Three semi-permanent cloud bands exist in the Southern Hemisphere extending southeastward from the equator, through the tropics, and into the subtropics. The most prominent of these features occurs in the South Pacific and is referred to as the South Pacific Convergence Zone (SPCZ). Similar convergence zones, with less intensity, exist in the South Atlantic (SACZ) and Indian (SICZ) oceans. We attempt to explain the physical mechanisms that promote the diagonal orientation of the SPCZ and the processes that determine the timescales of its variability. It is argued that the slowly varying sea surface temperature patterns produce upper tropospheric wind fields that vary substantially in longitude. Regions where 200 hPa zonal winds decrease with longitude (i.e., negative zonal stretching deformation, or dU/dx<0) reduce the group speed of the eastward propagating synoptic (3-6 day period) Rossby waves and locally increase the wave energy density. Such a region of wave accumulation occurs in the vicinity of the SPCZ, thus providing a physical basis for the diagonal orientation and earlier observations that the zone acts as a "graveyard" of propagating synoptic disturbances. In essence, dU/dx=0 demarks the boundary of the graveyard while regions where dU/dx<0 denote the graveyard itself. Composites of the life cycles of synoptic waves confirm this hypothesis. From the graveyard hypothesis comes a more general theory accounting for the SPCZ's spatial orientation and its longer term variability influenced by the El Niño-Southern Oscillation (ENSO), or alternatively, the changing background SST associated with different phases of ENSO.

Les zones de convergence sont des objets clés à la compréhension de la dynamique de la lithosphère. Elles sont le siège de déformations majeures comme en témoignent la concentration et l’intensité des séismes qui leur sont associées. A plus grande échelle de temps et d'espace, ces déformations résultent généralement en un empilement d’unités dont l’étude offre l'accès aux différents niveaux structuraux mis en jeu dans l'organisation de la chaîne de montagnes. Caractériser précisément la dynamique de structuration de ces unités ainsi que les paramètres contrôlant cette dynamique constitue une étape cruciale permettant d’aller plus loin, notamment quantitativement, dans notre connaissance de la dynamique lithosphérique. Cette thèse a comme double objectif (1) de préciser le comportement rhéologique des roches aux conditions Pressions-Température P-T du faciès éclogitique au sein de l' interface de subduction et (2) de caractériser et quantifier l' influence de la rhéologie de la plaque supérieure, et plus spécifiquement, le rôle de sa partie crustale, sur l'évolution spatio-temporelle des zones de convergence. Pour cela, une approche multi-disciplinaire a été utilisée. Dans un premier temps, je présente une analyse multi-échelle couplant travail de terrain et de pétrologie métamorphique qui a permis d'étudier la déformation au sein de roches HP-BT à l' interface de subduction au niveau de la klippe du Mont-Emilius (Alpes occidentales, Italie). Je détaille ensuite une étude quantitative alliant modélisation numérique thermo-mécanique 3D et 2D de zones de convergence. L'ensemble des modèles a permis d'analyser de nombreux paramètres influençant la structure rhéologique de la plaque supérieure tels que le géotherme initial, l'épaisseur de la lithosphère et de la croûte et la nature des matériaux impliqués. L'ensemble des modèles réalisés sont contraints/confrontés par/aux des données issues d'exemples naturels. Les résultats de l'étude sur des roches déformées au sein de l’interface de subduction mettent en évidence le possible comportement cassant des roches à des conditions de pression et température de l'ordre de 2.15-2.40 GPa, 500-550 °C, i.e., dans le faciès éclogitique. L’enregistrement d’un tel mode de déformation est d'une importance capitale car il remet en question le paradigme d’un comportement ductile sans résistance au niveau de l’ interface de subduction. Les résultats obtenus via les modèles numériques montrent par ailleurs que la rhéologie de la plaque supérieure, ainsi que celle de sa seule partie crustale, a une influence de premier ordre sur la dynamique globale des zones de convergence en modifiant notamment le mode de subduction, la cinématique de la fosse, le mode d'exhumation lors d'une collision, le timing de la déchirure du slab et de la formation de bassins d'arrière-arc, la répartition et l'intensité de la déformation au sein de la plaque supérieure. La combinaison des méthodes de pétrologie et de modélisation numérique a permis d'obtenir une analyse quantifiée de l' influence de la rhéologie des lithosphères impliquées dans les zones de convergence sur la dynamique de ces zones. Cette thèse présente ainsi de nouvelles contraintes à notre compréhension de la réponse mécanique de la lithosphère, en fonction de sa structuration rhéologique et de sa place au sein des zones de convergence à petite et grande échelle. Les nouvelles données présentées révèlent l' impact majeur de la rhéologie de la lithosphère dans les zones de convergence. Ce paramètre amène ainsi à reconsidérer notre vision actuelle des zones de convergence. / Convergence zones are key objects to the understanding of the lithosphere dynamics. They are the location correspond to places of intense deformation as evidenced by the concentration and magnitude of recorded earthquakes. On a larger scale of time and space, these deformations generally result in nappes stacking whose study offers access to the different structural levels involved in the mountain belt structuration. Precisely characterizing the structuring dynamics of these units as well as the parameters controlling this dynamic is a crucial step that would allow in particular a better quantification of lithospheric dynamics. The aim of this thesis is twofold: (1) clarifying the rheological behavior of rocks in the Pressure-Temperature (P-T) conditions of the eclogitic facies at the subduction interface and (2) characterizing and quantifying the influence of the overriding plate rheology, and more specifically, the role of its crustal part, on the spatio-temporal evolution of convergence zones. For this, I used a multi-disciplinary approach. First, I present a multi-scale analysis combining fieldwork and metamorphic petrology, which allowed me to study the deformation within High Pressure-Low Temperature (HP-LT) rocks at the subduction interface in the Mont-Emilius klippe (Western Alps, Italy). Then, I show the results of a quantitative study combining 3D and 2D thermo-mechanical modeling of convergence zones. The entire set of models allowed me to analyze different parameters influencing the rheological structure of the overriding plate, such as the initial geotherm, the thicknesses of the lithosphere and the crust, and the nature of the involved materials. All the performed models are constrained/compared by/with data from natural examples. The results of the study on deformed rocks within the subduction interface highlight the possible brittle behavior of rocks at pressure and temperature conditions on the order of 2.15-2.40 GPa and 500-550 °C, i.e., in the eclogitic facies. The recording of such a deformation mode is of paramount importance because it challenges the paradigm of subduction interface caracterized by ductile behavior without resistance. The results obtained with the numerical models show that the rheology of the overriding plate, as well as that of only its crustal part, has a first-order influence on the overall dynamics of the convergence zones by modifying the mode of subduction, trench kinematics, the mode of exhumation during collision, the timing for slab break-off and back-arc basin formation, the location and intensity of deformation within the overriding plate. The combination of petrology and numerical modeling methods allowed me to obtain a quantified analysis of the influence of the rheology of the lithospheres involved in convergence zones on the dynamics of these zones. This thesis presents new constraints for our understanding of the mechanical response of the lithosphere at different spatial scales as a function of its rheological structure. The new data presented here reveal the major impact of the lithosphere rheology in convergence zones. This parameter leads us to reconsider our current view of the convergence zones.

The east-west oriented cloud bands in the tropics are called the Inter-tropical Con-vergence Zones (ITCZ). Till recently, the ITCZ has been assumed to have a simple vertical structure with convergence near the surface boundary layer and divergence near the tropopause. Recent work has shown that the ITCZ can have a complex ver-tical structure with multi-level ows. This complex structure has a profound impact on the mass, momentum and energy budget in the ITCZ. This thesis addresses the factors that govern the shallow meridional circulation that occurs in the ITCZ and the mechanisms that govern the abrupt poleward transition and the gradual poleward migration . The shallow meridional circulation forms when the boundary layer ow that con-verges in the ITCZ, rises above the boundary layer and diverges in the lower tropo-sphere. The ow above the boundary layer is in the direction opposite to the direction of the ow within the boundary layer. Some authors have argued that this is caused by the reversal of pressure gradients just above the boundary layer in response to strong sea surface temperature gradients. This hypothesis neglects the eect of plan-etary rotation on the ow and was found to be insucient to explain the formation of shallow meridional circulation. In the east Pacic ocean, the shallow circulation forms only to the south of the ITCZ when the ITCZ forms away from the equator, while it is absent when the ITCZ forms close to the equator. The aqua-planet simulations of the equatorial and the o-equatorial ITCZ were conducted using Community Atmosphere Model (CAM 3.0). The model used the Eulerian dynamical core with T42 horizontal resolution and 26 levels in vertical. Each simulation was run for 3 years and analysis of last six months was presented. The simulations reproduced the contrast in the vertical structure of the equatorial and o-equatorial ITCZ. The shallow circulation was simulated with-out the reversal of pressure gradients and the SST gradients were weakest when the shallow circulation was simulated. We have proposed a new mechanism for the exis-tence of shallow meridional circulation in the ITCZ. We have argued that, in Earth's atmosphere, the mean horizontal ow generally occurs in the direction perpendicular to the direction of applied pressure gradient due to the action of Coriolis force. If the local rotational eects of the ow (relative vorticity) cancels the action of the Coriolis force, then a ow along the pressure gradient is possible. We demonstrated that this condition was satised only to the south of the ITCZ when it forms away from the equator. The ITCZ is characterized by the maximum mass convergence in the boundary layer. The mass convergence is mainly caused by the deceleration of poleward ow in the boundary layer. When the ITCZ forms close to the equator, the ow in the boundary layer is a resultant of vector addition of three forces, a pressure gradient force in the north-south direction (i.e., the ow towards low pressure), a Coriolis force which acts in the east-west direction( perpendicular to the direction of the ow), and surface friction which opposes the resultant ow. When the ITCZ forms away from the equator a three way balance does not capture the dynamics of ow. As the poleward ow is accelerated towards low pressure, it has to advect a considerable amount of zonal momentum with it which acts to retard the poleward ow. This eect of advection of zonal momentum has to be included in the force balance to obtain an accurate estimate of the ow and associated convergence. The ITCZ acts like a heat engine. The energy is gained near the surface, some energy is transported towards pole while some is utilized in driving the meridional circulation. The rest is rejected near the tropopause. The transport within the troposphere occurs through the vertical or horizontal advection of the energy due to vertical and horizontal motions respectively. Our analysis of the ITCZ suggests that; a large amount of transport occurs through horizontal motions that was neglected in the previous studies. The detailed analysis suggests that the latent energy in the form of mass of water vapor is exported out of the ITCZ at dierent levels in association with the multilevel ows. The equatorial and the o-equatorial ITCZ are dierent because, evaporation is larger in the o-equatorial ITCZ when compared to the equatorial ITCZ. The ITCZ shows a strong sub-seasonal variability in its location in the Indian Ocean and the west Pacic Ocean during boreal summer. There are two favorable locations, one near the equator and another away from the equator, for formation of the ITCZ. The equatorial ITCZ either propagates abruptly or gradually to the o-equatorial location. A detailed analysis of moisture and momentum budget of the simulated abrupt and gradual propagations enabled us to separate the role of thermo-dynamic and dynamic processes. We found that, if the equatorial ITCZ would propa-gate abruptly or gradually to the o-equatorial location is decided by the availability of the water vapor in the boundary layer between the two locations of the ITCZ, i.e., by the thermodynamic processes. But, such a transition to the o-equatorial location is allowed only when the constraints imposed by the re-adjustment in the circulation are satised. In simple terms, these constraints emerge due to two processes. 1. The Earth (lower boundary of the atmosphere) spins at maximum eective radius near the equator. As a result, the atmosphere gains maximum angular momentum near the equator (`zonal momentum' in Cartesian co-ordinates) . The ITCZ is one of the primary avenues to transport the zonal momentum from the lower troposphere to the upper troposphere. When the favorable location of ITCZ is near the equator, the location of ITCZ and the location where atmosphere gains maximum zonal momentum are coincident. The ITCZ and associated meridional circulation transports the zonal momentum upwards which is then transported polewards. As the favorable location of ITCZ moves away from the equator, the two locations are die rent. As a result, the atmospheric ow has to re-adjust so that the zonal momentum is transported from the equator to the favorable location of the ITCZ which then transports it upwards and polewards. In summary, this thesis proposes a new mechanism for the generation of shallow meridional circulation, the abrupt transition and the gradual propagations of the ITCZ.