Etna eruption update: 22 November 2006

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Summit eruption continues at Mount Etna
Istituto Nazionale di Geofisica e Vulcanologia ? Sezione di Catania
From: Boris Behncke (behncke@xxxxxxxxxx) and Sonia Calvari (calvari@xxxxxxxxxx)
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(All times are in GMT)


Episodic eruptive activity continued at the Southeast Crater of Etna (SEC) 
through late November 2006, involving a number of explosive and effusive vents 
on and around the SEC cone. At the same time, constant lava effusion continued 
from a short fissure at 2800 m elevation on the upper ESE flank (the western 
headwall of the Valle del Bove), contributing to the growth of a complex lava 
field up to 3 km long. One particularly violent episode on 16 November 
culminated with the fracturing and piecemeal collapse of the SSE flank of the 
SEC cone, accompanied by explosions, rockfalls, steam and rock debris.

The following is from Boris Behncke and Sonia Calvari and is based on daily 
observations by numerous individuals of the INGV staff (see www.ct.ingv.it for 
reports in Italian, updates and individual authorships).


Following one week of intermittent ash emissions and weak Strombolian activity 
on late 4 November, a new strong eruptive episode (the 10th since late August 
2006) started at the SEC summit vent at 2004 on 5 November and continued with 
some fluctuations and intermittent ash emissions for the next 9.5 hours. Light 
ash falls occurred over populated areas to the SE. At about 21.47 on the 5th, 
the effusion rate increased at a vent at 3050 m altitude at the southern base 
of the central summit cone (herafter named ?3050 m vent?), which had been 
continuously active since 27 October. A new lobe of lava traveled across the 
flat area south of Etna?s summit cone complex (known as the Cratere del Piano). 
An apparent increase in the effusion rate was also noted at the effusive 
fissure at 2800 m on the ESE flank (hereafter named ?2800 m vent?), with active 
lava lobes extending downslope. Lava effusion from the 3050 vent ended during 
the forenoon of 6 November, and for the following 48 hours, lava emission 
continued only at the 2800 vent.
The next (11th) eruptive episode at the SEC occurred on 8 November. Ash 
emissions from the summit of the SEC were followed by vigorous Strombolian 
activity that continued until approximately 2200. Around 1600, lava started to 
flow from a new vent located in the saddle between the SEC cone and the 
adjacent main summit cone, at an elevation of ~3180 m (hereafter referred to 
as ?3180 m vent?). The lava reached the SW base of the SEC cone in a few 
minutes where it bifurcated into several short lobes, the largest and 
westernmost lobe stopping at the E margin of the lava flow field from the 3050 
m vent. Lava from the 3180 m vent had ceased flowing by ~1845 whereas 
spattering and lava effusion continued at the 3050 m vent for some time; 
spattering ended at that vent around 1930 but lava continued to flow for 
another 24 hours.

Eruptive episode #12 from the SEC started at 2100 on 10 November, when the 
volcanic tremor amplitude showed a rapid increase. Bad weather hampered visual 
observations until 11 November, when it became evident that this episode had 
repeated in much detail its predecessor, with lava emission occurring from both 
the 3050 m and 3180 m vents. Strombolian activity from the SEC summit ceased at 
1100 on 11 November. Lava emission from the 3050 m vent continued until the 
following night, and the associated lava flow field grew mainly on its W side, 
with flow fronts descending to ~2800 m. For the next five days, lava emission 
continued unabated from the 2800 m vent, whereas the SEC and all other vents 
remained inactive.

Following a sharp increase in volcanic tremor amplitude at 0500 on 16 November, 
vigorous ash emissions started at the SEC summit at 0507 and were gradually 
replaced by intense Strombolian bursts, marking the onset of eruptive episode 
#13. Very early during this episode, lava issued from the 3180 m vent, forming 
a lobe about 100 m long before activity at this vent ceased. Lava effusion from 
the summit started at 0615 and triggered a series of rockfalls down the SE 
flank of the SEC cone, before the lava descended on the same flank. At 0626, 
brownish ash was emitted from a spot next to the effusive vent, and major 
rockfalls and avalanches started shortly thereafter. These originated at the S 
rim of what remained of the 2004-2005 collapse pit on the E flank of the SEC. 
Plumes rising from the descending avalanches contained both brownish ash and 
white steam. Avalanching was most intense between 0631 and 0640, after which 
the new lava flow rapidly descended the lower SE flank of the cone and began to 
extend beyond its base toward the area of the 2800 m vent. At the same time, 
strong emissions of black ash marked the opening of another explosive vent next 
to the summit, and a third explosive vent became active in the same area. For 
the next several hours, the vents continued to eject ash and occasionally 
bombs, and to produce vigorous Strombolian activity.

At 0700 emissons of white vapor occurred from the SE flank of the SEC cone; a 
few minutes later large rock avalanches started to descend that flank. 
Simultaneously a fissure began to cut from near the summit downslope on the SSE 
flank, triggering rockfalls and dust avalanches also on that side of the cone. 
This fissure initially propagated approximately 100 m downslope and then 
temporarily stopped, before it propagated another 150 m downslope at 0720. 
During the following 15 minutes, another fissure perpendicular to the earlier 
one cut SE-ward across the flank, generating more rockfalls and dust 
avalanches. The resulting fissure system had the form of an inverted Y 
delimiting a block that was actively pushed outward by magma intruding into the 
flank of the cone.

Lava began to issue from the lower end of the W branch of the fissure system at 
about 0810. At approximately the same time, the 3050 m vent started to emit 
lava. By this time, the upper portion of the fissure cutting the SSE flank of 
the SEC cone had significantly enlarged and become a deep trench. Dense volumes 
of steam were emitted from this trench at 0831 and were followed a few minutes 
later by another series of rockfalls and avalanches. Direct observation from 
~0.7 km distance showed that the most energetic of these avalanches resulted 
from the collapse of low fountains of gas and tephra that occurred at the lower 
end of the large trench. The avalanches and rockfalls lasted approximately 15 
minutes, then a voluminous surge of lava issued from the lower end of the 
opening trench.

Over the next few hours this sequence of events (vapor emission ? rockfalls and 
avalanches ? lava emission) was repeated several times as the trench widened 
and propagated further downslope. During the few moments when steam and dust 
clouds cleared and the interior of the trench became visible, a cascade of very 
fluid lava was seen in the center of the trench. Apparently, the lava issued 
from a source high in the head wall of the trench, and at times spurted from 
the vent like a firehose.

At 1100, white steam plumes, rockfalls and dust avalanches appeared high on the 
SE flank of the SEC cone, in the area where the summit lava flow was emitted. 
These phenomena marked a major collapse of the eastern wall of the trench, 
which eventually cut into the descending summit lava flow, diverting it from 
its original course into the trench. The original flow, which had descended 
immediately S of the 2800 m vent down to ~2600 m elevation, rapidly stopped, 
although lava continued to drain from the main flow channel and accumulated in 
a thickening lobe at the base of the cone.

A series of events started at approximately 1425 with several vertical jets of 
black tephra that shot upward. These emissions occurred at ~150 m distance from 
the base of the cone and were very distinct in color from the brownish dust 
clouds which at the same time descended from the trench. The activity at the 
new site appeared to migrate rapidly both toward the SEC as dark plumes began 
to rise closer to the cone, while a ground-hugging plume of white vapor shot in 
the opposite direction. A few tens of seconds later, very dense clouds of dark 
brown material began to appear at the base of the surging white cloud and 
formed a distinct flow that rapidly overtook the front of the white cloud while 
speeding toward SE. At the slope break that forms the W rim of the Valle del 
Bove (~2800 m) both clouds disappeared from view in weather clouds, but at the 
site where the activity had originated, a huge plume of white vapor soared 
skyward. White vapor continued to rise from the area and from the path of the 
white and dark brown clouds for more than 15 minutes.

Another explosive emission of white steam and dark brown plumes occurred at 
~1455 from a spot still farther away from the. Like the 1425 event, it 
generated ground-hugging clouds of steam and dark brown material, the latter 
again travelling faster than the earlier. During the following hours, the 
activity at the SEC gradually decreased, with several spectacular cascades of 
lava descending through the trench on the SSE side of the cone. Steam 
explosions and rock avalanches occurred at the lower termination of the trench 
at 1525. Strombolian activity ceased at 1500, but lava emission continued into 
the night. This lava does not seem to have extended far from the base of the 
SEC cone, since investigation during the following day failed to reveal any 
fresh lava on top of the debris deposits emplaced during the major explosive 
events at 1425 and 1455. A minor lava flow was also fed from a new short 
fissure approximately 80 m E of the 3050 m vent. During the evening a small 
lobe of lava was emitted from the accumulation of lava the base of the SEC cone.

Fieldwork and aerial surveys during the following two days revealed that the 
1425 and 1455 explosions and related flows had left two main types of deposit. 
One was of lobate shape and extended a few hundred meters from the source of 
the explosions to the SE, covering a footpath that had been made by mountain 
guides to allow tourists to approach the persistently active 2800 m vent. On 
the ground the deposit consisted of very fine-grained reddish-brown ash made up 
almost exclusively of lithic fragments. Toward north the deposit gradually 
thickened and larger clasts were found on its surface, some of which 
represented fresh magmatic material. Close to the 2800 m vent, the deposit 
abruptly graded into a sort of debris flow rich in lithics but with up to 25% 
of fresh magmatic clasts. These latter showed a peculiar flattened-out 
morphology. Where this deposit overlay the tourist path near the 2800 vent it 
was 1.5-2 m thick. In one place the flow had entrained a plastic-coated sign 
warning tourists from leaving the path. The plastic showed no evidence of 
strong heating, so that it is assumed that the flow was cold in the moment when 
it arrived at that spot.

Volcanic tremor amplitude began to increase during the late afternoon of 18 
November, and during a helicopter flight at 1800 the 2800 m vent showed 
vigorous spattering. Active lava from the vent travelled ~3 km to Monte 
Centenari. Bright incandescence was also noted within the 3180 m vent during 
this overflight.

At 0400 on 19 November, episode #14 started from the SEC. Strombolian activity 
occurred from 2 vents at the summit while lava flowed through the 16 November 
trench and divided into numerous braiding lobes on top of the debris deposit 
emplaced 3 days earlier. The longest lobe travelled along the prominent channel 
in the main debris flow, passing immediately to the S of the 2800 m vent and 
extending to ~2600 m elevation. This episode was much less violent than its 
predecessor and lacked the explosions, surges and flows characteristic of that 
event. Strombolian activity continued until the late evening, while lava 
effusion ended early on 20 November. As during previous episodes, lava had also 
briefly issued from the 3050 m and 3180 m vents. In addition, a few meters long 
flow started from another fissure that opened at about 3200 m, on the saddle 
between Bocca Nuova and SEC. This upper flow merged with the flow coming out 
from the 3180 m vent.

The 15th eruptive episode at the SEC started at 1200 on 21 November. Direct 
observations were rendered impossible by inclement weather through nightfall, 
but at ~1500 a black ash plume was seen rising above the cloud cover to 
approximately 1.5 km above the summit. Light ash falls occurred along the 
Ionian coast near Giarre and further north, while at Rifugio Citelli (~6 km NE 
of the SEC), the ash deposit was nearly continuous. After 1900, the cloud cover 
gradually opened, allowing direct views of the strong Strombolian explosions 
generating jets sometimes >300 m high. Lava once more flowed through the 16 
November trench on the SSE flank of the cone toward the 2800 m vent. Likewise, 
the 3050 m and 3180 m vents had reactivated, although the latter had apparently 
ceased erupting early during the episode. Lava flowed from the trench until 
shortly after midnight on 22 November. Bad weather precluded further 
observations until the evening of that day, when all activity was again limited 
to the 2800 vent.

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Dr. Sonia Calvari
Istituto Nazionale di Geofisica e Vulcanologia
Sezione di Catania
Piazza Roma 2
95123 Catania (Italy)
Tel. +39 095 7165800 direct: +39 095 7165862
Fax: +39 095 435801 url: www.ct.ingv.it
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