“…As described by Kvenvolden [1988b] and considered in numerous observational and modeling studies [e.g., Berndt et al, 2014;Brothers et al, 2014;Davies et al, 2015;Gorman and Senger, 2010;Johnson et al, 2015;Kennett et al, 2003;Marín-Moreno et al, 2015;Marín-Moreno et al, 2013;Mienert et al, 2005;Pecher et al, 2005;Phrampus and Hornbach, 2012;Phrampus et al, 2014;Reagan and Moridis, 2009;Reagan et al, 2011;Ruppel, 2011a;Skarke et al, 2014;Stranne et al, 2016a;Stranne et al, 2016b;Weinstein et al, 2016;Westbrook et al, 2009] gas hydrates within upper continental slope sediments constitute the key marine hydrate population that is susceptible to degradation during ocean warming (Figure 9). The GHSZ vanishes on upper slopes (i.e., the "feather edge" of hydrate stability in Ruppel [2011a]).…”