Night-time satellite imagery from 8 November of the eruption that began on 3 November near Dalaffilla and Alu volcanoes revealed a multi-lobed lava-flow field with a primary channelized flow that traveled NE. The source appears to be a one or more NW-SE-trending eruptive fissures NW of Dalaffilla. The flow field on the 8 November image was an estimated 9.3 km long and 3 km wide, with an area of about 15 square kilometers. Thermal anomalies detected by satellites were present during 12-16 November.

Geological Summary. The summit region of Alu, ~5 km NW of the Dalafilla stratovolcano, is an ellipsoidal volcanic horst, elongated NNW-SSE, and formed primarily of older basaltic lava flows. Recent fractures along the axis of the Erta Ale range cut the main horst of Alu and areas to the SSE. Fumarolic activity is located on the numerous parallel faults. Fissure vents west of the horst have fed silicic lava flows, and voluminous youthful basaltic lava flows to the east extend north as far as Lake Bakili. Dalafilla, also referred to as Gabuli, is a steep-sided cone that rises 300 m above surrounding lava fields due to extrusion of viscous, silicic lava flows. Basaltic lava flows from regional fissures surround the volcano. Fumarolic activity occurs in the 100-m-wide summit crater and has weathered surrounding lava flows. The first historical eruption of Alu-Dalafilla took place in 2008, when lava flows from vents between the two edifices traveled NE.

Sources: Hawai'i Institute of Geophysics and Planetology (HIGP) Thermal Alerts Team, US Geological Survey Hawaiian Volcano Observatory (HVO), Simon Carn