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Solar Bayesian Analysis Toolkit-A New Markov Chain Monte Carlo IDL Code for Bayesian Parameter Inference
被引:36
作者:

Anfinogentov, Sergey A.
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机构:
Inst Solar Terr Phys SB RAS, Lermontov St 126, Irkutsk 664033, Russia Inst Solar Terr Phys SB RAS, Lermontov St 126, Irkutsk 664033, Russia

Nakariakov, Valery M.
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机构:
Univ Warwick, Phys Dept, Ctr Fus Space & Astrophys, Coventry CV4 7AL, W Midlands, England
Russian Acad Sci, St Petersburg Branch, Special Astrophys Observ, St Petersburg 196140, Russia Inst Solar Terr Phys SB RAS, Lermontov St 126, Irkutsk 664033, Russia

Pascoe, David J.
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机构:
Katholieke Univ Leuven, Math Dept, Ctr Math Plasma Astrophys, Celestijnenlaan 200B Bus 2400, B-3001 Leuven, Belgium Inst Solar Terr Phys SB RAS, Lermontov St 126, Irkutsk 664033, Russia

Goddard, Christopher R.
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机构:
Univ Warwick, Phys Dept, Ctr Fus Space & Astrophys, Coventry CV4 7AL, W Midlands, England Inst Solar Terr Phys SB RAS, Lermontov St 126, Irkutsk 664033, Russia
机构:
[1] Inst Solar Terr Phys SB RAS, Lermontov St 126, Irkutsk 664033, Russia
[2] Univ Warwick, Phys Dept, Ctr Fus Space & Astrophys, Coventry CV4 7AL, W Midlands, England
[3] Russian Acad Sci, St Petersburg Branch, Special Astrophys Observ, St Petersburg 196140, Russia
[4] Katholieke Univ Leuven, Math Dept, Ctr Math Plasma Astrophys, Celestijnenlaan 200B Bus 2400, B-3001 Leuven, Belgium
基金:
英国科学技术设施理事会;
俄罗斯科学基金会;
欧洲研究理事会;
关键词:
Solar physics;
Bayesian statistics;
Astronomy data analysis;
Astronomy software;
Markov chain Monte Carlo;
D O I:
10.3847/1538-4365/abc5c1
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We present the Solar Bayesian Analysis Toolkit (SoBAT), which is a new easy to use tool for Bayesian analysis of observational data, including parameter inference and model comparison. SoBAT is aimed (but not limited) to be used for the analysis of solar observational data. We describe a new IDL code designed to facilitate the comparison of a user-supplied model with data. Bayesian inference allows prior information to be taken into account. The use of Markov Chain Monte Carlo sampling allows efficient exploration of large parameter spaces and provides reliable estimation of model parameters and their uncertainties. The Bayesian evidence for different models can be used for quantitative comparison. The code is tested to demonstrate its ability to accurately recover a variety of parameter probability distributions. Its application to practical problems is demonstrated using studies of the structure and oscillation of coronal loops.
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