard , J. : 2019 , Solar Models with Convective Overshoot, Solar-wind Mass Loss, and PMS Disk Accretion: Helioseismic Quantities, Li Depletion, and Neutrino Fluxes . 881 , 103 . https://doi.org/10.3847/1538-4357/ab2f77 . 2019...

2019 doi
[242]

, Nahar , S.N

barticle Zhao , L. , Nahar , S.N. , Pradhan , A.K. : 2024 , R-matrix calculations for opacities: IV. Convergence, completeness, and comparison of relativistic R-matrix and distorted wave calculations for Fe XVII and Fe XVIII . Journal of Physics B Atomic Molecular Physics 57 ,...

2024 doi
[243]

, Amarsi , A.M

barticle Zhou , Y. , Amarsi , A.M. , Aguirre B rsen-Koch , V. , Karlsmose , K.G. , Collet , R. , Nordlander , T. : 2023 , 3D Stagger model atmospheres with FreeEOS. I. Exploring the impact of microphysics on the Sun . 677 , A98 . https://doi.org/10.1051/0004-6361/202346398 . 2...

2023 doi

Pith tools

Reviewed August 7, 2026 · model on record in the stance chip above.

[1] [1]

, Aliotta , M

botherref Acharya , B. , Aliotta , M. , Balantekin , A.B. , Bemmerer , D. , Bertulani , C.A. , Best , A. , Brune , C.R. , Buompane , R. , Cavanna , F. , Chen , J.W. , Colgan , J. , Czarnecki , A. , Davids , B. , deBoer , R.J. , Delahaye , F. , Depalo , R. , Garc \' a , A. , Gatu Johnson , M. , Gazit , D. , Gialanella , L. , Greife , U. , Guffanti , D. , G...

work page doi:10.48550/arxiv.2405.06470 2024

[2] [2]

, Mathis , S

barticle Aerts , C. , Mathis , S. , Rogers , T.M. : 2019 , Angular Momentum Transport in Stellar Interiors . 57 , 35 . https://doi.org/10.1146/annurev-astro-091918-104359 . 2019ARA&A..57...35A . barticle

doi:10.1146/annurev-astro-091918-104359 2019

[3] [3]

, Barklem , P.S

barticle Amarsi , A.M. , Barklem , P.S. , Asplund , M. , Collet , R. , Zatsarinny , O. : 2018 , Inelastic O+H collisions and the O I 777 nm solar centre-to-limb variation . 616 , A89 . https://doi.org/10.1051/0004-6361/201832770 . 2018A&A...616A..89A . barticle

doi:10.1051/0004-6361/201832770 2018

[4] [4]

, Grevesse , N

barticle Amarsi , A.M. , Grevesse , N. , Asplund , M. , Collet , R. : 2021 , The solar carbon, nitrogen, and oxygen abundances from a 3D LTE analysis of molecular lines . 656 , A113 . https://doi.org/10.1051/0004-6361/202141384 . 2021A&A...656A.113A . barticle

doi:10.1051/0004-6361/202141384 2021

[5] [5]

, Ogneva , D

barticle Amarsi , A.M. , Ogneva , D. , Buldgen , G. , Grevesse , N. , Zhou , Y. , Barklem , P.S. : 2024 , The solar beryllium abundance revisited with 3D non-LTE models . 690 , A128 . https://doi.org/10.1051/0004-6361/202451778 . 2024A&A...690A.128A . barticle

doi:10.1051/0004-6361/202451778 2024

[6] [6]

, Lecoanet , D

barticle Anders , E.H. , Lecoanet , D. , Brown , B.P. : 2019 , Entropy Rain: Dilution and Compression of Thermals in Stratified Domains . 884 , 65 . https://doi.org/10.3847/1538-4357/ab3644 . 2019ApJ...884...65A . barticle

doi:10.3847/1538-4357/ab3644 2019

[7] [7]

O . , Pietrofaccia , L. , Pilipenko , N. , Pocar , A. , Raikov , G. , Ranalli , M.T. , Ranucci , G. , Razeto , A. , Re , A. , Redchuk , M. , Rossi , N. , Sch \

barticle Appel , S. , Bagdasarian , Z. , Basilico , D. , Bellini , G. , Benziger , J. , Biondi , R. , Caccianiga , B. , Calaprice , F. , Caminata , A. , Cavalcante , P. , Chepurnov , A. , D'Angelo , D. , Derbin , A. , Di Giacinto , A. , Di Marcello , V. , Ding , X.F. , Di Ludovico , A. , Di Noto , L. , Drachnev , I. , Franco , D. , Galbiati , C. , Ghiano ...

2022

[8] [8]

, Corbard , T

barticle Appourchaux , T. , Corbard , T. : 2019 , Searching for g modes. II. Unconfirmed g-mode detection in the power spectrum of the time series of round-trip travel time . 624 , A106 . https://doi.org/10.1051/0004-6361/201935196 . 2019A&A...624A.106A . barticle

doi:10.1051/0004-6361/201935196 2019