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dc.contributor.authorRäbinä, J.en
dc.contributor.authorMönkölä, S.en
dc.contributor.authorRossi, T.en
dc.contributor.authorMarkkanen, J.en
dc.contributor.authorGritsevich, M.en
dc.contributor.authorMuinonen, K.en
dc.date.accessioned2021-08-31T15:02:27Z-
dc.date.available2021-08-31T15:02:27Z-
dc.date.issued2016-
dc.identifier.citationControlled time integration for the numerical simulation of meteor radar reflections / J. Räbinä, S. Mönkölä, T. Rossi, et al. — DOI 10.1016/j.jqsrt.2016.02.009 // Journal of Quantitative Spectroscopy and Radiative Transfer. — 2016. — Vol. 178. — P. 295-305.en
dc.identifier.issn224073-
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access, Green3
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-84991383977&doi=10.1016%2fj.jqsrt.2016.02.009&partnerID=40&md5=04b71b19532f921fdeb3f881d17d2ea6
dc.identifier.otherhttps://jyx.jyu.fi/bitstream/123456789/49940/1/1s2.0s0022407315301254main.pdfm
dc.identifier.urihttp://elar.urfu.ru/handle/10995/102202-
dc.description.abstractWe model meteoroids entering the Earth[U+05F3]s atmosphere as objects surrounded by non-magnetized plasma, and consider efficient numerical simulation of radar reflections from meteors in the time domain. Instead of the widely used finite difference time domain method (FDTD), we use more generalized finite differences by applying the discrete exterior calculus (DEC) and non-uniform leapfrog-style time discretization. The computational domain is presented by convex polyhedral elements. The convergence of the time integration is accelerated by the exact controllability method. The numerical experiments show that our code is efficiently parallelized. The DEC approach is compared to the volume integral equation (VIE) method by numerical experiments. The result is that both methods are competitive in modelling non-magnetized plasma scattering. For demonstrating the simulation capabilities of the DEC approach, we present numerical experiments of radar reflections and vary parameters in a wide range. © 2016 Elsevier Ltd.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherElsevier Ltden
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceJ. Quant. Spectrosc. Radiat. Transf.2
dc.sourceJournal of Quantitative Spectroscopy and Radiative Transferen
dc.subjectDISCRETE EXTERIOR CALCULUSen
dc.subjectELECTROMAGNETIC SCATTERINGen
dc.subjectMETEORSen
dc.subjectPLASMATIC OBJECTSen
dc.subjectRADAR REFLECTIONSen
dc.subjectVOLUME INTEGRAL EQUATIONen
dc.subjectCALCULATIONSen
dc.subjectEARTH ATMOSPHEREen
dc.subjectFINITE DIFFERENCE TIME DOMAIN METHODen
dc.subjectINTEGRAL EQUATIONSen
dc.subjectMAGNETOPLASMAen
dc.subjectNUMERICAL METHODSen
dc.subjectNUMERICAL MODELSen
dc.subjectRADARen
dc.subjectRADAR REFLECTIONen
dc.subjectDISCRETE EXTERIOR CALCULUSen
dc.subjectELECTROMAGNETIC SCATTERINGen
dc.subjectMETEORSen
dc.subjectPLASMATIC OBJECTSen
dc.subjectVOLUME INTEGRAL EQUATIONen
dc.subjectTIME DOMAIN ANALYSISen
dc.subjectELECTROMAGNETIC METHODen
dc.subjectMETEORen
dc.subjectNUMERICAL METHODen
dc.subjectPLASMAen
dc.subjectRADARen
dc.subjectSCATTERINGen
dc.titleControlled time integration for the numerical simulation of meteor radar reflectionsen
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1016/j.jqsrt.2016.02.009-
dc.identifier.scopus84991383977-
local.contributor.employeeRäbinä, J., University of Jyvaskyla, Department of Mathematical Information Technology, University of Jyvaskyla, P.O. Box 35 (Agora)FI-40014, Finland
local.contributor.employeeMönkölä, S., University of Jyvaskyla, Department of Mathematical Information Technology, University of Jyvaskyla, P.O. Box 35 (Agora)FI-40014, Finland
local.contributor.employeeRossi, T., University of Jyvaskyla, Department of Mathematical Information Technology, University of Jyvaskyla, P.O. Box 35 (Agora)FI-40014, Finland
local.contributor.employeeMarkkanen, J., Department of Physics, University of Helsinki, P.O. Box 64FI-00014, Finland
local.contributor.employeeGritsevich, M., Finnish Geospatial Research Institute, P.O. Box 15, Masala, FI-02431, Finland, Dorodnicyn Computing Centre, Federal Research Center Computer Science and Control of the Russian Academy of Sciences, Moscow, 119333, Russian Federation, Institute of Physics and Technology, Ural Federal University, Ekaterinburg, 620002, Russian Federation
local.contributor.employeeMuinonen, K., Department of Physics, University of Helsinki, P.O. Box 64FI-00014, Finland, Finnish Geospatial Research Institute, P.O. Box 15, Masala, FI-02431, Finland
local.description.firstpage295-
local.description.lastpage305-
local.volume178-
local.contributor.departmentUniversity of Jyvaskyla, Department of Mathematical Information Technology, University of Jyvaskyla, P.O. Box 35 (Agora)FI-40014, Finland
local.contributor.departmentDepartment of Physics, University of Helsinki, P.O. Box 64FI-00014, Finland
local.contributor.departmentFinnish Geospatial Research Institute, P.O. Box 15, Masala, FI-02431, Finland
local.contributor.departmentDorodnicyn Computing Centre, Federal Research Center Computer Science and Control of the Russian Academy of Sciences, Moscow, 119333, Russian Federation
local.contributor.departmentInstitute of Physics and Technology, Ural Federal University, Ekaterinburg, 620002, Russian Federation
local.identifier.pure864732-
local.identifier.pureb633a486-0e7a-4310-a0ed-c71985e3766cuuid
local.identifier.eid2-s2.0-84991383977-
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