2006
DOI: 10.1080/11035890601282085
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The Late Wenlock Mulde positive carbon isotope (δ13Ccarb) excursion in North America

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Cited by 54 publications
(62 citation statements)
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“…In the past years, several pronounced, positive, short-lived Silurian stable carbon isotope excursions have been verified on different paleocontinents (Samtleben et al 1996(Samtleben et al , 2000Kaljo et al 1997;Wigforss-Lange 1999;Saltzman 2001;Cramer and Saltzman 2005;Martma et al 2005;Cramer et al 2006;Melchin and Holmden 2006;Kaljo and Martma 2006;Lehnert et al 2007; Kaljo et al 2007;Jeppsson et al 2007;Munnecke and Männik 2009). The one in the Late Ludlow with an amplitude of more than 10% in some regions represents the strongest shortlived positive d 13 C excursion known so far.…”
Section: Introductionmentioning
confidence: 92%
“…In the past years, several pronounced, positive, short-lived Silurian stable carbon isotope excursions have been verified on different paleocontinents (Samtleben et al 1996(Samtleben et al , 2000Kaljo et al 1997;Wigforss-Lange 1999;Saltzman 2001;Cramer and Saltzman 2005;Martma et al 2005;Cramer et al 2006;Melchin and Holmden 2006;Kaljo and Martma 2006;Lehnert et al 2007; Kaljo et al 2007;Jeppsson et al 2007;Munnecke and Männik 2009). The one in the Late Ludlow with an amplitude of more than 10% in some regions represents the strongest shortlived positive d 13 C excursion known so far.…”
Section: Introductionmentioning
confidence: 92%
“…Jeppsson 1990;Talent et al 1993;Samtleben et al 1996;Jeppsson and Aldridge 2000;Saltzman 2001Saltzman , 2005Kaljo et al 2003;Lehnert et al 2003;Cramer et al 2006). The overall magnitudes of the Silurian CIEs are today well known and they are well tied to the current graptolite and conodont stratigraphy (Talent et al 1993;Munnecke et al 2003;Porebska et al 2004;Jeppsson 2005;Jeppsson et al 2007).…”
Section: Introductionmentioning
confidence: 94%
“…Isotope data from many other Silurian sections exhibit very low oxygen values (below -10‰), indicative of diagenetic modification of the oxygen isotope record, but preserve a largely unmodified carbon isotope signal (see e.g. data 202 presented in Andrew et al 1994, Wigforss-Lange 1999, Cramer et al 2006) with excursions clearly recognizable. One might argue that it is possible that there is no CIE in this interval due to isolation of the Welsh Basin resulting from progressive closure of the Iapetus Ocean (as suggested by Woodcock et al 1988, Smith & Ainsworth 1989.…”
Section: The Upper Leintwardine Formation/lower Whitcliffe Formation mentioning
confidence: 99%