Methane seeps and mud volcanoes in Italy: Gas origin, fractionation and emission to the atmosphere

被引:79
作者
Etiope, Giuseppe [1 ]
Martinelli, Giovanni
Caracausi, Antonio
Italiano, Francesco
机构
[1] Ist Nazl Geofis & Vulcanol, Sect Roma 2, Rome, Italy
[2] Emilia Romagna Region, Environmental Protect Agcy, Bologna, Italy
[3] Ist Nazl Geofis & Vulcanol, Palermo, Italy
关键词
D O I
10.1029/2007GL030341
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Molecular composition, CH4 isotopes and gas flux of all main terrestrial mud volcanoes and other methane seeps in Italy are being assessed for the first time. Whereas 74% of the Italian gas reservoirs are biogenic, about 80% of the seeps release thermogenic gas. Dry- seep gas generally maintains the reservoir C-1/( C-2 + C-3) " Bernard'' ratio while mud volcanoes show molecular fractionation likely occurring during advective migration. Accordingly, a simple and direct use of the " Bernard'' parameter might be misleading when applied to mud volcanoes as it could not always reflect the reservoir composition. Methane flux into the atmosphere from macro-seep areas is in the order of 10(2) - 10(6) t km (-2) y (-1). Microseepage is widespread throughout large areas and, on a regional scale, it provides the main methane output. A first emission estimate for the total hydrocarbon- prone area of Italy suggests levels of 10(5) t y (-1), comparable to national sources from fossil fuel industry.
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页数:5
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