Climatic variability of dynamics in the winter stratosphere Kanukhina A.Y. Suvorova E.V. - PowerPoint PPT Presentation

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Climatic variability of dynamics in the winter stratosphere Kanukhina A.Y. Suvorova E.V.

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analysis of SPW of zonal wavenumber 1 and 2 (not shown here) from NCEP/NCAR data ... Temperature, geopotential height and zonal wind distribution in the tropo ... – PowerPoint PPT presentation

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Title: Climatic variability of dynamics in the winter stratosphere Kanukhina A.Y. Suvorova E.V.


1
Climatic variability of dynamics in the winter
stratosphere

Kanukhina A.Y.

Suvorova E.V.
Ulyanets E.K.

Pogoreltsev A.I. 9-13,September,2007
  • The Russian State Hydrometeorological
    UniversitySt.Petersburg

2
Why it is important?
  • A strong longitudinal inhomogeneity of
    meteorological fields is one of the main
    properties of stratospheric dynamics during
    winter. The fundamental problem of atmospheric
    dynamics including seasonal, interannual, and
    decadal variability of temperature and planetary
    wave activity within the troposphere and
    stratosphere, as well as possible effects within
    middle atmosphere caused by these changes becomes
    increasingly relevant for climate research.
  • The reason
  • the need to study dynamical and photochemical
    processes impacts on observed climatic changes of
    atmospheric temperature
  • there is a growing evidence that additional
    extended-range tropospheric forecast skill may
    also come from slow variations of the circulation
    and planetary waves in the stratosphere

3
Planetary waves
  • oscillations with typical periods of about 230
    days
  • large-scale (global) character
  • predominantly of tropospheric origin
  • 2 types
  • 1 - the stationary planetary waves (SPW),
    associated with the quasi-steady meteorological
    structures
  • 2 - the travelling planetary waves, which
    propagate predominantly westward, even though
    sometimes (rarely) the eastward propagation
    dominates
  • Example of Saturns waves of ionized particles
    http//photojournal.jpl.nasa.gov/catalog/PIA09186

4
The main objectives
  • analysis of SPW of zonal wavenumber 1 and 2 (not
    shown here) from NCEP/NCAR data since 1959
  • interannual, interdecadal and long-term SPW
    variability analysis
  • numerical simulation of SPW propagation with
    linearized model and stratospheric background
    conditions that are characteristic for different
    decades, comparison of stratospheric reanalyses
    with numerical model results
  • analysis of middle and upper atmosphere
    variability due to SPW based on numerical
    results, and comparison with experimental results
    from literature.

5
Previous results
  • noticeable climatic changes of the temperature in
    the lower atmosphere which have different signs
    at low and high latitudes
  • changes of the positions and intensity of
    tropospheric jets are in a good agreement with an
    increase of temperature latitudinal gradient
  • the results of simulation with the background
    zonal wind typical for 1960 and 2000 show an
    increase in amplitude of the SPW1 in the
    stratosphere and mesosphere of the winter
    hemisphere during the last decades

6
Modeled amplitudes of geopotential height
disturbances for SPW1 1960
2000

7
NCEP/NCAR (National Center for Environmental
Prediction - National Center for Atmospheric
Research) data
  • Temperature, geopotential height and zonal wind
    distribution in the tropo- and stratosphere
  • in December, January and February during 1948
    and 2007 period of NCEP re-analysis
  • 2,50 2,50 grid, 6 hours interval
  • Global Grids with 144x73 points
  • 1000, 500, 400, 300, 200, 100, 30, 10 hPa levels
  • Scientific Reference
  • Kistler, R., E. Kalnay, W. Collins, S. Saha,
    G. White, J. Woollen, M. Chelliah, W. Ebisuzaki,
    M. Kanamitsu, V. Kousky, H. van den Dool, R.
    Jenne, M. Fiorino, 2001Bulletin of the American
    Meteorological Society, Feb2001, Vol. 82 Issue 2,
    p247

8
  • SPW1 amplitude variations (geopotential height)
  • 30 hPa level, 62.5 north

9
Interpretation of wavelet spectra for travelling
waves
  • If AwAe --gt
  • ÃwAw-Ae, Ãspw2Ae, Ãe0
  • If AwltAe,
  • ÃeAe-Aw, Ãspw2Aw, Ãw0
  • Ãe, Ãw recalculated eastward and westward PW
    amplitudes
  • Ãspw recalculated periodical change of SPW
    amplitudes

10
Amplitude wavelet spectra for SPW
11
Amplitude wavelet spectra for travelling PW
12
Averaged over 1959-2007 spectra for SPW and
westward propagating waves m1, 30 hPa level,
62 N
See next slide (enlaged image)
SPW
Westward wave
13
Averaged over 1959-2007 Spectra for SPW and
westward propagating wavesm1, 30 hPa level, 62
N
SPW
Westward wave
14
Variability of SPW and 5 day wave amplitudes,
m1, 30 hPa level, 62 N




15
Variability of the 10 and 16 - day wave
amplitudes, m1, 30 hPa level, 62 N




16
Summary and results
  • during the last decades the winter-time averaged
    amplitude of SPW1 increases at the higher-middle
    latitudes of the Northern Hemisphere
  • the growth in the amplitude of the stratospheric
    vacillations
  • the amplitudes of longer-period normal
    atmospheric modes or the so-called 10- and 16-day
    waves diminish
  • stratospheric dynamics becomes more stochastic
  • Growth of vacillations amplitude leads to
    increasing travelling PW amplitudes but it isnt
    so. Possible reason is CO2 concentration rising
    (intensifying of radiative dumping and resonance
    quality fall escpessially for normal modes of low
    frequency).

17
Future work
  • perform similar analysis for July to estimate
    interhemispheric differences
  • Estimate the tropospheric manifestations of the
    changes in stratospheric dynamics, and effects in
    the upper atmosphere caused by these changes

18
Thank you for attention !
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