2004
DOI: 10.1016/s0377-0273(03)00320-2
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Carbon dioxide and carbon monoxide emission rates from an alkaline intra-plate volcano: Mt. Erebus, Antarctica

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Cited by 40 publications
(30 citation statements)
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“…Few data on volcanic emission rates of CO are available in the literature, but our values are comparable to Mt. Erebus (1.74 kg/s [ Wardell et al , 2004]) and higher than those observed at Oldoinyo Lengai (0.08 kg/s [ Oppenheimer et al , 2002]), a carbonatite volcano on the East African Rift zone. Halogen emissions (HCl and HF) from Nyiragongo are lower than typical emissions from Mt.…”
Section: Discussionsupporting
confidence: 56%
“…Few data on volcanic emission rates of CO are available in the literature, but our values are comparable to Mt. Erebus (1.74 kg/s [ Wardell et al , 2004]) and higher than those observed at Oldoinyo Lengai (0.08 kg/s [ Oppenheimer et al , 2002]), a carbonatite volcano on the East African Rift zone. Halogen emissions (HCl and HF) from Nyiragongo are lower than typical emissions from Mt.…”
Section: Discussionsupporting
confidence: 56%
“…Our measurements contribute to a better evaluation of H 2 emissions from active volcanism. While it has long been known that volcanoes are important atmospheric sources of “reduced” chemical species such as CO [ Wardell et al , 2004] and H 2 S [ Aiuppa et al , 2005], the volcanic contribution to the global H 2 atmospheric budget is poorly known: the only available estimate is from Warneck [1988], who reported a global H 2 volcanic flux of ∼200 Gg yr −1 . If our mean H 2 ‐SO 2 ratio of 0.013 (molar) is used in tandem with time‐averaged SO 2 flux from Etna of 1600 Gg yr −1 (or 4500 t d −1 [ Allard , 1997]), we obtain a first‐order assessment of the volcano's H 2 flux of 0.65 Gg yr −1 (range 0.1–2 Gg yr −1 ).…”
Section: Discussionmentioning
confidence: 99%
“…This lack of information is due to from the inherent analytical complexity of resolving the volcanic CO 2 isotopic signature from the overwhelming atmospheric CO 2 signal (Gagliardi et al 2002). Thus, whilst CO 2 concentrations in volcanic plumes are increasingly investigated thanks to the advent of modern IR (infrared) spectroscopic methods (Allard et al 1991a(Allard et al , 1994Gerlach et al 1997Gerlach et al , 1998Gerlach et al , 2002Burton et al 2000;Goff et al 2001;Wardell et al 2001Wardell et al , 2004Aiuppa et al 2006Aiuppa et al , 2007Aiuppa et al , 2008Oppenheimer et al 2006;Hager et al 2008), there are no isotopic constraints on the origin of such gas emissions, which prevents us from more in depth characterisation of CO 2 exchanges among the different geochemical reservoirs.…”
Section: Introductionmentioning
confidence: 99%