Comparative study between ground-based observations and NAVGEM-HA analysis data in the mesosphere and lower thermosphere region

dc.bibliographicCitation.firstPage11979eng
dc.bibliographicCitation.issue20eng
dc.bibliographicCitation.lastPage12010eng
dc.bibliographicCitation.volume20eng
dc.contributor.authorStober, Gunter
dc.contributor.authorBaumgarten, Kathrin
dc.contributor.authorMcCormack, John P.
dc.contributor.authorBrown, Peter
dc.contributor.authorCzarnecki, Jerry
dc.date.accessioned2021-08-19T09:53:45Z
dc.date.available2021-08-19T09:53:45Z
dc.date.issued2020
dc.description.abstractRecent studies have shown that day-to-day variability of the migrating semidiurnal solar (SW2) tide within the mesosphere and lower thermosphere (MLT) is a key driver of anomalies in the thermosphere-ionosphere system. Here, we study the variability in both the amplitude and phase of SW2 using meteor radar wind and lidar temperature observations at altitudes of 75-110 km as well as wind and temperature output from the Navy Global Environmental Model-High Altitude (NAVGEM-HA), a high-altitude meteorological analysis system. Application of a new adaptive spectral filter technique to both local radar wind observations and global NAVGEM-HA analyses offers an important cross-validation of both data sets and makes it possible to distinguish between migrating and non-migrating tidal components, which is difficult using local measurements alone. Comparisons of NAVGEM-HA, meteor radar and lidar observations over a 12-month period show that the meteorological analyses consistently reproduce the seasonal as well as day-to-day variability in mean winds, mean temperatures and SW2 features from the ground-based observations. This study also examines in detail the day-to-day variability in SW2 during two sudden stratospheric warming, events that have been implicated in producing ionospheric anomalies. During this period, both meteor radar and NAVGEM-HA winds show a significant phase shift and amplitude modulation, but no signs of coupling to the lunar tide as previous studies have suggested. Overall, these findings demonstrate the benefit of combining global high-altitude meteorological analyses with ground-based observations of the MLT region to better understand the tidal variability in the atmosphere. © 2020 Author(s).eng
dc.description.sponsorshipLeibniz_Fondseng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/6527
dc.identifier.urihttps://doi.org/10.34657/5574
dc.language.isoengeng
dc.publisherKatlenburg-Lindau : EGUeng
dc.relation.doihttps://doi.org/10.5194/acp-20-11979-2020
dc.relation.essn1680-7324
dc.relation.ispartofseriesAtmospheric chemistry and physics 20 (2020), Nr. 20eng
dc.relation.issn1680-7316
dc.rights.licenseCC BY 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/eng
dc.subjectsemidiurnal solar (SW2)eng
dc.subjectmesosphere and lower thermosphere (MLT)eng
dc.subjectNavy Global Environmental Model-High Altitude (NAVGEM-HA)eng
dc.subject.ddc550eng
dc.titleComparative study between ground-based observations and NAVGEM-HA analysis data in the mesosphere and lower thermosphere regioneng
dc.typearticleeng
dc.typeTexteng
dcterms.bibliographicCitation.journalTitleAtmospheric chemistry and physicseng
tib.accessRightsopenAccesseng
wgl.contributorIAPeng
wgl.subjectGeowissenschafteneng
wgl.typeZeitschriftenartikeleng
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