2019
DOI: 10.5194/angeo-37-943-2019
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Nonlinear forcing mechanisms of the migrating terdiurnal solar tide and their impact on the zonal mean circulation

Abstract: Abstract. We investigate the forcing mechanisms of the terdiurnal solar tide in the middle atmosphere using a mechanistic global circulation model. In order to quantify their individual contributions, we perform several model experiments and separate each forcing mechanism by switching off the remaining sources. We find that the primary excitation is owing to the terdiurnal component of solar radiation absorption in the troposphere and stratosphere. Secondary sources are nonlinear tide–tide interactions and gr… Show more

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Cited by 15 publications
(21 citation statements)
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“…Compared to earlier MUAM versions that use a highly tuned linear Lindzen-type GW parameterization for the middle atmosphere (e.g. Jacobi et al, 2015;Lilienthal and Jacobi, 2019;Samtleben et al, 2019), the winter mesospheric jet is enhanced in the present simulations. In the lower thermosphere, the main impact of the whole atmosphere GW parameterization is to drive a vertical/meridional circulation, mainly by the GWs with high phase speeds, which are able to propagate through the MLT wind jets.…”
Section: Discussionmentioning
confidence: 63%
“…Compared to earlier MUAM versions that use a highly tuned linear Lindzen-type GW parameterization for the middle atmosphere (e.g. Jacobi et al, 2015;Lilienthal and Jacobi, 2019;Samtleben et al, 2019), the winter mesospheric jet is enhanced in the present simulations. In the lower thermosphere, the main impact of the whole atmosphere GW parameterization is to drive a vertical/meridional circulation, mainly by the GWs with high phase speeds, which are able to propagate through the MLT wind jets.…”
Section: Discussionmentioning
confidence: 63%
“…MUAM is a 3-D, primitive equation, mechanistic global circulation model based on the earlier Cologne Model of the Middle Atmosphere-Leipzig Institute for Meteorology (COMMA-LIM), described by Jakobs et al (1986), Fröhlich et al (2003b) and Jacobi et al (2006). Recent versions of the MUAM model are described by Lilienthal et al (2017), Lilienthal et al (2018), Lilienthal and Jacobi (2019), Jacobi et al (2019) and Samtleben et al (2019). The model reaches from the surface at 1000 hPa to a log-pressure height of 160 km, with a constant scale height of H = 7 km and a vertical resolution of 2.842 km.…”
Section: Description Of the Model And The Experimentsmentioning
confidence: 99%
“…Above 30 km, the background winds can develop freely in the model and are only affected by the zonal mean temperature nudging below. In contrast to other model experiments (e.g., Pogoreltsev et al, 2007;Pogoreltsev, 2007;Lilienthal et al, 2017;Samtleben et al, 2019), we do not include planetary wave forcing at the lower boundary to avoid undesired wave coupling with tides. In our experiments, we perform ensemble runs with 11 members using ERA-Interim data from 2000 to 2010 in order to describe interannual variability.…”
Section: Description Of the Model And The Experimentsmentioning
confidence: 99%
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