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dc.contributor.authorMann, Ingrid
dc.contributor.authorGunnarsdottir, Tinna
dc.contributor.authorHäggström, Ingemar
dc.contributor.authorEren, Saliha
dc.contributor.authorTjulin, Anders
dc.contributor.authorMyrvang, Margaretha
dc.contributor.authorRietveld, Mike T
dc.contributor.authorDalin, Peter
dc.contributor.authorJozwicki, Dorota
dc.contributor.authorTrollvik, Henriette Marie Tveitnes
dc.date.accessioned2019-09-16T12:25:56Z
dc.date.available2019-09-16T12:25:56Z
dc.date.issued2019-06-17
dc.description.abstractWe discuss the influence of charged dust on radar observations in the Earth ionosphere. This region in the upper Earth atmosphere can be described as a partially ionized, low‐temperature plasma. Plasma parameters vary by orders of magnitude spatially and in time. Dust particles influence the charge balance, in some cases dusty plasma condition is met. The polar mesospheric echoes are an example of dust plasma interactions observed with radar. The mesosphere is a region where atmospheric temperature decreases with altitude and can reach frost point temperature. The formation of the polar mesospheric radar echoes involves neutral atmosphere dynamics, which is latitude dependent and it involves charged dust particles, especially icy dust that forms in the polar summer mesosphere. Charged dust can also influence incoherent scatter that results from electromagnetic waves scattering off electrons, where the electrons are coupled to other charged components. Observers rarely report charged dust signatures in the incoherent scatter spectra; we show that there is a good chance for doing so with improved observations. The incoherent scatter can possibly also be used to estimate the amount of charged dust in the direct vicinity of a meteor, as we show based on the order of magnitude considerations. This prospect of new observational results makes theoretical investigations of radio‐wave scattering in the presence of charged dust with size distributions worthwhile.en_US
dc.descriptionSource at <a href=https://doi.org/10.1002/ctpp.201900005>https://doi.org/10.1002/ctpp.201900005</a>.en_US
dc.identifier.citationMann, I., Gunnarsdottir, T., Häggström, I., Eren, S., Tjulin, A., Myrvang, M., ... Trollvik, H. (2019). Radar studies of ionospheric dusty plasma phenomena. <i>Contributions to Plasma Physics, 59</i>(6), e201900005. https://doi.org/10.1002/ctpp.201900005en_US
dc.identifier.cristinIDFRIDAID 1682551
dc.identifier.doi10.1002/ctpp.201900005
dc.identifier.issn0863-1042
dc.identifier.issn1521-3986
dc.identifier.urihttps://hdl.handle.net/10037/16205
dc.language.isoengen_US
dc.publisherWileyen_US
dc.relation.journalContributions to Plasma Physics
dc.relation.projectIDinfo:eu-repo/grantAgreement/RCN/FRINATEK/275503/Norway/Mesospheric Dust in the Small Size Limit: Radar Studies, Model Calculations and Supporting Observations//en_US
dc.rights.accessRightsopenAccessen_US
dc.subjectVDP::Mathematics and natural science: 400::Physics: 430::Astrophysics, astronomy: 438en_US
dc.subjectVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Astrofysikk, astronomi: 438en_US
dc.subjectdusty plasmaen_US
dc.subjectincoherent scatteren_US
dc.subjectionospheric physicsen_US
dc.subjectnanoparticlesen_US
dc.subjectradar observationsen_US
dc.titleRadar studies of ionospheric dusty plasma phenomenaen_US
dc.typeJournal articleen_US
dc.typeTidsskriftartikkelen_US
dc.typePeer revieweden_US


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