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

The Milne–Eddington (M-E) atmosphere model is commonly adopted in the inversion of the magnetic fields in the solar photosphere. By applying the Levenberg–Marquardt algorithm or training a neural network (NN) model, the magnetic field vector can be quickly inferred from the Stokes profile but lacks...

وصف كامل

التفاصيل البيبلوغرافية
الحاوية / القاعدة:The Astrophysical Journal
المؤلفون الرئيسيون: Chong Xu, JinLiang Wang, Hao Li, ZiYao Hu, XianYong Bai, JiaBen Lin, Hui Liu, ZhenYu Jin, KaiFan Ji
التنسيق: مقال
اللغة:الإنجليزية
منشور في: IOP Publishing 2024-01-01
الموضوعات:
Solar magnetic fields
Computational methods
Bayesian statistics
Markov chain Monte Carlo
الوصول للمادة أونلاين:https://doi.org/10.3847/1538-4357/ad8b2b

الانترنت

https://doi.org/10.3847/1538-4357/ad8b2b

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