On the role of anisotropic MF/HF scattering in mesospheric wind estimation

dc.bibliographicCitation.firstPage158
dc.bibliographicCitation.journalTitleEarth, planets and space : EPSeng
dc.bibliographicCitation.volume70
dc.contributor.authorRenkwitz, Toralf
dc.contributor.authorTsutsumi, Masaki
dc.contributor.authorLaskar, Fazlul I.
dc.contributor.authorChau, Jorge L.
dc.contributor.authorLatteck, Ralph
dc.date.accessioned2022-12-20T13:23:14Z
dc.date.available2022-12-20T13:23:14Z
dc.date.issued2018-10-1
dc.description.abstractThe Saura radar is designed and used to measure winds and electron densities at polar latitudes (69∘N) within the D region, namely between 50 and 100 km altitude. A relatively narrow radar beam can be generated and steered into distinct pointing directions as a rather large antenna array is used. From the observed radial velocities of the individual pointing directions, the horizontal and vertical wind fields can be obtained using the Doppler beam swinging (DBS) method. With recent upgrades to the radar, the interferometric capabilities are largely improved allowing simultaneous application of different wind estimation techniques now, and also echo localization. In recent studies, Saura DBS winds assuming isotropic scattering were found to be underestimated in comparison with highly reliable winds observed with the MAARSY MST radar in the presence of polar mesospheric summer echoes (PMSE). This underestimation has been investigated by analyzing the scattering positions as well as applying the imaging Doppler interferometry technique. Besides this, Saura winds derived with the classical DBS method seem to be error prone at altitudes above 90 km and even below this altitude for periods of enhanced ionization, e.g., particle precipitations. Various methods taking into account the scattering positions have been used to correct the wind underestimation. These winds are compared to MST radar winds during PMSE, and an optimal combination of these methods for the Saura radar is presented. This combined wind data appears to be reliable; it shows reasonable amplitudes as well as tidal structures for the entire altitude region.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/10688
dc.identifier.urihttp://dx.doi.org/10.34657/9724
dc.language.isoeng
dc.publisherHeidelberg : Springer
dc.relation.doihttps://doi.org/10.1186/s40623-018-0927-0
dc.relation.essn1880-5981
dc.rights.licenseCC BY 4.0 Unported
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subject.ddc550
dc.subject.otherD regioneng
dc.subject.otherInterferometryeng
dc.subject.otherRadareng
dc.subject.otherScatteringeng
dc.subject.otherWind estimationeng
dc.titleOn the role of anisotropic MF/HF scattering in mesospheric wind estimationeng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorIAP
wgl.subjectGeowissenschaftenger
wgl.typeZeitschriftenartikelger
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