2004
DOI: 10.1016/s0377-0273(03)00348-2
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Modeling of the steady-state temperature field in lava flow levées

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Cited by 16 publications
(16 citation statements)
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“…Lava heat is released in the atmosphere from the core of an active flow by conduction through the basal, lateral, and surface crusts [Oppenheimer, 1991;Klingelhofer et al, 1999;Quareni et al, 2004]. At the surface, heat losses are dominated by radiation (5 × 10 4 W m −2 ) and convection (10 4 W m −2 ), whereas conduction from the base to the ground is predominant (10 3 W m −2 [Harris et al, 2005]).…”
Section: Heat Flow Estimationmentioning
confidence: 99%
“…Lava heat is released in the atmosphere from the core of an active flow by conduction through the basal, lateral, and surface crusts [Oppenheimer, 1991;Klingelhofer et al, 1999;Quareni et al, 2004]. At the surface, heat losses are dominated by radiation (5 × 10 4 W m −2 ) and convection (10 4 W m −2 ), whereas conduction from the base to the ground is predominant (10 3 W m −2 [Harris et al, 2005]).…”
Section: Heat Flow Estimationmentioning
confidence: 99%
“…Such channeled flows leaving a levee‐channel morphology in deposits on the slope are also observed in very different environments and for flows involving completely different materials such as landslide deposits on Mars [ Mangold et al , 2003; Treiman and Louge , 2004] or submarine landslides [ Klaucke et al , 2004]. Although lava flows have a totally different mechanical behavior, similar morphological features are observed in their deposits [ Sakimoto and Gregg , 2001; Quareni et al , 2004].…”
Section: Introductionmentioning
confidence: 99%
“…Several explanations have been proposed for the channeling of these unconfined flows and their levee‐channel morphology: Bingham rheology leading to lateral static zones as is the case for lava flows [ Yamamoto et al , 1993; Quareni et al , 2004; Mangold et al , 2003], drainage of the central part of the deposit with static levees [ Rowley et al , 1981] and differential deflation and differential fluidization of borders during emplacement due to polydispersity of the particles [ Rowley et al , 1981; Wilson and Head , 1981]. The levee‐channel morphology observed on Martian landslides was first interpreted as indicating the presence of water during emplacement [ Malin and Edgett , 2000].…”
Section: Introductionmentioning
confidence: 99%
“…Pluton emplacement has been modelled as a large body of viscous fluid which plastically deforms its surroundings, and experiments have focussed on pluton geometry and how space is accommodated in the lithosphere. Perhaps one of the earliest analogue experiments to study granitic pluton emplacement was carried out by Ramberg (1970), who used a combination of clay, putties, wax-oil mixtures, plates of concrete, and aqueous solutions to simulate diapiric ascent of fluid-like magmas through rock layers with differing competency (see Tables 1 and 2). In his experiments, Ramberg used a centrifuge model arrangement capable of reaching an acceleration of 4000 × g. Roman-Berdiel et al (1997) and Roman-Berdiel (1999) studied granite emplacement by injecting low-viscosity Newtonian silicone putty into a tank of sand.…”
Section: Magma Chamber To Plutonmentioning
confidence: 99%
“…Lava flow numerical models have been used to simulate edifice growth from the accumulation of multiple lava flows (Annen et al, 2001), the insulating properties of lava tubes (Keszthelyi, 1995), cooling of pahoehoe lavas (Keszthelyi and Denlinger, 1996), and formation of lava levees (Quareni et al, 2004), and from a hazard perspective, flow length, rates of emplacement, and inundation areas. For hazard and risk assessment purposes, simulated lava flows are emplaced over a digital elevation model to predict the inundation pathways of flows.…”
Section: Application Of Numerical Lava Flow Modelsmentioning
confidence: 99%