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  5. Lava tube morphology on Etna and evidence for lava flow emplacement mechanisms
 
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Lava tube morphology on Etna and evidence for lava flow emplacement mechanisms

Author(s)
Calvari, S.  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione OE, Catania, Italia  
Pinkerton, H.  
Lancaster University  
Language
English
Obiettivo Specifico
1.5. TTC - Sorveglianza dell'attività eruttiva dei vulcani
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Journal
Journal of Volcanology and Geothermal Research  
Issue/vol(year)
/90(1999)
Pages (printed)
263-280
Date Issued
1999
URI
https://www.earth-prints.org/handle/2122/3144
Subjects
04. Solid Earth::04.08. Volcanology::04.08.06. Volcano monitoring  
Subjects

Mount Etna

lava tube

Abstract
Lava tubes play a pivotal role in the formation of many lava flow fields. A detailed examination of several compound
‘a‘a lava flow fields on Etna confirmed that a complex network of tubes forms at successively higher levels within the flow
field, and that tubes generally advance by processes that include flow inflation and tube coalescence. Flow inflation is
commonly followed by the formation of major, first-order ephemeral vents which, in turn, form an arterial tube network.
Tube coalescence occurs when lava breaks through the roof or wall of an older lava tube; this can result in the unexpected
appearance of vents several kilometers downstream. A close examination of underground features allowed us to distinguish
between ephemeral vent formation and tube coalescence, both of which are responsible for abrupt changes in level or flow
direction of lava within tubes on Etna. Ephemeral vent formation on the surface is frequently recorded underground by a
marked increase in size of the tube immediately upstream of these vents. When the lining of an inflated tube has collapsed,
‘a‘a clinker is commonly seen in the roof and walls of the tube, and this is used to infer that inflation has taken place in the
distal part of an ‘a‘a lava flow. Tube coalescence is recognised either from the compound shape of tube sections, or from
breached levees, lava falls, inclined grooves or other structures on the walls and roof. Our observations confirm the
importance of lava tubes in the evolution of extensive pahoehoe and ‘a‘a flow fields on Etna.
Sponsors
grant from the commission of the European Communities under the Fourth Framework Programme, Environment and Climate, Contract ENV4-CT97-0713.
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