S. Calvari et H. Pinkerton, FORMATION OF LAVA TUBES AND EXTENSIVE FLOW-FIELD DURING THE 1991-1993ERUPTION OF MOUNT-ETNA, J GEO R-SOL, 103(B11), 1998, pp. 27291-27301
Detailed mapping during the 1991-1993 eruption of Mount Etna has shown
that there is a relationship between tumuli, ephemeral vents, lava tu
bes, and their parent lava flows. During this eruption, many tubes for
med in stationary, inflated 'a'a lava flows. Ephemeral vents at the fr
onts of these stationary flows and above lava tubes fed secondary lava
flows, many of which subsequently developed new tubes. The resulting
complex network of tubes, ephemeral vents, and secondary flows was res
ponsible for most of the widening, thickening, and lengthening of the
1991-1993 Etna lava flow field. The supply of relatively uncooled lava
via tubes to distal parts of this flow field allowed lava to flow 3 k
m farther from the vent than the longest channel-fed lava flow. Our ob
servations suggest that lava tubes play a more important role in the f
ormation of extensive 'a'a flow fields on Etna than has previously bee
n recognized.