Fig. 2: Simulated Hg enrichment and Δ199Hg shift in model runs #1 and #3. | Communications Earth & Environment

Fig. 2: Simulated Hg enrichment and Δ199Hg shift in model runs #1 and #3.

From: Mercury isotope evidence for marine photic zone euxinia across the end-Permian mass extinction

Fig. 2

Simulated Hg enrichment factor (EF) and Δ199Hg shift in the coastal sediments in response to an increase in volcanism only (a), combined volcanism and soil erosion (b), and volcanism and coastal PZE (c). The amounts of soil erosion are expressed as times background soil erosion rate coefficients (kse_bg); the intensities of PZE are expressed as increasing isotope enrichment factors of odd-MIF associated with photoreduction of Hg(II) in the coastal ocean (Eocc(II-0),pho). The thick and thin solid lines represent simulations under high and low volcanic Hg emissions, respectively; the thick and thin solid lines of Δ199Hg shift are largely overlapped due to insensitive response of Δ199Hg to volcanic Hg emissions. The vertical shading and dashed lines are the same as Fig. 1. The simulated EF and Δ199Hg shifts (lines) are calculated relative to their background steady-state values of the model. The measured EF and Δ199Hg shifts (data symbols) are calculated relative to their background Hg/TOC (40 ppb/%) and Δ199Hg values (0.09‰) of the Late Permian. Note two samples with high EF values (45 and 78) at ~251.941 Ma (onset of the EPME) are excluded due to low TOC values (<0.2%). Fsubaerial Hg_bg: background subaerial volcanic Hg flux.

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