Abstract

Abstract. Vertical temperature profiles obtained by radiosonde and Raman lidar measurements are used to investigate a climatology of total energy density of gravity waves (GW) in the Upper Troposphere (UT) and the Lower Stratosphere (LS) from 1992 to 2004 above Mahé (4° S, 55° E), Tromelin (15° S, 54° E) and La Réunion (21° S, 55° E) located in the tropical South-West Indian Ocean. The commonly used spectral index value (p≈5/3) of the intrinsic frequency spectrum is used for calculating estimated total energy density in the UT and LS. Estimated total energy density provides good estimation of total energy density in the LS but underestimates total energy density by one half in the UT above Mahé and Tromelin probably due to the activity of near-inertial frequency waves. Estimated total energy density reveals a strong seasonal variability as a function of latitude and convection as an evident active source of GW activity in the LS in austral summer. Above La Réunion, a semi-annual GW activity is observed in the LS with the signature of the subtropical barrier in the UT. Moreover, radiosondes and Raman lidar provide consistent GW surveys in the UT/LS at heights<23 km above La Réunion.

Highlights

  • Introduction150-m vertical resolution from January 1999 to May 2004 at 1830–1900 Upper Troposphere (UT)

  • Tropical atmospheric Gravity-Waves (GW) play a key role in exchanges between atmospheric layers in terms of transport of momentum and atmospheric constituents (Holton, 1975; Ehhalt et al, 1983)

  • To model observed GW patterns in simple models of middle atmosphere, recent investigations focused on the characteristics of GW sources and/or GW spectral parameters near sources in the Upper Troposphere (UT) and the Lower Stratosphere (LS)

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Summary

Introduction

150-m vertical resolution from January 1999 to May 2004 at 1830–1900 UT. Short-scale structures with vertical wavelengths

Experimental data
Gravity wave energy density
Full Text
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