Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/126060
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dc.contributor.authorVincent, R.A.en
dc.contributor.authorKovalam, S.en
dc.contributor.authorMurphy, D.J.en
dc.contributor.authorReid, I.M.en
dc.contributor.authorYounger, J.P.en
dc.date.issued2019en
dc.identifier.citationJournal of Geophysical Research: Atmospheres, 2019; 124(21):11070-11085en
dc.identifier.issn2169-897Xen
dc.identifier.issn2169-8996en
dc.identifier.urihttp://hdl.handle.net/2440/126060-
dc.description.abstractDirect measurement of mean vertical velocities in the mesosphere‐lower thermosphere (60–110 km) is not possible due to their small values. Here we derive vertical velocities using the divergence of the mean meridional wind over the Antarctic summer pole using MF radar wind measurements made at Davis Station (69°S, 78°E) between 1994 and 2018. Estimates of vertical velocity are restricted to a 21‐day period centered just after solstice when the equatorward wind reaches its maximum value of about 15 m s⁻¹ at heights near 90 km. The Medium Frequency (MF) radar winds are calibrated against colocated meteor wind radar observations. Neutral densities required for the vertical wind calculations are obtained from zonally averaged temperature measurements obtained by the MLS instrument aboard the AURA satellite. The estimated vertical velocities have peak values varying between 2 and 6 cm s⁻¹ with significant interannual variability. While the peak values do not show significant long‐term change, there is a long‐term decrease in the mean height of maximum winds of about 0.6 km per decade that is statistically significant. The interannual variability is linked to the date of transition in the stratospheric zonal circulation from winter eastward to summer westward flow. Meridional and vertical velocities are smaller and peak at lower altitudes during early transitions (20–30 days prior to solstice) than is the case for late transitions that occur at solstice or later.en
dc.description.statementofresponsibilityR.A. Vincent, S. Kovalam, D.J. Murphy, I.M. Reid, and J.P. Youngeren
dc.language.isoenen
dc.publisherWiley; American Geophysical Unionen
dc.rights©2019. American Geophysical Union. All Rights Reserved.en
dc.subjectMesosphere‐thermosphere; winds and temperature; vertical velocity; middle atmosphere couplingen
dc.titleTrends and variability in vertical winds in the Southern Hemisphere Summer Polar Mesosphere and Lower Thermosphereen
dc.typeJournal articleen
dc.identifier.rmid1000005255en
dc.identifier.doi10.1029/2019JD030735en
dc.identifier.pubid506065-
pubs.library.collectionPhysics publicationsen
pubs.library.teamDS14en
pubs.verification-statusVerifieden
pubs.publication-statusPublisheden
dc.identifier.orcidVincent, R.A. [0000-0001-6559-6544]en
dc.identifier.orcidKovalam, S. [0000-0001-6528-0072]en
dc.identifier.orcidReid, I.M. [0000-0003-2340-9047]en
dc.identifier.orcidYounger, J.P. [0000-0003-2918-1709]en
Appears in Collections:Physics publications

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