Stratosphere analysis: looking for possible stratwarming events



  Teleconnections and long range forecasts  
AAO (Antarctic Oscillation) NAM (North Annular Mode) SCAND (Scandinavia pattern) Stratosphere Analysis
AO (Arctic Oscillation) NAO (North Atlantic Oscillation) SOI (Southern Oscillation) North-Pole Stratosphere Temp
EA (East Atlantic) Polar/Eurasia SST (Sea Surface Temperature) 10 hPa Temp&Geop
EA/WR (East Atl./Western Russia) PNA (Pacific North-America) 100 hPa Temp&Geop
MJO (Madden Julian Oscillation) QBO (Quasi-Biennial Oscillation) Intraseasonal Oscillations


Teleconnective indices - Stratosphere analysis (identification of stratwarming events)

This page contains some graphs and diagrams useful for identifying possible stratwarming events, i.e. sudden and remarkable increase of the stratosphere temperature over the polar regions. The stratosphere is the second layer of the atmosphere of the Earth, located above the troposphere and below the mesosphere that extends between about 15 and 60 km of altitude (see figure). The phenomenon is also known as Sudden Stratospheric Warming (SSW). In some cases the westerly polar night jet disappears and easterly winds appear during the warming.
The warming is called a minor warming, when the polar temperature increases more than 25 degrees in a period of a week or less at any stratospheric level. If the zonal mean temperature increases poleward from 60 degrees latitude and the net zonal mean zonal winds become easterly at 10 hPa (30 km) or below, it is classified as a major. In a major SSW the sudden temperature heating is notable, even +70 °C in a few days.
The increase in the temperature of the stratosphere can have repercussions on meteorological evolution, particularly in the northern hemisphere. Stratwarming can result in a rupture of the polar vortex with consequent irruptions of cold air towards mid-latitudes. This event, labeled as major, is also anticipated by a change in the circulation of the winds at high altitude (usually the pressure level is observed at 10 hPa, corresponding to about 30 km of altitude). A shift of the polar vertex towards the mid-latitudes, with consequent thermal drop, is also always part of the major events.
The SSW was discovered in 1952 by Scherhag[1], but it took some time (1971) before the mechanism was theoretically identified by Matsuno[2]. The SSW is caused by a rapid amplification of planetary waves propagating upward from the troposphere. Planetary waves deposit westward momentum and create a strong meridional circulation which produces a large warming in the polar stratosphere due to adiabatic heating (e.g., McIntyre 1982, [3]).
The split of the polar vortex involves the formation in the polar zone of a large area of ​​high pressure characterized by positive temperature anomalies, both in the troposphere and in the stratosphere. At the same time, the two lobes originating from the split are heading south (towards north in the southern hemisphere) bringing with them bad weather and falling temperatures.
The polar vortex split phenomenon preceded the largest cold outbreaks also observed in Italy, but there is no direct correlation between observation of large colds and stratwarming events. That is, it is possible that a frost wave is caused by other factors. One example above all was observed in 1956, since the irruption of cold air was not preceded by SSW.
It usually takes 2-3 weeks for the polar vortex to heal.
[1]: Die explosionsartige Stratospharenerwarmung des Spatwinters 1951/52, Ber. Deut. Wetterdienst 38, 51-63. [2]: A dynamical model of the stratospheric sudden warming. J. Atmos. Sci., 28, 1479-1494
[3]: How well do we understand the dynamics of stratospheric warming? J. Meteor. Soc. Japan, 60, 37-65

Temperature cross section of the atmospher and first four layers
Temperature cross section of the atmospher and first four layers.
Credits: ucsd.edu
Strong polar vortex map
Example of a strong polar vortex, observed in November 2013. Credits: wikipedia.org.
Weak polar vortex map
Example of a weak polar vortex, observed in January 2014. Credits: wikipedia.org.

Interaction between Stratosphere and Troposphere

The relationship between the stratosphere and the troposphere has widely been recognized. During winter, tropospheric planetary waves propagate into the stratosphere along the westerly jet. More recently, the converse relationship that the zonal mean zonal wind anomalies slowly propagate from the subtropical upper stratosphere to the polar region of the lower stratosphere and the troposphere during the boreal winter, is also noted.
It has been shown that SSWs occur in association with slowly propagating zonal mean zonal wind anomalies, and the related changes in the troposphere exhibits the Annular Mode (AO) like structure. Tthe downward propagation of the AO from the stratosphere to the troposphere occurs in association with SSWs.


E-P Flux Analysis

The stratospheric and the tropospheric circulation are connected with each other through wave mean flow interactions. The Eliassen-Palm (E-P) flux is widely used to characterize the wave activity. The direction of the E-P flux is proportional to the group velocity and indicates the direction of the propagation of the waves. Approximately, the vertical and horizontal components of the E-P flux are proportional to the eddy heat and momentum flux, respectively. The divergence of E-P flux is proportional to the northward flux of quasi-geostrophic potential vorticity, so that it is a direct measure of the total forcing of the zonal mean flow by eddies. Therefore, the E-P flux and its divergence are important and useful to diagnose planetary waves propagation as well as the effective mean zonal force induced by the waves.


Polar Regions Temperatures - Analysis and Forecast

The following diagram, based on GFS analysis and forecast, shows observed and predicted temperature values on the polar regions (average between 60° N and 90° N) between 200 and 1 hPa.

North pole temperatures analysis and forecast
Temperature analysis and forecast on the polar regions at different altitudes. Credits: stratobserve.com


Zonal winds 6 ° N - Analysis and forecast

In a free atmosphere and far from the friction forces of the earth's surface, the so-called geostrophic wind is observed in good approximation. This is an ideal wind obtained in stationary conditions from the equilibrium between the gradient forces (i.e. the force that pushes the air between a center of high pressure and one of low pressure) and the Coriolis force (that is, the force which in the northern hemisphere deflects motion to the right). The geostrophic wind has a direction parallel to the isobars and in the northern hemisphere it keeps the high pressure on its right.
The intensity of the geostrophic wind increases with latitude and with the horizontal pressure gradient and decreases with increasing air density.
The zonal wind follows the lines of the parallels, forming latitudinal circles, in the west-east direction. As written previously, SSW have been shown to occur in association with mean zonal wind anomalies.
The following diagram, based on GFS analysis and forecast, shows observed and predicted zonal wind speeds on the polar regions at 60° N between 200 and 1 hPa.

North pole zonal wind speed analysis and forecast
60° N wind speed; analysis and forecast at different altitudes.
Credits: stratobserve.com

30-hPa temperature over the North/South Pole

30-hPa temperature level over the North Pole
Time-series representation of temperatures at the 30-hPa level over the North Pole. The black line shows daily temperatures, and the gray line indicates the normal (i.e., the 1991-2020 average). 30 hPa corresponds to about 25 km of altitude. Credits: ds.data.jma.go.jp
30-hPa temperature level over the South Pole
Time-series representation of temperatures at the 30-hPa level over the South Pole. The black line shows daily temperatures, and the gray line indicates the normal (i.e., the 1991-2020 average). 30 hPa corresponds to about 25 km of altitude.
Credits: ds.data.jma.go.jp


10-hPa temperature over the North/South Pole

10-hPa temperature level over the North Pole
Time-series representation of temperatures at the 10-hPa level over the North Pole. The black line shows daily temperatures, and the gray line indicates the normal (i.e., the 1991-2020 average). 10 hPa corresponds to about 30 km of altitude. Credits: ds.data.jma.go.jp
10-hPa temperature level over the South Pole
Time-series representation of temperatures at the 10-hPa level over the South Pole. The black line shows daily temperatures, and the gray line indicates the normal (i.e., the 1991-2020 average). 10 hPa corresponds to about 30 km of altitude.
Credits: ds.data.jma.go.jp


Time-height cross section of zonal mean temperature

North pole zonal mean temperature
Time-height cross section of zonal mean temperature averaged over 60° N - 90° N (top) and time-series representation of vertical components of E-P flux averaged over 30° N - 90° N at the 100-hPa level (bottom).
The black and gray lines on the top indicate 10-hPa and 30-hPa temperature, respectively. The gray shading on the bottom denotes the vertical components of E-P flux for whole zonal wave numbers, and the red, blue and green lines denote the vertical components of E-P flux for zonal wavenumbers 1, 2 and 3, respectively. The unit for the vertical component of E-P flux is m2/s2.
Credits: ds.data.jma.go.jp
South pole zonal mean temperature
Time-height cross section of zonal mean temperature averaged over 60° S - 90° S (top) and time-series representation of vertical components of E-P flux averaged over 30° S - 90° S at the 100-hPa level (bottom).
The black and gray lines on the top indicate 10-hPa and 30-hPa temperature, respectively. The gray shading on the bottom denotes the vertical components of E-P flux for whole zonal wave numbers, and the red, blue and green lines denote the vertical components of E-P flux for zonal wavenumbers 1, 2 and 3, respectively. The unit for the vertical component of E-P flux is m2/s2.
Credits: ds.data.jma.go.jp


Zonal wind & Vertical components of 100-hPa E-P flux

North pole zonal mean wind
Time-height cross section of zonal mean wind averaged over 60° N - 90° N (top) and time-series representation of vertical components of E-P flux averaged over 30° N - 90° N at the 100-hPa level (bottom).
The gray shading on the bottom denotes the vertical components of E-P flux for whole zonal wave numbers, and the red, blue and green lines denote the vertical components of E-P flux for zonal wavenumbers 1, 2 and 3, respectively. The unit for the vertical component of E-P flux is m2/s2.
Credits: ds.data.jma.go.jp
South pole zonal mean wind
Time-height cross section of zonal mean wind averaged over 60° S - 90° S (top) and time-series representation of vertical components of E-P flux averaged over 30° S - 90° S at the 100-hPa level (bottom).
The gray shading on the bottom denotes the vertical components of E-P flux for whole zonal wave numbers, and the red, blue and green lines denote the vertical components of E-P flux for zonal wavenumbers 1, 2 and 3, respectively. The unit for the vertical component of E-P flux is m2/s2.
Credits: ds.data.jma.go.jp


30-hPa zonal mean zonal wind

30-hPa zonal mean zonal wind in the Northern Hemisphere
Latitude-time cross section of 30-hPa zonal mean zonal wind in the Northern Hemisphere. The contour interval is 10 m/s.
Credits: ds.data.jma.go.jp
30-hPa zonal mean zonal wind in the Southern Hemisphere
Latitude-time cross section of 30-hPa zonal mean zonal wind in the Southern Hemisphere. The contour interval is 10 m/s.
Credits: ds.data.jma.go.jp


30-hPa zonal mean temperature

30-hPa zonal mean temperature in the Northern Hemisphere
Latitude-time cross section of 30-hPa zonal mean temperature in the Northern Hemisphere. The contour interval is 10 °C.
Credits: ds.data.jma.go.jp
30-hPa zonal mean temperature in the Southern Hemisphere
Latitude-time cross section of 30-hPa zonal mean temperature in the Southern Hemisphere. The contour interval is 10 °C.
Credits: ds.data.jma.go.jp


10-hPa zonal mean zonal wind

10-hPa zonal mean zonal wind in the Northern Hemisphere
Latitude-time cross section of 10-hPa zonal mean zonal wind in the Northern Hemisphere. The contour interval is 10 m/s.
Credits: ds.data.jma.go.jp
10-hPa zonal mean zonal wind in the Southern Hemisphere
Latitude-time cross section of 10-hPa zonal mean zonal wind in the Southern Hemisphere. The contour interval is 10 m/s.
Credits: ds.data.jma.go.jp


10-hPa zonal mean temperature

10-hPa zonal mean temperature in the Northern Hemisphere
Latitude-time cross section of 10-hPa zonal mean temperature in the Northern Hemisphere. The contour interval is 10 °C.
Credits: ds.data.jma.go.jp
10-hPa zonal mean temperature in the Southern Hemisphere
Latitude-time cross section of 10-hPa zonal mean temperature in the Southern Hemisphere. The contour interval is 10 °C.
Credits: ds.data.jma.go.jp


100-hPa Vertical E-P flux (total wave)

100-hPa Vertical E-P flux (total wave) in the Northern Hemisphere
Latitude-time cross section of vertical components of E-P flux at the 100-hPa level in the Northern Hemisphere.
The contour interval is 6 m2/s2 (higher than 3m2/s2) and 3 m2/s2(lower than 3 m2/s2).
Credits: ds.data.jma.go.jp
100-hPa Vertical E-P flux (total wave) in the Southern Hemisphere
Latitude-time cross section of vertical components of E-P flux at the 100-hPa level in the Southern Hemisphere.
The contour interval is 6 m2/s2 (higher than 3m2/s2) and 3 m2/s2(lower than 3 m2/s2).
Credits: ds.data.jma.go.jp


30-hPa temperature change in a week

30-hPa temperature change in a week in the Northern Hemisphere
30-hPa temperature change in a week in the Northern Hemisphere.
The contour interval is 5 °C. The pink and light blue shadings indicate warming and cooling, respectively. The red shading denotes warming for values higher than 25 °C.
Credits: ds.data.jma.go.jp
30-hPa temperature change in a week in the Southern Hemisphere
30-hPa temperature change in a week in the Southern Hemisphere.
The contour interval is 5 °C. The pink and light blue shadings indicate warming and cooling, respectively. The red shading denotes warming for values higher than 25 °C.
Credits: ds.data.jma.go.jp


30-hPa temperature

30-hPa temperature in the Northern Hemisphere
30-hPa temperature in the Northern Hemisphere. The contour interval is 2 °C.
Credits: ds.data.jma.go.jp
30-hPa temperature in the Southern Hemisphere
30-hPa temperature in the Northern Hemisphere. The contour interval is 2 °C.
Credits: ds.data.jma.go.jp


30-hPa height

<b>30-hPa height in the Northern Hemisphere</b>.
                                                      The contour interval is 120 m.<br>Credits: ds.data.jma.go.jp
30-hPa temperature in the Northern Hemisphere. The contour interval is 2 °C.
Credits: ds.data.jma.go.jp
30-hPa height in the Southern Hemisphere
30-hPa height in the Southern Hemisphere. The contour interval is 120 m.
Credits: ds.data.jma.go.jp


10-hPa temperature change in a week

10-hPa temperature change in a week in the Northern Hemisphere
10-hPa temperature change in a week in the Northern Hemisphere.
The contour interval is 5 °C. The pink and light blue shadings indicate warming and cooling, respectively. The red shading denotes warming for values higher than 25 °C.
Credits: ds.data.jma.go.jp
10-hPa temperature change in a week in the Southern Hemisphere
10-hPa temperature change in a week in the Southern Hemisphere.
The contour interval is 5 °C. The pink and light blue shadings indicate warming and cooling, respectively. The red shading denotes warming for values higher than 25 °C.
Credits: ds.data.jma.go.jp


10-hPa temperature

10-hPa temperature in the Northern Hemisphere
10-hPa temperature in the Northern Hemisphere. The contour interval is 2 °C.
Credits: ds.data.jma.go.jp
10-hPa temperature in the Southern Hemisphere
10-hPa temperature in the Northern Hemisphere. The contour interval is 2 °C.
Credits: ds.data.jma.go.jp


10-hPa temperature

10-hPa temperature in the Northern Hemisphere
10-hPa temperature in the Northern Hemisphere. The contour interval is 2 °C.
Credits: ds.data.jma.go.jp
10-hPa temperature in the Southern Hemisphere
10-hPa temperature in the Northern Hemisphere. The contour interval is 2 °C.
Credits: ds.data.jma.go.jp


10-hPa height

10-hPa height in the North Hemisphere
10-hPa height in the Northern Hemisphere. The contour interval is 120 m.
Credits: ds.data.jma.go.jp
10-hPa height in the Southern Hemisphere
10-hPa height in the Southern Hemisphere. The contour interval is 120 m.
Credits: ds.data.jma.go.jp


Latitude-height cross section of zonal mean temperature

Latitude-height cross section of zonal mean temperature in theNorthern Hemisphere
Latitude-height cross section of zonal mean temperature in the Northern Hemisphere. The contour interval is 5 °C.
Credits: ds.data.jma.go.jp
Latitude-height cross section of zonal mean temperature in the Southern Hemisphere
Latitude-height cross section of zonal mean temperature in the Southern Hemisphere. The contour interval is 5 °C.
Credits: ds.data.jma.go.jp


Latitude-height cross section of zonal mean wind

Latitude-height cross section of zonal mean wind in the Norhern Hemisphere
Latitude-height cross section of zonal mean zonal wind in the Northern Hemisphere. The contour interval is 5 m/s.
Credits: ds.data.jma.go.jp
Latitude-height cross section of zonal mean wind in the Southern Hemisphere
Latitude-height cross section of zonal mean wind in the Southern Hemisphere. The contour interval is 5 m/s.
Credits: ds.data.jma.go.jp


Latitude-height cross section of zonal mean zonal wind and E-P flux

Latitude-height cross section of zonal mean zonal wind and E-P flux in the Northern Hemisphere
Latitude-height cross section of zonal mean zonal wind and E-P flux in the Northern Hemisphere. The contours show zonal wind at intervals of 5 m/s. The vectors indicate E-P flux scaled by square root of pressure (units: m3/s2 (meridional components), m2/s2 (vertical components).
Credits: ds.data.jma.go.jp
Latitude-height cross section of zonal mean zonal wind and E-P flux in the Southern Hemisphere
Latitude-height cross section of zonal mean zonal wind and E-P flux in the Southern Hemisphere. The contours show zonal wind at intervals of 5 m/s. The vectors indicate E-P flux scaled by square root of pressure (units: m3/s2 (meridional components), m2/s2 (vertical components).
Credits: ds.data.jma.go.jp

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