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Cited article:

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The Future of Solar Modelling: Requirements for a New Generation of Solar Models

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Impact of near-degeneracy effects on linear rotational inversions for red giant stars

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NNHMC: An Efficient Stokes Inversion Method Using a Neural Network (NN) Model Combined with the Hamiltonian Monte Carlo (HMC) Algorithm

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The Astrophysical Journal 977 (1) 101 (2024)
https://doi.org/10.3847/1538-4357/ad8b2b