Planetary waves in the upper stratosphere and lower mesosphere during 2009 Arctic major stratospheric warming

The AURA-MLS daily mean temperatures and zonal wind from NASA-MERRA reanalysis for latitudes between 60° N and 80° N are used to investigate the planetary wave (PW) characteristics in the stratosphere and lower mesosphere during sudden stratospheric warming (SSW) (November 2008 to March 2009). Here,...

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Bibliographic Details
Published in:Annales Geophysicae
Main Authors: P. Kishore, I. Velicogna, M. Venkat Ratnam, J. H. Jiang, G. N. Madhavi
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2012
Subjects:
Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
Arctic
Merra
Online Access:https://doi.org/10.5194/angeo-30-1529-2012
https://doaj.org/article/2b164bc2f8f94bac9f9bca33feefa6dc
Description
Summary:The AURA-MLS daily mean temperatures and zonal wind from NASA-MERRA reanalysis for latitudes between 60° N and 80° N are used to investigate the planetary wave (PW) characteristics in the stratosphere and lower mesosphere during sudden stratospheric warming (SSW) (November 2008 to March 2009). Here, we used a novel method called empirical mode decomposition (EMD) to extract the PWs from the temperature data. The EMD is an interesting approach to decompose signals into locally periodic components, the intrinsic mode functions (IMFs), and will easily identify the embedded structures, even those with small amplitudes. The spectral analysis reveals prevailing planetary wave periods of ~6-day, ~8-day, ~15-day, and ~21–23-day in IMFs 1, 2, 3, and 4, respectively. Clear upward propagation of these waves (20–30 days) is observed, suggesting that sources for these oscillations are in the troposphere.

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