102nd Annual Meeting of the Cordilleran Section, GSA, 81st Annual Meeting of the Pacific Section, AAPG, and the Western Regional Meeting of the Alaska Section, SPE (8–10 May 2006)

Paper No. 5
Presentation Time: 9:20 AM

THE ROLE OF REMOTE SENSING IN MONITORING OF AUGUSTINE VOLCANO


WEBLEY, Peter1, DEAN, Ken2, DEHN, Jon2, BAILEY, John1, SCHNEIDER, Dave3, WESSELS, Rick3, LOVICK, Joseph2, RINKLEFF, Peter2 and IZBEKOV, Pavel2, (1)Arctic Region Super Computing Centre (ARSC), University of Alaska Fairbanks (UAF), 909 Koyukuk Drive, Fairbanks, AK 99775, (2)Geophysical Institute, University of Alaska Fairbanks, Fairbanks, AK 99775, (3)Alaska Volcano Observatory, U.S. Geological Survey, Anchorage, AK 99508, pwebley@gi.alaska.edu

Augustine Volcano erupted explosively starting on 11 January 2006 and over the next few weeks many more events followed disrupting air traffic throughout the region. Satellite data were used to detect and monitor surface and airborne components of the eruption. Augustine Volcano is located in the Lower Cook Inlet, 275 km (171 miles) SW of Anchorage, Alaska. It is situated at 59.36 N, 153.43 W and has an elevation of 1260m (4134ft). Volcanic activity is routinely monitored throughout the North Pacific Region as part of the Alaska Volcano Observatory project. Augustine became seismically active with subtle ground inflation starting in May 2005. On 12 December a 75 km long, low level gas plume was observed blowing to the SE. Airborne thermal imaging detected increased surface heating in early January. The volcano erupted multiple times between 11 - 28 January sending ash clouds up to 40,000 feet. The 13th and 14th eruptions consisted of six separate events resulting in 6 simultaneously drifting ash clouds in the Alaska region. From 28 January to 4 February the volcano was in a state of continuous eruption. After this period, activity decreased. Pyroclastic flows and lahars occurred throughout the eruption. A light ash fall was observed at many locations in the region. This presentation will focus primarily on the detection and analysis of volcanic clouds and thermal anomalies observed on satellite data. Data from three groups of satellites: GOES, AVHRR and MODIS were analyzed using visible and infrared wavelengths from time sequential data sets. Animations showing the dispersion of the ash clouds were simulated using the Puff model and compared to ground based instruments and ash fall observations. Changes in the temperature and morphology of thermal anomalies are related to heating of the dome, pyroclastic flows and lahars.