Journal
GEOPHYSICAL JOURNAL INTERNATIONAL
Volume 205, Issue 1, Pages 122-133Publisher
OXFORD UNIV PRESS
DOI: 10.1093/gji/ggv557
Keywords
Effusive volcanism; Lava rheology and morphology; Eruption mechanisms and flow emplacement; Remote sensing of volcanoes
Categories
Funding
- project MEDiterranean SUpersite Volcanoes (MED-SUV), an FP7 [ENV.2012.6.4-2 Call]
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Remote sensing thermal data of active lava flows allow the evaluation of effusion rates. This is made possible by a simple formula relating the lava effusion rate to the heat flux radiated per unit time from the surface of the flow. Due to the assumptions of the model, this formula implies that heat flux, surface temperature and lava temperature vary as a function of the flow thickness. These relationships, never verified or validated before, have been used by several authors as a proof of the weakness of the model. Here, multispectral infrared and visible imaging spectrometer (MIVIS) high spatial resolution (5-10 m) thermal data acquired during Etna's 2001 eruption were used to investigate downflow heat flux variations in the lava flow emitted from a vent located at 2100 m a.s.l. A high correlation between the downflow heat flux and the lava flow thickness (measured from a pre-existing digital elevation model) was found. Topography beneath the flow appears to play an important role both in lava emplacement mechanisms and flow dynamics. MIVIS-derived downflow effusion rates are consistent with the law of conservation of mass assessing the reliability of remote sensing techniques.
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