ABSTRACT

By using a permanent network of multi-component gas analyzer systems (Multi-GAS), we report for the first time the H₂O-CO₂-SO₂ composition of the volcanic gases emitted prior to, during, and after terminal Strombolian activity at Mount Etna’s central craters (CCs). We show that the summer 2012 Strombolian episodes of the Bocca Nuova crater (BNC), the largest of Etna’s CCs, are associated with the emission of the most CO₂-rich gas measured at the volcano thus far. The BNC plume was particularly CO₂-rich with CO₂/SO₂ up to 100, H₂O/CO₂ < 1 in the quiescent periods between Strombolian episodes. However, more CO₂-poor gas with CO₂/SO₂ < 27, H₂O/CO₂ > 1 prevailed at the BNC and at other degassing vents such as Voragine and Northeast craters during Strombolian eruptions. Based on the results of numerical simulations of volcanic degassing, conclude that the shallow Etna plumbing system was invaded in summer 2012 by a CO₂-rich gas front likely supplied by the deep (>100 MPa pressure) volcano’s magmatic storage zone. This deep gas-bubble supply eventually caused a general rejuvenation of the resident magma in the upper conduits/shallow reservoirs, thereby triggering the first Strombolian episodes on the volcano’s summit after years of quiescence.