The Effects of Hydrostatic Pressure on the Deep Submarine Silicic Lavas - Havre 2012 Eruption
Abstract:
The Havre 2012 eruption was the first deep submarine silicic eruption ever recorded (Carey et al. 2014; Jutzeler et al. 2014). The high-resolution map and seafloor observations obtained by the MESH cruise (Soule and Carey, 2015) revealed that the eruption produced fourteen silicic lavas of 0.24±0.08 km3 in total volume along the southern rim of the Havre caldera. Differences in lava volume (<0.001~0.12 km3), length (0.002~1.35 km), composition (69~71 wt.% SiO2), morphology (domes or channelized lobes), and depth (1500 ~ 900 mbsl) provide an excellent opportunity to investigate the influence of environment vs magma properties on lava morphology in the deep submarine setting.
Our morphological analysis on 1-m gridded bathymetry suggests that the lobate lavas have the multiple levee structures which allow calculation of the apparent yield strength of the lava flow approximating it to a Bingham fluid (Hulme, 1974). The initial calculations for lava lobes emplaced on a gentle slope (< 10°) demonstrate yield strength of <105 Pa which is comparable to lavas of andesitic, or even basaltic-andesitic composition. This calculation together with measurements of 0.9 wt.% residual H2O in glass derived from FTIR (Fourier Transform Infrared Spectroscopy) analysis on a single lava (Mundana, 2016) supports the hypothesis that hydrostatic pressure can influence the viscosity (and hence morphology) of submarine lavas through the suppression of volatile exsolution.