2008
DOI: 10.5194/acp-8-845-2008
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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 satellite 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 gravi… Show more

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Cited by 105 publications
(132 citation statements)
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“…7a shows amplitude variations that are strongly modulated by the QBO, with enhanced wave activity in periods of transition from easterly to westerly stratospheric wind (westerly shear zones). Similar results have been found by Randel and Wu (2005); Ern et al (2008); Alexander and Ortland (2010); Flannaghan and Fueglistaler (2013). These peaks in Kelvinwave activity are expected since Kelvin-wave energy is accumulated below the critical level, which is located near the zero-wind line.…”
Section: Temporal Variations In Kelvin-wave Activitysupporting
confidence: 85%
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“…7a shows amplitude variations that are strongly modulated by the QBO, with enhanced wave activity in periods of transition from easterly to westerly stratospheric wind (westerly shear zones). Similar results have been found by Randel and Wu (2005); Ern et al (2008); Alexander and Ortland (2010); Flannaghan and Fueglistaler (2013). These peaks in Kelvinwave activity are expected since Kelvin-wave energy is accumulated below the critical level, which is located near the zero-wind line.…”
Section: Temporal Variations In Kelvin-wave Activitysupporting
confidence: 85%
“…They include contributions of slow and quasi-stationary variations such as the annual cycle and interannual variability (El Niño-Southern Oscillation (ENSO) and the QBO). Sub-seasonal variability (periods shorter than 100 days) essentially contains signals of the MJO and equatorial waves (e.g., Wheeler and Kiladis, 1999;Ern et al, 2008). We isolate Kelvin-wave activity by selecting wave numbers k = +1 to +6, periods from 4 to 30 days, and equivalent depths from 8 to 240 m. After filtering, reverse fast Fourier transformations (FFTs) are applied to reconstruct atmospheric variability associated with individual types of waves.…”
Section: Gridding and Spectral Analysismentioning
confidence: 99%
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“…See also Preusse et al (2006), Eq. (10) in Ern et al (2008), and the discussion in Ern et al (2015).…”
Section: Satellite Observations Of Gravity Wave Amplitudes Momentum mentioning
confidence: 95%
“…For this purpose, longitude-time spectra are estimated for a fixed set of altitudes and latitudes. This procedure is described in detail in Ern et al (2011), and it accounts also for fast traveling planetary waves, such as shortperiod Kelvin waves (e.g., Ern et al, 2008;Ern and Preusse, 2009; or quasi 2-day waves (e.g., Ern et al, 2013). Tides, however, are removed separately, as described in Ern et al (2013).…”
Section: Satellite Observations Of Gravity Wave Amplitudes Momentum mentioning
confidence: 99%