2004
DOI: 10.1029/2003jb002537
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Numerical modeling of lava flow cooling applied to the 1997 Okmok eruption: Approach and analysis

Abstract: [1] Throughout February and March of 1997 Okmok Volcano, in the eastern Aleutian Islands of Alaska, erupted a 6 km long lava flow of basaltic 'a'a within its caldera. A numerical model for lava flow cooling was developed and applied to the flow to better understand the nature of its cooling. Radiation and convection from the surface, as well as conduction to the ground, were used to transport the flow's heat to its surroundings in the model. Internally, a conduction-only approach moved heat from the interior o… Show more

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Cited by 70 publications
(78 citation statements)
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References 59 publications
(119 reference statements)
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“…Radiative heat loss from the lava flow to the atmosphere is affected by air temperature, wind, and precipitation (e.g., Patrick et al 2004) but diminishes rapidly with decreasing temperature, typically in less time (minutes to hours) than it takes to emplace the flow. However, convective heat loss to the atmosphere continues throughout cooling (Neri 1998) and would lead to more rapid cooling of the lava.…”
mentioning
confidence: 99%
“…Radiative heat loss from the lava flow to the atmosphere is affected by air temperature, wind, and precipitation (e.g., Patrick et al 2004) but diminishes rapidly with decreasing temperature, typically in less time (minutes to hours) than it takes to emplace the flow. However, convective heat loss to the atmosphere continues throughout cooling (Neri 1998) and would lead to more rapid cooling of the lava.…”
mentioning
confidence: 99%
“…Keszthelyi and Denlinger, 1996;Wooster et al 1997;Cashman et al 1999;Patrick et al 2004;Kolzenburg et al 2016). Lava flows cool by thermal radiation and atmospheric convection from the surface and by conduction to the underlying country-rock (Keszthelyi and Denlinger, 1996;Neri, 1998;Patrick et al 2004).…”
Section: Discussionmentioning
confidence: 99%
“…where σ is the Stefan-Boltzmann constant (5.67051 × 10 −8 W/ m 2 /K 4 ), ε is the emissivity of the lava surface (assumed to be 0.95 for basalt; Patrick et al 2004), A flow is the final area of the cooling lava flow field (84 km 2 ; Pedersen et al 2017), and BT MIR,flow and BT MIR,bk are the average brightness temperatures of the flow surface pixels and surrounding background, respectively, calculated from selected MODIS-MIROVA cloud-free images (Fig. 6).…”
Section: Lava Flow Field Radiant Heat Fluxmentioning
confidence: 99%
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“…Lava flows can be centimetres to tens of metres thick (MacDonald, 1953), have emplacement temperatures of 800-1200°C (Kilburn, 2015) and can take weeks to months to cool to ambient temperatures (e.g., Patrick et al, 2004;Patrick et al, 2005). However, it is possible to get very close to active lava flows unharmed and unburnt, and in all but rare cases lava flows are slow enough to be outwalked (Blong, 1984).…”
Section: Lava Flowmentioning
confidence: 99%