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Report on Ulawun (Papua New Guinea) — September 1993


Ulawun

Bulletin of the Global Volcanism Network, vol. 18, no. 9 (September 1993)
Managing Editor: Edward Venzke.

Ulawun (Papua New Guinea) Vapor emissions; slight increase in seismicity

Please cite this report as:

Global Volcanism Program, 1993. Report on Ulawun (Papua New Guinea) (Venzke, E., ed.). Bulletin of the Global Volcanism Network, 18:9. Smithsonian Institution. https://doi.org/10.5479/si.GVP.BGVN199309-252120



Ulawun

Papua New Guinea

5.05°S, 151.33°E; summit elev. 2334 m

All times are local (unless otherwise noted)


"Visual activity continued to remain at low levels during June, July, August, and September. Emissions consisted of weak-to-moderate white vapour from June through August, with occasional white/blue vapour in June, August, and September. The RSAM seismic monitor showed an increase in activity for some short periods in July. It was not possible to confirm these observations from the conventional seismograph due to severe radio interference. The few records that were readable appeared to show low-frequency events or short bursts of tremor at times consistent with the RSAM observations. Seismic activity was low in June, August, and September."

Geological Summary. The symmetrical basaltic-to-andesitic Ulawun stratovolcano is the highest volcano of the Bismarck arc, and one of Papua New Guinea's most frequently active. The volcano, also known as the Father, rises above the N coast of the island of New Britain across a low saddle NE of Bamus volcano, the South Son. The upper 1,000 m is unvegetated. A prominent E-W escarpment on the south may be the result of large-scale slumping. Satellitic cones occupy the NW and E flanks. A steep-walled valley cuts the NW side, and a flank lava-flow complex lies to the south of this valley. Historical eruptions date back to the beginning of the 18th century. Twentieth-century eruptions were mildly explosive until 1967, but after 1970 several larger eruptions produced lava flows and basaltic pyroclastic flows, greatly modifying the summit crater.

Information Contacts: C. McKee, N. Lauer, L. Sipison, B. Talai, R. Stewart, and D. Lolok, RVO.