Impact of local gravity wave forcing in the lower stratosphere on the polar vortex stability: effect of longitudinal displacement
<p>The effects of gravity wave (GW) breaking hotspots in the lower stratosphere, especially the role of their longitudinal distribution, are evaluated through a sensitivity study by using a simplified middle atmosphere circulation model. For the position of the local GW hotspot, we first selec...
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Copernicus Publications
2020-01-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/38/95/2020/angeo-38-95-2020.pdf |
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author | N. Samtleben A. Kuchař P. Šácha P. Šácha P. Šácha P. Pišoft C. Jacobi |
author_facet | N. Samtleben A. Kuchař P. Šácha P. Šácha P. Šácha P. Pišoft C. Jacobi |
author_sort | N. Samtleben |
collection | DOAJ |
description | <p>The effects of gravity wave (GW) breaking hotspots in the lower stratosphere, especially the role of their longitudinal distribution, are evaluated through a sensitivity study by using a simplified middle atmosphere circulation model.
For the position of the local GW hotspot, we first selected a fixed latitude range between 37.5 and 62.5<span class="inline-formula"><sup>∘</sup></span> N and a longitude range from 112.5 to 168.75<span class="inline-formula"><sup>∘</sup></span> E, as well as an altitude range between 18 and 30 km.
This confined GW hotspot was then shifted in longitude by 45<span class="inline-formula"><sup>∘</sup></span> steps, so that we created eight artificial GW hotspots in total.
Strongly dependent on the location of the respective GW hotspot with regard to the phase of the stationary planetary wave of wavenumber 1 (SPW 1) generated in the model, the local GW forcing may interfere constructively or destructively with the modeled SPW 1.
GW hotspots, which are located in North America near the Rocky Mountains, lead to an increase in the SPW 1 amplitude and EP flux, while hotspots located near the Caucasus, the Himalayas or the Scandinavian region lead to a decrease in these parameters.
Thus, the polar vortex is less (Caucasus and Himalayan hotspots) or more weakened (Rocky Mountains hotspot) by the prevailing SPW activity.
Because the local GW forcing generally suppresses wave propagation at midlatitudes, the SPWs 1 propagate into the polar region, where the refractive index turned to positive values for the majority of the artificial GW hotspots.
An additional source of SPW 1 may be local instabilities indicated by the reversal in the meridional potential vorticity gradient in the polar region in connection with a positive EP divergence.
In most cases, the SPWs 1 are breaking in the polar region and maintain the deceleration and, thus, the weakening of the polar vortex.
While the SPWs 1 that form when the GW hotspots are located above North America propagate through the polar region into the middle atmosphere, the SPWs 1 in the remaining GW hotspot simulations were not able to propagate further upwards because of a negative refractive index above the positive refractive index anomaly in the polar region.
GW hotspots, which are located near the Himalayas, influence the mesosphere–lower thermosphere region because of possible local instabilities in the lower mesosphere generating additional SPWs 1, which propagate upwards into the mesosphere.</p> |
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spelling | doaj.art-12dabf03406a42acba2b0d22325ef8f42022-12-21T23:56:39ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762020-01-01389510810.5194/angeo-38-95-2020Impact of local gravity wave forcing in the lower stratosphere on the polar vortex stability: effect of longitudinal displacementN. Samtleben0A. Kuchař1P. Šácha2P. Šácha3P. Šácha4P. Pišoft5C. Jacobi6Institute for Meteorology, Universität Leipzig, Stephanstr. 3, 04103 Leipzig, GermanyDepartment of Atmospheric Physics, Faculty of Mathematics and Physics, Charles University, V Holesovickach 2, 180 00 Prague 8, Czech RepublicInstitute for Meteorology, Universität für Bodenkultur Wien, Gregor-Mendel-Straße 33, 1180 Vienna, AustriaDepartment of Atmospheric Physics, Faculty of Mathematics and Physics, Charles University, V Holesovickach 2, 180 00 Prague 8, Czech RepublicEPhysLab, Faculty of Sciences, Universidade de Vigo, Campus As Lagoas, s/n, 32004 Ourense, SpainDepartment of Atmospheric Physics, Faculty of Mathematics and Physics, Charles University, V Holesovickach 2, 180 00 Prague 8, Czech RepublicInstitute for Meteorology, Universität Leipzig, Stephanstr. 3, 04103 Leipzig, Germany<p>The effects of gravity wave (GW) breaking hotspots in the lower stratosphere, especially the role of their longitudinal distribution, are evaluated through a sensitivity study by using a simplified middle atmosphere circulation model. For the position of the local GW hotspot, we first selected a fixed latitude range between 37.5 and 62.5<span class="inline-formula"><sup>∘</sup></span> N and a longitude range from 112.5 to 168.75<span class="inline-formula"><sup>∘</sup></span> E, as well as an altitude range between 18 and 30 km. This confined GW hotspot was then shifted in longitude by 45<span class="inline-formula"><sup>∘</sup></span> steps, so that we created eight artificial GW hotspots in total. Strongly dependent on the location of the respective GW hotspot with regard to the phase of the stationary planetary wave of wavenumber 1 (SPW 1) generated in the model, the local GW forcing may interfere constructively or destructively with the modeled SPW 1. GW hotspots, which are located in North America near the Rocky Mountains, lead to an increase in the SPW 1 amplitude and EP flux, while hotspots located near the Caucasus, the Himalayas or the Scandinavian region lead to a decrease in these parameters. Thus, the polar vortex is less (Caucasus and Himalayan hotspots) or more weakened (Rocky Mountains hotspot) by the prevailing SPW activity. Because the local GW forcing generally suppresses wave propagation at midlatitudes, the SPWs 1 propagate into the polar region, where the refractive index turned to positive values for the majority of the artificial GW hotspots. An additional source of SPW 1 may be local instabilities indicated by the reversal in the meridional potential vorticity gradient in the polar region in connection with a positive EP divergence. In most cases, the SPWs 1 are breaking in the polar region and maintain the deceleration and, thus, the weakening of the polar vortex. While the SPWs 1 that form when the GW hotspots are located above North America propagate through the polar region into the middle atmosphere, the SPWs 1 in the remaining GW hotspot simulations were not able to propagate further upwards because of a negative refractive index above the positive refractive index anomaly in the polar region. GW hotspots, which are located near the Himalayas, influence the mesosphere–lower thermosphere region because of possible local instabilities in the lower mesosphere generating additional SPWs 1, which propagate upwards into the mesosphere.</p>https://www.ann-geophys.net/38/95/2020/angeo-38-95-2020.pdf |
spellingShingle | N. Samtleben A. Kuchař P. Šácha P. Šácha P. Šácha P. Pišoft C. Jacobi Impact of local gravity wave forcing in the lower stratosphere on the polar vortex stability: effect of longitudinal displacement Annales Geophysicae |
title | Impact of local gravity wave forcing in the lower stratosphere on the polar vortex stability: effect of longitudinal displacement |
title_full | Impact of local gravity wave forcing in the lower stratosphere on the polar vortex stability: effect of longitudinal displacement |
title_fullStr | Impact of local gravity wave forcing in the lower stratosphere on the polar vortex stability: effect of longitudinal displacement |
title_full_unstemmed | Impact of local gravity wave forcing in the lower stratosphere on the polar vortex stability: effect of longitudinal displacement |
title_short | Impact of local gravity wave forcing in the lower stratosphere on the polar vortex stability: effect of longitudinal displacement |
title_sort | impact of local gravity wave forcing in the lower stratosphere on the polar vortex stability effect of longitudinal displacement |
url | https://www.ann-geophys.net/38/95/2020/angeo-38-95-2020.pdf |
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