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Methods for the Evaluation of the Stochastic Properties of the Ionosphere for Earthquake Prediction—Random Matrix Theory

dc.contributor.authorBřízová, Leontýna
dc.contributor.authorKříž, Jan
dc.contributor.authorStudnička, Filip
dc.contributor.authorŠlégr, Jan
dc.date.accessioned2019-10-17T07:27:44Z
dc.date.available2019-10-17T07:27:44Z
dc.date.issued2019
dc.description.abstractSeismo-ionospheric coupling is a field of great interest and is currently subject to rigorous study; using both ground and satellite data and many phenomenological features, the ionospheric precursors of earthquakes were identified. In this work, we present methods to study the stochastic properties of the lower ionosphere, derived from the data obtained with very low frequency (VLF) receivers at frequencies in the range of 19.6 to 37.5 kHz. Two main approaches are described: auto-correlation and random matrix theory treatments of amplitude time series data. It is shown that before shallow earthquakes with magnitudes greater than four, there are measurable changes that can be used in earthquake prediction. Although the exact form of the causal chain that leads to these changes are currently subject to diligent study, we believe that the investigations described herein are worth adding to the repertoire of ionospheric precursors.eng
dc.description.abstract-translatedSeismo-ionospheric coupling is a field of great interest and is currently subject to rigorous study; using both ground and satellite data and many phenomenological features, the ionospheric precursors of earthquakes were identified. In this work, we present methods to study the stochastic properties of the lower ionosphere, derived from the data obtained with very low frequency (VLF) receivers at frequencies in the range of 19.6 to 37.5 kHz. Two main approaches are described: auto-correlation and random matrix theory treatments of amplitude time series data. It is shown that before shallow earthquakes with magnitudes greater than four, there are measurable changes that can be used in earthquake prediction. Although the exact form of the causal chain that leads to these changes are currently subject to diligent study, we believe that the investigations described herein are worth adding to the repertoire of ionospheric precursors.cze
dc.formatp. 1-8
dc.identifier.doi10.3390/atmos10070413
dc.identifier.issn2073-4433
dc.identifier.obd43875291
dc.identifier.urihttp://hdl.handle.net/20.500.12603/56
dc.language.isoeng
dc.noteArticle Number: 413eng
dc.peerreviewedyes
dc.publicationstatuspostprint
dc.publisherMDPI-Molecular diversity preservation international
dc.relation.ispartofAtmosphere, volume 10, issue: 7eng
dc.rightsPráce není přístupnáeng
dc.subjectionospheric precursorseng
dc.subjectstochastic propertieseng
dc.subjectlower ionosphereeng
dc.subjectionosférické prekurzorycze
dc.subjectstochastické vlastnosticze
dc.subjectspodní ionosféracze
dc.titleMethods for the Evaluation of the Stochastic Properties of the Ionosphere for Earthquake Prediction—Random Matrix Theoryeng
dc.title.alternativeMetody pro hodnocení stochastických vlastností ionosféry pro předpověď zemětřesení - náhodná teorie maticcze
dc.typearticle

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