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dc.contributor.authorTsepelev, I.en
dc.contributor.authorIsmail-Zadeh, A.en
dc.contributor.authorStarodubtseva, Y.en
dc.contributor.authorKorotkii, A.en
dc.contributor.authorMelnik, O.en
dc.date.accessioned2021-08-31T15:09:14Z-
dc.date.available2021-08-31T15:09:14Z-
dc.date.issued2019-
dc.identifier.citation“Crust development inferred from numerical models of lava flow and its surface thermal measurements„ / I. Tsepelev, A. Ismail-Zadeh, Y. Starodubtseva, et al. — DOI 10.4401/ag-7745 // Annals of Geophysics. — 2019. — Vol. 62. — Iss. 2. — P. 1-17. — VO226.en
dc.identifier.issn15935213-
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access, Gold3
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85094904153&doi=10.4401%2fag-7745&partnerID=40&md5=c19324d5bdc7ef936be1856112b500f0
dc.identifier.otherhttps://www.annalsofgeophysics.eu/index.php/annals/article/download/7745/7127m
dc.identifier.urihttp://elar.urfu.ru/handle/10995/103360-
dc.description.abstractPropagation of a lava flow is governed by slope topography, magma rheology, heat exchange with the atmosphere and the underlying ter− rain, and the rate of the eruption. Highly viscous crust is formed due to cooling and solidification of the uppermost layer of the flow. We consider here two numerical model problems for lava flows, both based on the fundamental physics of a hot fluid flow: a model problem, where thermal conditions (e.g. temperature and heat flow) at the lava surface are unknown a priori (a direct model problem), and a model problem, where the lava surface conditions are known and determined from observations (an inverse model problem). In both models, the lava viscosity depends on temperature and the volume fraction of crystals. By way of solving the direct model problem, we perform a para− metric study of steady state lava flows to investigate the influence of the heat flux, viscosity, and effusion rate on the lava crust devel− opment. Numerical experiments show that a lava crust becomes thicker in the case of the nonlinear heat transfer compared to the case of a linear heat flow at the interface of lava with the atmosphere. Also, the crust thickens at lower lava effusion rates, while higher rates re− sult in a rapid lava advection, slower cooling, and development of a thinner crust. Moreover, a lava crust becomes thicker with a higher coefficient of conductive heat transfer, or a higher lava viscosity, or the growth of effective emissivity of the lava surface. By way of solv− ing the inverse model problem, we use an assimilation technique (that is, a method for an optimal combination of a numerical model of lava flows with observations) to propagate the temperature and heat flow, inferred from measurements at the interface between lava and the atmosphere, into the lava flow interior and to analyse the evolving lava crust. Results of thermal data assimilation illustrate that the physical parameters of lava flows, including the thickness of it crust, can be recovered from measured surface thermal data well enough at least for slow effusion rates. © 2019 the Istituto Nazionale di Geofisica e Vulcanologia. All rights reserved.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherEditrice Compositori s.r.l.en
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceAnn. Geophys.2
dc.sourceAnnals of Geophysicsen
dc.subjectDATA ASSIMILATIONen
dc.subjectLAVA CRUSTen
dc.subjectLAVA RHEOLOGYen
dc.subjectNONLINEAR HEAT FLUXen
dc.subjectNUMERICAL MODELLINGen
dc.subjectCRUSTen
dc.subjectDATA ASSIMILATIONen
dc.subjectFLOW MODELINGen
dc.subjectHEAT FLOWen
dc.subjectHEAT FLUXen
dc.subjectHEAT TRANSFERen
dc.subjectLAVA FLOWen
dc.subjectNUMERICAL MODELen
dc.subjectRHEOLOGYen
dc.subjectTEMPERATUREen
dc.subjectVOLCANIC ERUPTIONen
dc.title“Crust development inferred from numerical models of lava flow and its surface thermal measurements„en
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.4401/ag-7745-
dc.identifier.scopus85094904153-
local.contributor.employeeTsepelev, I., Institute of Mathematics and Mechanics, Ural Branch of the Russian Academy of Sciences, Yekaterinburg, Russian Federation
local.contributor.employeeIsmail-Zadeh, A., Institute of Applied Geosciences, Karlsruhe Institute of Technology, Karlsruhe, Germany, Institute of Earthquake Prediction Theory and Mathematical Geophysics, Russian Academy of Sciences, Moscow, Russian Federation
local.contributor.employeeStarodubtseva, Y., Institute of Mathematics and Mechanics, Ural Branch of the Russian Academy of Sciences, Yekaterinburg, Russian Federation
local.contributor.employeeKorotkii, A., Institute of Mathematics and Mechanics, Ural Branch of the Russian Academy of Sciences, Yekaterinburg, Russian Federation, Institute of Natural Sciences and Mathematics, Ural Federal University, Yekaterinburg, Russian Federation
local.contributor.employeeMelnik, O., Institute of Mechanics, Lomonosov Moscow State University, Moscow, Russian Federation
local.description.firstpage1-
local.description.lastpage17-
local.issue2-
local.volume62-
dc.identifier.wos000500751200001-
local.contributor.departmentInstitute of Mathematics and Mechanics, Ural Branch of the Russian Academy of Sciences, Yekaterinburg, Russian Federation
local.contributor.departmentInstitute of Applied Geosciences, Karlsruhe Institute of Technology, Karlsruhe, Germany
local.contributor.departmentInstitute of Earthquake Prediction Theory and Mathematical Geophysics, Russian Academy of Sciences, Moscow, Russian Federation
local.contributor.departmentInstitute of Natural Sciences and Mathematics, Ural Federal University, Yekaterinburg, Russian Federation
local.contributor.departmentInstitute of Mechanics, Lomonosov Moscow State University, Moscow, Russian Federation
local.identifier.pure11121983-
local.description.orderVO226-
local.identifier.eid2-s2.0-85094904153-
local.identifier.wosWOS:000500751200001-
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