Thibaut Dauhut

PhD in meteorology

Clouds above the beach

About me

Hi ! My name is Thibaut Dauhut.
I am a postdoctoral researcher at Max Planck Institute for Meteorology in Hamburg, Germany.
I study how deep convection transports air and water into the tropical lower stratosphere. This transport impacts the composition and the radiative properties of the stratosphere, both of key importance for the future of our climate. I work with cutting-edge Large-Eddy Simulations (LES), with resolutions as fine as 100 m. I investigate the small-scale processes (updrafts, low-level convergence, entrainment by cloud eddies, overshoots) that determine the capability of the very deep convective systems to hydrate the stratosphere.

My Journey

Thesis

The_three_Atmospheric_Circulations

Hector the Convector, the epitome of the tropical convection that hydrates the stratosphere

Thibaut Dauhut

PhD at Laboratoire d'Aérologie, Université de Toulouse and CNRS
Defended at Observatoire Midi-Pyrénées on 14 November 2016

The tropical thunderstorms play an uncertain role in the transport of tropospheric air into the stratosphere, limiting our capability to predict the future climate. The transport by the thunderstorms may be underestimated by the climate models, due to their coarse resolutions. The efficiency of this transport is analysed using numerical simulations of the thunderstorm Hector the Convector with resolutions down to 100 m, the finest ever used for a case of very deep convection. The overshoots, that were observed at its top at 18 km altitude, are captured and the net hydration of the stratosphere is quantified. The contribution of the tropical thunderstorms to the water flux from the troposphere to the stratosphere is then estimated to about 20 %. The almost convergence at 200 m and 100 m suggests that such resolutions are necessary to correctly represent the updafts. The individual analysis of the updrafts indicates that the two tallest contribute beyond 90 % of the mass flux into the stratosphere. They are larger, more vigorous and contain more water than the tallest updrafts one hour before and one hour after, and their convective core was weakly diluted. The supply from the surface by the convergence lines, intensified by the cold pools, and the weak dilution of the two tallest updrafts are determinant for the development of very deep convection. The isentropic analysis of the overturning inside Hector confirms the mass flux computed with the updrafts analysis. It corrects the estimate in the lower troposphere by taking into account the turbulent flux, and in the upper troposphere by filtering out the gravity waves. It highlights the importance of the latent heating due to freezing in the two tallest updrafts during the phase of overshoot in the stratosphere.

Reports

The_three_Atmospheric_Circulations

The atmospheric circulation led by convective heating in the frame of the Madden-Julian Oscillation

Thibaut Dauhut

Laboratoire de Météorologie Dynamique, ENS Paris, France
Internship of Master 2 from March to June 2012

The mechanisms of the eastward propagation of the Madden-Julian Oscillation (MJO) are still under investigation. The dynamical response of the troposphere to the convective heating induced by the active phase of MJO is studied here. It seems to be strengthened by the meridional gradient of the Earth surface temperature. It is modulated by the intensity, the extent and the variations of the convective heating. The mid-level westerly jet, west of the heating, seems to play a key role in the eastward MJO propagation. It extends eastward under the heating, up to a few degrees east beyond the heating center. The convergence of the low-level winds is shifted to the east, where the low-level winds and the energy fluxes from the surface are damped. Both the shift of the low-level convergence and the energy accumulation at the surface foster the displacement of the convection to the east of the heating center. Conversely, in this region, the subsiding flow warms the troposphere from the top, which rather inhibits the convection.

Isentropic streamfunctions of very deep Hector using theta_s with and without precipitation

The link between tropical cyclones in Australia and Rossby wave breaking

Thibaut Dauhut

Monash Weather And Climate, Melbourne, Australia
Internship of Master 1 from April to July 2011

This study focuses on one of the possible causes for tropical cyclogenesis in the Australian region during summer. Rossby wave breaking in the mid-latitudes could play a role in their formation by providing precursor vortices, which are subsequently transported towards the tropics where they promote organized convection. A detection method has been developed with the NC Language. Several statistical analyses have been used to determine the extent to which precursor anomalies have played a part over the past twenty years in the formation of tropical cyclones and tropical storms. The calculations are based on the ERAI dataset. About 10% of all tropical storms and cyclones are associated with potential vorticity anomalies from the mid-latitudes and, on average, those anomalies are detectable 5 days before the storms form. Despite the simplicity of the tracking method, which is potentially improvable, the results are encouraging, particularly for tropical weather forecasting.

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Transport of tracers by one of the tallest updrafts of Hector

Liquid films subjected to thermal strains

Thibaut Dauhut

GRASP, Université de Liege, Belgium
Internship of Licence 3 from May to June 2010

We form a liquid film using a solution of water – glycerol – surfactant that we hold in a vertical rectangular metallic frame. The film is made of two interfaces of surfactant between which the solution is confined. The solution flows downward between the interfaces causing the drainage phenomenon. The drainage is balanced by the solution supply at the top of the film. The top bar is a lengthways split cylinder in which the pump system injects the solution at a constant debit. The bottom bar heats the film on its full width as hot water flows through at a predefined temperature. The whole system reproduces typical Rayleigh-Bénard cells. The temperature fields in the film are recorded by an infra-red camera and the iMovie software. They are processed using imageJ and gnuplot software.