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Fig. 8 | Earth, Planets and Space

Fig. 8

From: A novel Bayesian approach for disentangling solar and geomagnetic field influences on the radionuclide production rates

Fig. 8

Assessing solar activity and GDM reconstruction of the Bayesian model with the synthetic dataset. Posterior distributions of solar activity (a) and GDM (b) depicted with means (red lines) and 2-sigma uncertainty of a thousand realizations (light red shadings). The prior distributions are also depicted with the 2-sigma uncertainty (black dashed lines). The blue lines represent the reference ϕ' and M' and the orange lines represent the recent values that the model is connected to, i.e., ϕHE16 and GDM based on COV-OBS. × 2. c Shows the mean (red line) and 2-sigma uncertainty (light red shading) of a thousand 14C production rate curves generated by the recovered ϕ and M. The reference 14C production rate is represented by the blue line. d Shows the histogram of the model-data residuals (grey bars) defined as the differences between individual posterior realizations of 14C production rate and the input 14C data, normalized by the data uncertainties. A standard normal distribution is shown as the blue line for comparison

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