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Geodynamically induced variations in the emission of CO2 gas at San Faustino (Central Apennines, Italy)

Academic Article
Publication Date:
2012
abstract:
The Central Apennines are affected by frequent earthquakes of moderate magnitude that occur mainly within the upper part of the crust at depths of <15km. A large number of cold gas emissions that are rich in CO 2 are also found in the region. One particular vent with a high rate of degassing was equipped with a sensor to measure flow rates, which were recorded for a number of different periods between 2005 and 2010. Factors that could affect potentially CO 2 flow rates include barometric pressure, atmospheric temperature, precipitation and local seismicity. Our analysis indicates that the periods of anomalous flow rate were related not to the environmental factors but probably to the deformative processes of the crust associated with the local seismicity. Local seismic events as expression of geodynamic processes occurred always before and during these anomalous gas flow periods. This correlation exists only for events that occurred eastwards of the gas emission site close to the Martana fault zone. We herein consider this correlation as indication for a continuous interaction between the field of static strain and the deep fluid pressure. An approximation of the fluid pressure transmission towards the gas emission site gives reasonable values of 1-10m 2sec -1. To make comparisons with the long-term effects of the static strain, we also recorded the short-term effects of the dynamic release of strain induced by the series of strong earthquakes that took place in L'Aquila in 2009. We detected a significant anomalous flow rate that occurred at the same time as this seismic sequence, during which widespread degassing was induced around the focal zone.
Iris type:
01.01 Articolo in rivista
Keywords:
CO2; fluids; geodynamic; seismicity; static strain
List of contributors:
Telesca, Luciano
Authors of the University:
TELESCA LUCIANO
Handle:
https://iris.cnr.it/handle/20.500.14243/174132
Published in:
GEOFLUIDS (OXFORD. PRINT)
Journal
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