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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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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