Real‐time data received from Mount Erebus Volcano, Antarctica

Internal and eruptive volcano processes involve complex interactions of multi‐phase fluids with the solid Earth and the atmosphere, and produce diverse geochemical, visible, thermal, elastic, and anelastic effects. Multidisciplinary experimental agendas are increasingly being employed to meet the challenge of understanding active volcanoes and their hazards [e.g., Ripepe et al. , 2002; Wallace et al. , 2003]. Mount Erebus is a large (3794 m) stratovolcano that forms the centerpiece of Ross Island, Antarctica, the site of the principal US. (McMurdo) and New Zealand (Scott) Antarctic bases. With an elevation of 3794 m and a volume of ∼1670 km 3 , Erebus offers exceptional opportunities for extended study of volcano processes because of its persistent, low‐level, strombolian activity (Volcano Explosivity Index 0–1) and exposed summit magma reservoir (manifested as a long‐lived phonolitic lava lake). Key scientific questions include linking conduit processes to near‐field deformations [e.g., Aster et al. , 2003] ,explosion physics [ e.g., Johnson et al. , 2003], magmatic differentiation and residence [e.g., Kyle et al. , 1992], and effects on Antarctic atmospheric and ice geochemistry [e.g., Zreda‐Gostynska et al. , 1997]. The close proximity of Erebus (35 km) to McMurdo, and its characteristic dry, windy, cold, and high‐elevation Antarctic environment, make the volcano a convenient test bed for the general development of volcano surveillance and other instrumentation under extreme conditions.