“…Cailteux et al, 2015; Hoffman et al, 2011; Mickala et al, 2014), Kalahari (Hoffman et al, 2011, 2017), India (Jiang, Sohl, & Christie‐Blick, 2003; Kaufman et al, 2006), Laurentia (e.g., Creveling et al, 2016; Kunzmann et al, 2017; Macdonald et al, 2010; Macdonald, McClelland, et al, 2009; Prave et al, 2009), South China (Huang et al, 2009, 2011, 2013; Jiang et al, 2007, 2008, 2011; Jiang, Kennedy, et al, 2006; Jiang, Kennedy, & Christie‐Blick, 2003; Jiang, Shi, & Zhang, 2006; Tahata et al, 2013; Wang et al, 2008, 2014; Wang, Wang, et al, 2012; Xiong et al, 2013, 2014; Zhao et al, 2018; Zhou et al, 2007, 2010; Zhou, Luo, et al, 2017; Zhou & Xiao, 2007), Siberia (Sovetov & Komlev, 2005; Sovetov & Le Heron, 2016), Tarim (Shen et al, 2008; Xiao et al, 2004), Tuva‐Mongolia (Macdonald & Jones, 2011; Macdonald, Jones, & Schrag, 2009), and West Africa (Hoffman, 2011; Nédélec et al, 2007; Porter et al, 2004; Shields et al, 2007). As these Ediacaran cap carbonates were formed in transgressive system tracts (TST) in the process of rapid sea‐level rise after the Marinoan glacier ablation (Kennedy, 1996; Kuang et al, 2019, 2022; Mei et al, 2006; Wang, Wang, et al, 2017; Zhou et al, 2010), they generally share the following distinctive features: (1) direct overlying the Marinoan glacial diamictites, which are usually interpreted as a precursor of the Marinoan terminal deglaciation; (2) remarkably thin (usually only meter‐ to decameter‐thick) but laterally continuous strata (Hoffman et al, 2017); (3) unusual sedimentary structures, such as tepee‐like structures, tube‐like structures, sheet‐cracks and isopachous cemented brecciations (Hoffman &...…”