A method to improve the determination of wave perturbations close to the tropopause by using a digital filter

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Abstract

GPS radio occultation satellite data allowed to analyze in the last decade for the first time a large amount of atmospheric temperature profiles including both the troposphere and the stratosphere all over the globe. Wave amplitude enhancements have been systematically observed around tropopause levels, which are apparently due to artifacts generated by any digital filter used to isolate the wave components from these data. We present a new filtering method which can be equally applied to temperature or refractivity profiles. It was tested with synthetic temperature data based on NCEP reanalyes and observed wave climatologies and it was also statistically validated with GPS radio occultation profiles from the COSMIC mission. The suggested technique significantly reduces artificial enhancements around the tropopause, mainly at low latitudes, where a sharp lapse rate change usually exists. This represents an improvement in comparison to previous applications of standard filters. In addition it would allow the study of longer vertical wavelengths than previously done with other filtering procedures. © Author(s) 2011.

Figures

  • Fig. 1. A GPS RO temperature profile (solid), the background temperature determined by a filter (dashed) and their difference (dotted) on the right (Satellite CHAMP, lon = 293.81◦, lat =−18.55◦, 30 May 2001, 01:42 UTC).
  • Fig. 2. A unit pulse located at data point number 200 and the corresponding filter response with a low pass cut off equal to 50 times the uniform interval size on the horizontal axis between neighboring data points.
  • Fig. 3. Shown is (a) the RO temperature profile (solid) and the determined background temperature (dashed), (b) the bandpass filtered temperature (solid) and the background corresponding to large wavelengths (dashed), and (c) the double filtered temperature (Satellite COSMIC 1, lon = 239.36◦, lat =−2.38◦, 29 June 2010, 00:23 UTC).
  • Fig. 4. Same as Fig. 3 for a second GPS RO event (Satellite COSMIC 1, lon = 44.47◦, lat = 7.01◦, 21 March 2010, 16:20 UTC).
  • Fig. 6. Same as Fig. 5 for a second GPS RO event (Satellite COSMIC 1, lon = 95.29◦, lat =−23.02◦, 19 July 2010, 00:38 UTC).
  • Fig. 5. Bandpass (solid) and double filtered (dashed) relative temperature (black) and refractivity (gray) profiles of a GPS RO event (Satellite COSMIC 1, lon = 18.06◦, lat =−36.30◦, 19 July 2010, 19:07 UTC).
  • Fig. 7. Simulated mean average relative temperature variance and its uncertainty in the height interval 4–27 km against latitude: reference calculation (triangles) and the results for the complete (squares), separate (rhomboids) and double filtering (circles) procedures.
  • Fig. 8. Low, middle and high latitude mean temperature profiles from NCEP reanalyses zonally averaged during January 2007.

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CITATION STYLE

APA

Alexander, P., De La Torre, A., Llamedo, P., Hierro, R., Schmidt, T., Haser, A., & Wickert, J. (2011). A method to improve the determination of wave perturbations close to the tropopause by using a digital filter. Atmospheric Measurement Techniques, 4(9), 1777–1784. https://doi.org/10.5194/amt-4-1777-2011

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