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dc.contributor.authorVorobeva, Ekaterina
dc.contributor.authorDe Carlo, Marine
dc.contributor.authorLe Pichon, Alexis
dc.contributor.authorEspy, Patrick Joseph
dc.contributor.authorNäsholm, Sven Peter
dc.date.accessioned2021-09-16T07:10:52Z
dc.date.available2021-09-16T07:10:52Z
dc.date.created2021-06-12T13:10:47Z
dc.date.issued2021
dc.identifier.citationAnnales Geophysicae. 2021, 39 (3), 515-531.en_US
dc.identifier.issn0992-7689
dc.identifier.urihttps://hdl.handle.net/11250/2778451
dc.description.abstractThis study investigates the use of a vespagram-based approach as a tool for multi-directional comparison between simulated microbarom soundscapes and infrasound data recorded at ground-based array stations. Data recorded at the IS37 station in northern Norway during 2014–2019 have been processed to generate vespagrams (velocity spectral analysis) for five frequency bands between 0.1 and 0.6 Hz. The back azimuth resolution between the vespagram and the microbarom model is harmonized by smoothing the modeled soundscapes along the back azimuth axis with a kernel corresponding to the frequency-dependent array resolution. An estimate of similarity between the output of the microbarom radiation and propagation model and infrasound observations is then generated based on the image-processing approach of the mean square difference. The analysis reveals that vespagrams can monitor seasonal variations in the microbarom azimuthal distribution, amplitude, and frequency, as well as changes during sudden stratospheric warming events. The vespagram-based approach is computationally inexpensive, can uncover microbarom source variability, and has the potential for near-real-time stratospheric diagnostics and atmospheric model assessment.en_US
dc.language.isoengen_US
dc.publisherCopernicus Publicationsen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleBenchmarking microbarom radiation and propagation model against infrasound recordings: a vespagram-based approachen_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.source.pagenumber515-531en_US
dc.source.volume39en_US
dc.source.journalAnnales Geophysicaeen_US
dc.source.issue3en_US
dc.identifier.doihttps://doi.org/10.5194/angeo-39-515-2021
dc.identifier.cristin1915402
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1


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