STROMBOLIAN ERUPTIONS

Strombolian eruptions are named from the small volcano-island of Stromboli (image), located between Sicily and Italy. This volcano has been erupting almost constantly for hundreds of years. It erupts irregularly every twenty minutes or so to produce an episodic lightshow that gives rise to it's nickname, the "Lighthouse of the Mediterranean".

The term "strombolian" has been used indiscriminately to describe a variety of volcanic eruptions that vary from small volcanic blasts, to kilometer-high eruptive columns. However, true strombolian activity is characterized by short-lived, explosive outbursts of pasty lava ejected a few tens or hundreds of meters into the air. Unlike Hawaiian eruptions, Strombolian eruptions never develop a sustained eruption column. They eject relatively viscous basaltic lava from the throat of the volcano. Build up of the high gas pressures required to fragment this somewhat pasty lava, results in episodic explosions with booming blasts. Although Strombolian eruptions are much noisier than Hawaiian eruptions, they are no more dangerous. As shown in the image here, Strombolian explosions eject bomb- and lapilli-sized fragments that travel in parabollic ballistic paths before accumulating around the vent to construct the volcanic edifice. Typically, these eruptions form scoria cones composed of basaltic pryoclasts. However, mafic stratovolcanoes can also exhibit common Strombolian activity, evident for example, at Mt Eberus in Antarctica and at Stromboli itself.

Pyroclastic particles like Pele's tears, Pele's hair, and reticulite, which are common in Hawaiian eruptions, are not present in Strombolian eruptions. Spatter-fed flows are minor. Instead, Strombolian eruptions are dominated by scoria fragments, which are highly vesiculated clasts of basalt with a cindery appearance. Tephra bombs and lapilli accumulate around the vent to produce well-bedded, and often well-sorted, scoria-fall deposits

In contrast to Hawaiian eruptions, true Strombolian eruptions produce little or no flowing lava. However, during the end stages of scoria-cone formation, it is not unusual for Strombolian activity to wane and give way to the calm extrusion of basaltic lava flows. As a general rule, a'a lava flows appear to be more common than the more fluid pahoehoe types. As the vesiculating lava is de-gased toward the end of the eruption, it may ooze out from under the volcanic edifice to produce a lava flow, or pond in the vent to produce a lava lake. This will only occur if the underlying basalt is fluid enough to flow, which has not proved to be the case at Stromboli itself.

THE STROMBOLIAN ERUPTION OF PARICUTIN

A classic example of a Strombolian-type eruption was the Paricutin eruption in 1943, about 200 miles west of Mexico City. This eruption marks the first time scientists were able to observe the complete life cycle of a volcano, from birth to extinction.

Three weeks before the Paricutin eruption occurred, the people near Paricutin village heard the rumbling noises that resembled thunder, yet they were confused because the skies were clear of clouds. The noises were associated with earthquakes at depth near Paricutin. On February 20, 1943 a farmer, Dionisio Pulido, and his wife were burning shrubbery in their cornfield when they observed the earth in front of them swell upward and crack to form a fissure 2-2.5 m across. They heard hissing sounds and later described the rise of "smoke" from the fissure, which had the repugnant smell of rotten eggs. The "rotten egg" smell is a hallmark of H2S gas, and the crack that opened in front of them was a fumarole.

Paricutin 1946	Paricutin 1944

Strombolian pyroclastic activity began at the site the following day and by the end of the day it generated a 40-m-high scoria cone. In one week it grew to a height of 100 m from the accumulation of bombs and lapilli, and it was raining down finer fragments that burned and eventually covered the village of Paricutin. The eruption was unusually long for a strombolian eruption, with several eruptive phases occurring over a 9-year period. After about two years of mostly pyroclastic activity the pyroclastic phase began to wane, and the outpouring of lava from the base of the cone became the dominant mode of eruption over the next 7 years. The eruption ceased in 1952. The final height of the scoria cone was 424 m.