Idealized large-eddy simulations of nocturnal low-level jets over subtropical desert regions and implications for dust-generating winds

dc.bibliographicCitation.firstPage1740
dc.bibliographicCitation.issue690eng
dc.bibliographicCitation.lastPage1752
dc.bibliographicCitation.volume141
dc.contributor.authorHeinold, Bernd
dc.contributor.authorKnippertz, Peter
dc.contributor.authorBeare, Robert J.
dc.date.accessioned2018-02-01T06:45:58Z
dc.date.available2019-06-26T17:22:03Z
dc.date.issued2014
dc.description.abstractNocturnal low-level jets (LLJs) are maxima in the wind profile, which often form above the stable nocturnal boundary layer. Over the Sahara, the world’s largest source of mineral dust, this phenomenon is of particular importance to the emission and transport of desert aerosol.We present the first ever detailed large-eddy simulations of dust-generating LLJs. Using sensitivity studies with the UK Met Office large-eddy model (LEM), two key controls of the nocturnal LLJ are investigated: surface roughness and the Coriolis force. Functional relationships derived from the LEM results help to identify optimal latitude–roughness configurations for a maximum LLJ enhancement. Ideal conditions are found in regions between 20 and 27◦N with roughness lengths >0.0001m providing long oscillation periods and large jet amplitudes. Typical LLJ enhancements reach up to 3.5ms−1 for geostrophic winds of 10ms−1. The findings are largely consistent with results from a theoretical LLJ model applied for comparison. The results demonstrate the importance of latitude and roughness in creating regional patterns of LLJ influence. Combining the functional relationships with high-resolution roughness data over northern Africa gives good agreement with the location of morning dust uplift in satellite observations. It is shown that shear-induced mixing plays an important role for the LLJ evolution and surface gustiness. With decreasing latitude the LLJ oscillation period is longer and, thus, shearinduced mixing is weaker, allowing a more stable nocturnal stratification to develop. This causes a later and more abrupt LLJ breakdown in the morning with stronger gusts, which can compensate for the slower LLJ evolution that leads to a weaker jet maximum. The findings presented here can serve as the first step towards a parametrization to improve the representationof the effectsofnocturnal LLJsondust emission in coarser-resolution models.eng
dc.description.versionpublishedVersioneng
dc.formatapplication/pdf
dc.identifier.urihttps://doi.org/10.34657/1025
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/908
dc.language.isoengeng
dc.publisherHoboken, NJ : Wileyeng
dc.relation.doihttps://doi.org/10.1002/qj.2475
dc.relation.ispartofseriesQuarterly Journal of the Royal Meteorological Society, Volume 141, Issue 690, Part A, Page 1740-1752eng
dc.rights.licenseCC BY-NC-ND 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/eng
dc.subjectnocturnal low-level jeteng
dc.subjectboundary-layer transitioneng
dc.subjectlarge-eddy simulationeng
dc.subjectdust emissioneng
dc.subjectSaharaeng
dc.subjectgustseng
dc.subjectshear-induced mixingeng
dc.subject.ddc550eng
dc.titleIdealized large-eddy simulations of nocturnal low-level jets over subtropical desert regions and implications for dust-generating windseng
dc.typearticleeng
dc.typeTexteng
dcterms.bibliographicCitation.journalTitleQuarterly Journal of the Royal Meteorological Societyeng
tib.accessRightsopenAccesseng
wgl.contributorTROPOSeng
wgl.subjectGeowissenschafteneng
wgl.typeZeitschriftenartikeleng
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