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Fig. 6. Silurian—Carboniferous atmospheric pO, and the “Devonian charcoal gap.” Atmospheric pO, curves are from Fig. 5. Fossil charcoal records: (1) Platyschima Shale Member, Downton Castle Formation (Glasspool et al., 2004); (2) Ditton Formation (Edwards and Axe, 2004); (3) Duncannon Member, Catskill Formation (Cressler, 2001); (4) Hangenberg Sandstone (Rowe and Jones, 2000); (5) Berea Sandstone (Beck et al., 1982); (6) Cementstone Group (Scott et al., 1985); (7) Horton Group (Falcon-Lang, 2000); (8) Moyny Limestone (Falcon-Lang, 1998); (9) Upper Shalwy Beds (Nichols and Jones, 1992); (10) Strathclyde Group (Scott and Jones, 1994); (/7) Namurian B units, Staffordshire, England (Scott et al., 1997). The presence of fossil charcoal implies atmospheric O2 levels >13% for sustained combustion of plant tissue; soil diffusion modeling imposes an O» minimum of 8% for the Late Devonian (arrow with “G”; Yapp, 1996). Inset at top: stratigraphic trends in inertinite and vitrinite abundances in the Famennian Ohio Shale and Early Tournaisian Sunbury Shale (Rimmer et al., 2004).

Figure 6 Silurian—Carboniferous atmospheric pO, and the “Devonian charcoal gap.” Atmospheric pO, curves are from Fig. 5. Fossil charcoal records: (1) Platyschima Shale Member, Downton Castle Formation (Glasspool et al., 2004); (2) Ditton Formation (Edwards and Axe, 2004); (3) Duncannon Member, Catskill Formation (Cressler, 2001); (4) Hangenberg Sandstone (Rowe and Jones, 2000); (5) Berea Sandstone (Beck et al., 1982); (6) Cementstone Group (Scott et al., 1985); (7) Horton Group (Falcon-Lang, 2000); (8) Moyny Limestone (Falcon-Lang, 1998); (9) Upper Shalwy Beds (Nichols and Jones, 1992); (10) Strathclyde Group (Scott and Jones, 1994); (/7) Namurian B units, Staffordshire, England (Scott et al., 1997). The presence of fossil charcoal implies atmospheric O2 levels >13% for sustained combustion of plant tissue; soil diffusion modeling imposes an O» minimum of 8% for the Late Devonian (arrow with “G”; Yapp, 1996). Inset at top: stratigraphic trends in inertinite and vitrinite abundances in the Famennian Ohio Shale and Early Tournaisian Sunbury Shale (Rimmer et al., 2004).