Vertical deformation of the Axial Seamount summit from repeated 1-m scale bathymetry surveys using AUVs

Axial Seamount is an intensely studied submarine hotspot volcano on the Juan de Fuca Ridge that erupted in 1998, 2011, and 2015. MBARI Mapping AUV surveys during 2006-2009 obtained nearly complete 1 m resolution topographic coverage of the Axial Seamount summit, including the caldera, the caldera rim, and the south rift zone. Surveys following both recent eruptions mapped new lava flows and extended coverage of the caldera rim and the north and south rifts. These include 2011 (post-eruption), 2014, and 2016 MBARI Mapping AUV surveys and 2015 (post-eruption) WHOI AUV Sentry surveys. These AUVs use 200 kHz or 400 kHz multibeam sonars operated from 50 m to 75 m altitudes to achieve 1 m lateral resolution and 0.1 m vertical precision. Differencing repeat surveys allows detection of topographic change > 0.2 m, a capability used to map the extent, morphology and volume of lava flows emplaced by the 2011 and 2015 eruptions. In situ pressure observations show the uplift and subsidence of the caldera center associated with pre-eruption inflation and co-eruption deflation of the sub-caldera magma chamber has a 2.5-3.5 m magnitude, and thus can be observed by repeat AUV surveys. A survey pattern crossing the caldera interior both E-W and N-S and extending 8 km down the south rift was established in 2011 that has been repeated in 2014, 2015, and 2016. The 2015 surveys established a larger, asterisk-shaped survey pattern extending about 4 km outside the caldera walls along seven lines that has now been repeated in 2016. Repeat survey comparison reveals the vertical deformation pattern of the eruption cycle. Between 2011 and 2014 the uplift has a maximum of 1.8 m near the caldera center, and diminishes steadily away from this site. Between 2014 and 2015 there is a 1.0 m subsidence of the caldera center associated with the April 2015 eruption. The comparison of the 2011 and 2015 surveys shows that the caldera floor is slightly uplifted four months after the 2015 eruption relative to four months after the 2011 eruption. Results incorporating the new 2016 surveys will be presented. These results are consistent with 1 cm precision pressure benchmark observations on the caldera and south rift by Chadwick and Nooner. Our AUV mapping method is less precise than pressure benchmark data but measures the deformation pattern over a larger, spatially continuous area.