Conduit pre-charge during repeated Plinian eruptions at Sakurajima volcano

Monday, 14 December 2020: 16:00
Virtual
Naoki Araya1, Michihiko Nakamura2, Atsushi Yasuda3, Satoshi Okumura2, Tomoki Sato4, Daisuke Miki5, Masato Iguchi6 and Nobuo Geshi7, (1)Tohoku University, Sendai, Japan, (2)Tohoku University, Department of Earth Science, Sendai, Japan, (3)Univ Tokyo, Tokyo, Japan, (4)JAMSTEC Japan Agency for Marine-Earth Science and Technology, Kanagawa, Japan, (5)Kyoto University, Sakurajima Volcano Research Center, Disaster Prevention Research Institute, Kyoto, Japan, (6)Kyoto University, Kyoto, Japan, (7)Geological Survey of Japan, Tsukuba, Japan
Abstract:
Understanding the magmatic conditions before the historic Plinian eruptions at the Sakurajima volcano (AD 1471, 1779, and 1914) is crucial to assess future eruption risks. We determined the depth of the pre-eruptive magma storage based on the volatile content in the phenocryst-hosted melt inclusions and in the groundmass glass that was equilibrated with plagioclase rims. The water content of the melt inclusions, determined by FT-IR reflectance spectroscopy (Yasuda, 2014), was 1.4–3.5 wt%, consistent with the estimates based on the plagioclase-melt hygrometer model of Waters and Lange (2015). The CO2 content of the inclusions was 29 ppm at maximum but mostly below the detection limit (~10 ppm). Assuming volatile saturation, we estimated the magma storage depths just before the historic Plinian eruptions to be 0.9–3.2 km. This depth is even shallower than the uppermost magma reservoir located beneath the Sakurajima volcano, as estimated using geodetic and seismological observations (Iguchi et al., 2013). We conclude that before every Plinian eruption, the Plinian magmas were fed from a shallow and thick conduit that was pre-charged from deeper reservoirs. This process may require the widening of the dike-shaped conduit, preserving the possibility that significant precursory phenomena could be detected before forming an eruption column. On the other hand, the magma could reach the surface quickly from the shallow conduit. Moreover, a thick dike-shaped conduit enables a high magma discharge rate (Costa et al., 2009), thereby facilitating vigorous explosive eruptions.