The Three Atmospheric Circulations over the Indian Ocean and the MaritimeContinent and Their Modulation by the Passage of the MJO
The Three Atmospheric Circulations over the Indian Ocean and the MaritimeContinent and Their Modulation by the Passage of the MJO
Daria Kuznetsova, Thibaut Dauhut and Jean-Pierre Chaboureau
Published on 28 November 2018
The passage of the Madden–Julian oscillation (MJO) over the Indian Ocean and the Maritime Continentis investigated during the episode of 23–30 November 2011. A Meso-NH convection-permitting simulationwith a horizontal grid spacing of 4 km is examined. The simulation reproduces the MJO signal correctly, showingthe eastward propagation of the primary rain activity.
A Third-Law Isentropic Analysis of a Simulated Hurricane
Reply to the Comments of Olivier Pauluis to the paper “A Third-Law Isentropic Analysis of a Simulated Hurricane”
Pascal Marquet and Thibaut Dauhut
Published on 10 August 2018
Detailed investigation of the moist-air entropy and its meaning for the atmospheric systems like the deep convective systems. The use of theta_s as a strict equivalent of the entropy is illustrated with the isentropic diagrams of Hector the Convector.
Giga-LES of Hector the Convector and Its Two Tallest Updrafts up to the Stratosphere
Giga-LES of Hector the Convector and Its Two Tallest Updrafts up to the Stratosphere
Thibaut Dauhut, Jean-Pierre Chaboureau, Juan Escobar and Patrick Mascart
Published on 7 December 2016
The updrafts inside Hector are identified using a clustering algorithm, that I developed to run on parallel supercomputers. Within more than 16 000 updrafts with vertical velocities larger than 10 m/s, only a dozen are 4-km tall. The two tallest only crontribute to more than 90% of the vertical mass flux across the tropical tropopause layer (TTL) and produce overshoots into the stratosphere.
The Atmospheric Overturning Induced by Hector the Convector
The Atmospheric Overturning Induced by Hector the Convector
Thibaut Dauhut, Jean-Pierre Chaboureau, Patrick Mascart and Olivier Paulius
Published on 20 September 2017
The overturning of Hector the Convector, a tropical multicellular convective system of northern Australia that regularly overshoots into the stratosphere, is synthesized at the scale of a large-eddy simulation. The isentropic analysis offers the advantage of filtering out the reversible motions due to gravity waves and taking into account the turbulent fluxes that contribute to the vertical transport. Two key circulations are charac- terized: the troposphere deep overturning and the mass exchange due to the overshoots into the stratosphere. The transition from deep to very deep convection is associated with a change in the diabatic tendency inside the tallest updrafts: the latent heat release due to the formation of a large amount of icy hydrometeors exceeds the loss of energy due to mixing with the drier, colder air of the environment.
Large-eddy simulations of Hector the convector making the stratosphere wetter
Large-eddy simulations of Hector the convector making the stratosphere wetter
Thibaut Dauhut, Jean-Pierre Chaboureau, Juan Escobar and Patrick Mascart
Published on 12 September 2014
A series of large-eddy simulations (LES) were performed for a Hector thunderstorm observed on 30 November 2005 over the Tiwi Islands. On that day, ice particles reaching 19-km altitude were measured. The LES developed overshooting updrafts penetrating the stratosphere that compared well with observations. While moistening appeared to be robust with respect to the grid spacing used, grid spacing on the order of 100 m may be necessary for a reliable estimate of hydration.
Near-inertial motions in the Brazil Current at 24°S-36°S: Observations by satellite tracked drifters
Near-inertial motions in the Brazil Current at 24°S-36°S: Observations by satellite tracked drifters
Arcilan T. Assireu, Thibaut Dauhut, Francisco A. dos Santos and João A. Lorenzzetti
Published on 12 July 2017
I did a one-year intership at the research institute for the natural ressources of the Federal University of Itajuba, Brazil.
During this period I characterised the near inertial currents (NICs) in the ocean and their link with the synoptic weather conditions.
All my results are presented in this study. I used the trajectories from drifters to examine motions in the inertial frequency band. The atmospheric conditions were favorable to NICs generations: the wind stress rotary spectrum is anticyclonically polarized with a near-inertial peak.
In the ocean, a large increase in the eddy kinetic energy is found in the f band south of 28°S. The predominance of NICs south of 28°S appears to be related to the Effective Coriolis Frequency.
Fennec dust forecast intercomparison over the Sahara in June 2011
Fennec dust forecast intercomparison over the Sahara in June 2011
Jean-Pierre Chaboureau, Cyrille Flamant, Thibaut Dauhut, Cécile Kocha, Jean-Philippe Lafore, Chistophe Lavaysse, Fabien Marnas, Mohamed Mokhtari, Jacques Pelon, Irene Reinares Martínez, Kerstin Schepanski, and Pierre Tulet
Published on 7 June 2016
The clustering algorithm, that I developed to run on parallel computers, can be used to identify any 2-D or 3-D meteorological strucutre. Here a nice example with the identification of the wind regimes over Africa, that latter lead to dust emission. Beside the harmattan (HRM), the cold pools (CPL) below some convective systems contribute to the observed large near-surface dust concentrations.
Overview of the Meso-NH model version 5.4 and its applications
Overview of the Meso-NH model version 5.4 and its applications
Christine Lac and co-authors
Published on 29 May 2018
The reference description of the tool I use to produce simulations: the non-hydrostatic atmospheric model Meso-NH.
