Longitudinal structure of stationary planetary waves in the middle atmosphere – extraordinary years

One important but little studied factor in the middle atmosphere meridional circulation is its longitudinal structure. Kozubek et al. (2015) disclosed the existence of the two-cell longitudinal structure in meridional wind at 10 hPa at higher latitudes in January. This two-cell structure is a co...

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Main Authors: J. Lastovicka, P. Krizan, M. Kozubek
Format: Article
Language:English
Published: Copernicus Publications 2018-01-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/36/181/2018/angeo-36-181-2018.pdf
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spelling doaj-d7971454517642f2a48ec8eb07635c412020-11-24T22:55:54ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762018-01-013618119210.5194/angeo-36-181-2018Longitudinal structure of stationary planetary waves in the middle atmosphere – extraordinary yearsJ. Lastovicka0P. Krizan1M. Kozubek2Institute of Atmospheric Physics ASCR, Bocni II, 14131 Prague, Czech RepublicInstitute of Atmospheric Physics ASCR, Bocni II, 14131 Prague, Czech RepublicInstitute of Atmospheric Physics ASCR, Bocni II, 14131 Prague, Czech RepublicOne important but little studied factor in the middle atmosphere meridional circulation is its longitudinal structure. Kozubek et al. (2015) disclosed the existence of the two-cell longitudinal structure in meridional wind at 10 hPa at higher latitudes in January. This two-cell structure is a consequence of the stratospheric stationary wave SPW1 in geopotential heights. Therefore here the longitudinal structure in geopotential heights and meridional wind is analysed based on MERRA data over 1979–2013 and limited NOGAPS-ALPHA data in order to find its persistence and altitudinal dependence with focus on extraordinary years. The SPW1 in geopotential heights and related two-cell structure in meridional wind covers the middle stratosphere (lower boundary  ∼  50 hPa), upper stratosphere and most of the mesosphere (almost up to about 0.01 hPa). The two-cell longitudinal structure in meridional wind is a relatively persistent feature; only 9 out of 35 winters (Januaries) display more complex structure. Morphologically the deviation of these extraordinary Januaries consists in upward propagation of the second (Euro-Atlantic) peak (i.e. SPW2 structure) to higher altitudes than usually, mostly up to the mesosphere. All these Januaries occurred under the positive phase of PNA (Pacific North American) index but there are also other Januaries under its positive phase, which behave in an ordinary way. The decisive role in the existence of extraordinary years (Januaries) appears to be played by the SPW filtering by the zonal wind pattern. In all ordinary years the mean zonal wind pattern in January allows the upward propagation of SPW1 (Aleutian peak in geopotential heights) up to the mesosphere but it does not allow the upward propagation of the Euro-Atlantic SPW2 peak to and above the 10 hPa level. On the other hand, the mean zonal wind filtering pattern in extraordinary Januaries is consistent with the observed pattern of geopotential heights at higher altitudes.https://www.ann-geophys.net/36/181/2018/angeo-36-181-2018.pdf
collection DOAJ
language English
format Article
sources DOAJ
author J. Lastovicka
P. Krizan
M. Kozubek
spellingShingle J. Lastovicka
P. Krizan
M. Kozubek
Longitudinal structure of stationary planetary waves in the middle atmosphere – extraordinary years
Annales Geophysicae
author_facet J. Lastovicka
P. Krizan
M. Kozubek
author_sort J. Lastovicka
title Longitudinal structure of stationary planetary waves in the middle atmosphere – extraordinary years
title_short Longitudinal structure of stationary planetary waves in the middle atmosphere – extraordinary years
title_full Longitudinal structure of stationary planetary waves in the middle atmosphere – extraordinary years
title_fullStr Longitudinal structure of stationary planetary waves in the middle atmosphere – extraordinary years
title_full_unstemmed Longitudinal structure of stationary planetary waves in the middle atmosphere – extraordinary years
title_sort longitudinal structure of stationary planetary waves in the middle atmosphere – extraordinary years
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2018-01-01
description One important but little studied factor in the middle atmosphere meridional circulation is its longitudinal structure. Kozubek et al. (2015) disclosed the existence of the two-cell longitudinal structure in meridional wind at 10 hPa at higher latitudes in January. This two-cell structure is a consequence of the stratospheric stationary wave SPW1 in geopotential heights. Therefore here the longitudinal structure in geopotential heights and meridional wind is analysed based on MERRA data over 1979–2013 and limited NOGAPS-ALPHA data in order to find its persistence and altitudinal dependence with focus on extraordinary years. The SPW1 in geopotential heights and related two-cell structure in meridional wind covers the middle stratosphere (lower boundary  ∼  50 hPa), upper stratosphere and most of the mesosphere (almost up to about 0.01 hPa). The two-cell longitudinal structure in meridional wind is a relatively persistent feature; only 9 out of 35 winters (Januaries) display more complex structure. Morphologically the deviation of these extraordinary Januaries consists in upward propagation of the second (Euro-Atlantic) peak (i.e. SPW2 structure) to higher altitudes than usually, mostly up to the mesosphere. All these Januaries occurred under the positive phase of PNA (Pacific North American) index but there are also other Januaries under its positive phase, which behave in an ordinary way. The decisive role in the existence of extraordinary years (Januaries) appears to be played by the SPW filtering by the zonal wind pattern. In all ordinary years the mean zonal wind pattern in January allows the upward propagation of SPW1 (Aleutian peak in geopotential heights) up to the mesosphere but it does not allow the upward propagation of the Euro-Atlantic SPW2 peak to and above the 10 hPa level. On the other hand, the mean zonal wind filtering pattern in extraordinary Januaries is consistent with the observed pattern of geopotential heights at higher altitudes.
url https://www.ann-geophys.net/36/181/2018/angeo-36-181-2018.pdf
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