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Volume 34, issue 2
Ann. Geophys., 34, 203–213, 2016
https://doi.org/10.5194/angeo-34-203-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 34, 203–213, 2016
https://doi.org/10.5194/angeo-34-203-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.

Regular paper 10 Feb 2016

Regular paper | 10 Feb 2016

Global distribution of vertical wavenumber spectra in the lower stratosphere observed using high-vertical-resolution temperature profiles from COSMIC GPS radio occultation

Noersomadi1 and T. Tsuda2 Noersomadi and T. Tsuda
  • 1Center of Atmospheric Science and Technology, National Institute of Aeronautics and Space (LAPAN), Bandung, Indonesia
  • 2Research Institute for Sustainable Humanosphere (RISH), Kyoto University, Kyoto, Japan

Abstract. We retrieved temperature (T) profiles with a high vertical resolution using the full spectrum inversion (FSI) method from the Constellation Observing System for Meteorology, Ionosphere and Climate (COSMIC) GPS radio occultation (GPS-RO) data from January 2007 to December 2009. We studied the characteristics of temperature perturbations in the stratosphere at 20–27 km altitude. This height range does not include a sharp jump in the background Brunt–Väisälä frequency squared (N2) near the tropopause, and it was reasonably stable regardless of season and latitude. We analyzed the vertical wavenumber spectra of gravity waves (GWs) with vertical wavelengths ranging from 0.5 to 3.5 km, and we integrated the (total) potential energy EpT. Another integration of the spectra from 0.5 to 1.75 km was defined as EpS for short vertical wavelength GWs, which was not studied with the conventional geometrical optics (GO) retrievals. We also estimated the logarithmic spectral slope (p) for the saturated portion of spectra with a linear regression fitting from 0.5 to 1.75 km.

Latitude and time variations in the spectral parameters were investigated in two longitudinal regions: (a) 90–150° E, where the topography was more complicated, and (b) 170–230° E, which is dominated by oceans. We compared EpT, EpS, and p, with the mean zonal winds (U) and outgoing longwave radiation (OLR). We also show a ratio of EpS to EpT and discuss the generation source of EpS. EpT and p clearly showed an annual cycle, with their maximum values in winter at 30–50° N in region (a), and 50–70° N in region (b), which was related to the topography. At 30–50° N in region (b), EpT and p exhibited some irregular variations in addition to an annual cycle. In the Southern Hemisphere, we also found an annual oscillation in EpT and p, but it showed a time lag of about 2 months relative to U. Characteristics of EpTand p in the tropical region seem to be related to convective activity. The ratio of EpT to the theoretical model value, assuming saturated GWs, became larger in the equatorial region and over mountainous regions.

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Short summary
We studied the characteristics of gravity waves in the lower stratosphere using high-vertical-resolution COSMIC GPS-RO temperature profiles retrieved by the FSI method. We analyzed vertical wavenumber spectrum of the normalized temperature perturbations and calculated the wave potential energy in the wavelength ranges from 0.5 to 3.5 and 0.5 to 1.75 km. We investigated the correlation between the spectral parameters with topography and the background mean zonal winds.
We studied the characteristics of gravity waves in the lower stratosphere using...
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