The Fe I 4377 Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis

arXiv:2607.29455 · astro-ph.SR, astro-ph.EP, astro-ph.IM · Submitted 2026-07-31 · Read on arXiv

Katlyn L. Hobbs, Christopher A. Watson, Jean C. Costes, Yvonne Unruh, Dana Clarice Yaptangco, Krishnamurthy Sowmya, Mitchell E. Young, Ernst J. W. de Mooij, Alexander G. M. Pietrow, Pál Váradi Nagy, Alexander I. Shapiro, Veronika Witzke, Federica Rescigno, Ryan A. Rubenzahl, Megan Bedell, Andrew Collier Cameron, Xavier Dumusque, Sean M. O'Brien, Benjamin M. J. Cadell, Baptiste Klein, Niamh Mallaghan, Niamh K. O'Sullivan, Toby Rodel, Sara Tavella

Queen's University Belfast · Queen's University Belfast · Queen's University Belfast · Imperial College London · Imperial College London · University of Graz · Queen's University Belfast · Queen's University Belfast · Leibniz-Institut für Astrophysik Potsdam · Independent Researcher · Max-Planck-Institut für Sonnensystemforschung · University of Graz · University of Birmingham · Flatiron Institute · Flatiron Institute · University of St Andrews · University of Geneva · Queen's University Belfast · Queen's University Belfast · University of Oxford · Queen's University Belfast · University of Oxford · Queen's University Belfast · University of Geneva

astro-ph.SR, astro-ph.EP, astro-ph.IM

Submitted: 2026-07-31

Comments: 16 pages, 12 figures. Accepted for publication in MNRAS

DOI: 10.1093/mnras/stag1462

Code: https://github.com/melix/astro4j

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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