2007
DOI: 10.5194/acpd-7-11685-2007
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Equatorial wave analysis from SABER and ECMWF temperatures

Abstract: Abstract. Equatorial planetary scale wave modes such as Kelvin waves or Rossby-gravity waves are excited by convective processes in the troposphere. In this paper an analysis for these and other equatorial wave modes is carried out with special focus on the stratosphere using temperature data from the SABER instrument as well as ECMWF temperatures. Space-time spectra of symmetric and antisymmetric spectral power are derived to separate the different equatorial wave types and the contribution of gravity waves i… Show more

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Cited by 39 publications
(127 citation statements)
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“…Unlike equatorial wave analysis, it is not necessary to separate the temperature data into symmetrical and anti-symmetrical components (Ern et al, 2009). The temperature spectra are not red so it is not necessary to divide the results by a background spectrum (Alexander et al, 2008b;Ern et al, 2008). Henceforth we use the notation E1 to represent any eastward s = 1 planetary wave, W1 to represent any westward s = 1 planetary wave, and so on.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…Unlike equatorial wave analysis, it is not necessary to separate the temperature data into symmetrical and anti-symmetrical components (Ern et al, 2009). The temperature spectra are not red so it is not necessary to divide the results by a background spectrum (Alexander et al, 2008b;Ern et al, 2008). Henceforth we use the notation E1 to represent any eastward s = 1 planetary wave, W1 to represent any westward s = 1 planetary wave, and so on.…”
Section: Discussionmentioning
confidence: 99%
“…Waves with ground based periods of 4 days (the Nyquist period) to 32 days and |s| < 9 are considered here. When considering ground-based frequencies, as measured by COSMIC and other satellites, the location of a wave in wavenumber-frequency space will not change with altitude under the assumption of a slowly varying background field despite changes in the background wind with altitude (Ern et al, 2008). The largest variances and thus largest wave activity are due to waves with |s| ≤ 2.…”
Section: Space-time Spectramentioning
confidence: 99%
“…While the wave signal observed in the troposphere is located at relatively slow phase speeds and mostly directly coupled to the convective systems, Kelvin waves observed in the stratosphere are dominated by "free" wave modes, which are excited by deep convection in the troposphere but not longer linked with the space-time patterns of the convective forcing (Randel and Wu, 2005;Ern et al, 2008;Kiladis et al, 2009).…”
Section: Introductionmentioning
confidence: 99%
“…In addition, only little was known about the spectrum of Kelvin waves and its temporal variations. However, improved satellite sensors recently provide these information for the troposphere (e.g., Wheeler and Kiladis, 1999;Straub and Kiladis, 2003;Cho et al, 2004) as well as for the stratosphere (Ern et al, 2008;Alexander et al, 2008) and the mesosphere (Garcia et al, 2005;). In our work we additionally use European Centre for Medium-Range Weather Forecasts (ECMWF) analyses which assimilate tropospheric measurements of convection and rain rates and have been validated to well represent also the stratospheric Kelvin wave amplitudes (Ern et al, 2008) and also Kelvin wave fluxes and zonal wind forcing have been found to be in good agreement with measurements (Ern and Preusse, 2009).…”
Section: Introductionmentioning
confidence: 99%
“…McIntyre and Palmer, 1984;Riese et al, 2002), tropical wave modes (e.g. Canziani, 1999;Smith et al, 2002;Ern et al, 2008) and tides (e.g. Ward et al, 1999;Zhang, 2008).…”
Section: Introductionmentioning
confidence: 99%