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Fig. 3 | Earth, Planets and Space

Fig. 3

From: Comparison between the Hamiltonian Monte Carlo method and the Metropolis–Hastings method for coseismic fault model estimation

Fig. 3

Inferred posterior probability density function (PDF) due to Hamiltonian Monte Carlo (HMC) and Random walk Metropolis–Hastings (RWMH) estimation. Both results of HMC and RWMH are shown by blue and red lines, respectively. The y-axis represent the normalized frequency of Markov chain Monte Carlo (MCMC). Then the insert values represent statistics (the mean, median, mode, and length of 95% confidence interval of PDFs from top to bottom) similarly presented in blue or red

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