Marine stratocumulus cloud regimes exert a strong climatic influence through their high solar reflectivity. Human-induced changes in stratocumulus clouds, attributed to an increase of the aerosol burden (indirect effects), can be significant given the cloud decks proximity to the continents; nevertheless, the magnitude and the final climatic consequences of these changes are uncertain. This thesis investigates further the interactions between aerosols, cloud microphysics, regional circulation, and radiative response in the Southeast Pacific stratocumulus cloud deck, one of the largest and most persistent cloud regimes in the planet. Specifically, three different aspects are addressed by this thesis: The importance of the synoptic atmospheric variability in controlling cloud microphysical and radiative changes, a validation analysis of satellite retrievals of cloud microphysics from MOderate Resolution Imaging Spectroradiometer (MODIS), and the quantitative assessments of cloud aerosol interactions along with their associated radiative forcing using primarily aircraft remote sensing data. Synoptic and satellite-derived cloud property variations for the Southeast Pacific region associated with changes in coastal satellite-derived cloud droplet number concentration (Nd) are analyzed through a composite technique. MAX and MIN Nd composites are defined by the top and bottom terciles of daily area-mean Nd values over the Arica Bight, the region with the largest mean oceanic Nd, for the five October months of 2001, 2005, 2006, 2007, and 2008. The MAX-Nd composite is characterized by a weaker subtropical anticyclone and weaker winds than the MIN-Nd composite. Additionally, the MAX-Nd composite clouds over the Arica Bight are thinner than the MIN-Nd composite clouds, have lower cloud tops, lower near-coastal cloud albedos, and occur below warmer and drier free tropospheres. At 85˚W, the top-of-atmosphere shortwave fluxes are significantly higher (50%) for the MAX-Nd, with thicker, lower clouds and higher cloud fractions than for the MIN-Nd. The change in Nd at this location is small, suggesting that the MAX-MIN Nd composite differences in radiative properties primarily reflects synoptic changes. The ability of MODIS level 2 retrievals to represent the cloud microphysics is assessed with in-situ measurements of droplet size distributions, collected during the VAMOS Ocean-Cloud-Atmosphere-Land Study Regional Experiment (VOCALS-REx). The MODIS cloud optical thickness (t) correlates well with the in-situ values with a positive bias (1.42). In contrast, the standard 2.1 micron-derived MODIS cloud effective radius (r_e) is found to systematically exceed the in-situ cloud-top r_e, with a mean bias of 2.08 um. Three sources of errors that could contribute to the MODIS r_e positive bias are investigated further: the spread of the cloud droplet size distribution, the presence of a separate drizzle mode, and the sensor viewing angles. The sensor zenith viewing angles were found to have little impact, while the algorithm assumption about the cloud droplet spectra and presence of a precipitation mode could affect the retrievals but not by enough to fully explain the positive MODIS r_e bias. The droplet spectra effects account for r_e offsets smaller than 0.6 um, 0.9 um, and 1.6 um for non-drizzling, light-drizzling, and heavy-drizzling clouds respectively. An explanation for the observed MODIS bias is lacking although three-dimensional radiative effects were not considered. This investigation supports earlier studies documenting a similar bias, this time using data from newer probes. MODIS r_e and t were also combined to estimate a liquid water path (LWP) and Nd. A positive bias was also apparent in LWP, and attributed to r_e. However, when selected appropriate parameters a priori, the MODIS Nd estimate was found to agree the best with the insitu aircraft observations of the four MODIS variables. Lastly, the first aerosol indirect effect (Twomey effect) is explicitly investigated with VOCALS-REx observations, collected during three daytime research flights (Nov 9, 11, and 13), utilizing an aerosol-cloud interactions metric, and defined as ACI=dln(t)/dln(Na), with Na corresponding to the accumulation mode aerosol concentration, t derived from a broadband pyranometer, and ACI binned by cloud LWP derived from a millimeter-wavelength radiometer. Aircraft remote sensing estimates of the ACI, during sub-cloud transects, show that the cloud aerosol-interactions are strong and close to the maximum theoretical value for thin clouds, with a decrease of ACI with LWP. Although an explanation for the dependence of ACI on LWP is lacking, we found that a decrease in ACI with LWP is associated with decreases in both surface meridional winds and Nd. Similar to ACI, albedo fractional changes due to Nd fractional changes also tended to be smaller for higher LWPs, but with an overall radiative forcing larger than conservative global estimates obtained in global circulation models. The findings of this thesis emphasize the strong stratocumulus albedo response to an aerosol perturbation and its dependence on the regional scale atmospheric configuration. The results presented here can be used as a benchmark for testing regional and climate models, as well as helping to improve the current parameterizations of the first aerosol indirect effect.

The marine stratocumulus clouds are highly sensitive to aerosol perturbations. In this study, we have explored the cloud susceptibility to aerosol using satellite observation and multi-model simulations over the Southeast Pacific Ocean (SEP). The climatology of satellite observation indicates that SEP is a relatively clean area with low aerosol optical depth (AOD). The SEP is a region of marine stratocumulus deck with cloud fraction (CF) reaching as high as 90% in many regions, with relatively low (140 cm−3) cloud droplet number concentration (CDNC) over the marine environment, and it increases as it moves towards the coast. The joint histogram analysis shows that the AOD-CDNC relation shows positive sensitivity and a non-linear CDNC-LWP (liquid water path) relationship; however, a negative sensitivity is dominant. The multimodel analysis shows that most models have a strong positive AOD-CDNC sensitivity, suggesting that the cloud albedo effect leads to net cooling. The general circulation models (GCM) reveal a negative radiative forcing (-0.28 to -1.36Wm−2) at the top of the atmosphere (TOA) when using the flux method. It supports the positive AODCDNC sensitivity and the resulting negative radiative forcing in GCMs. However, the CDNC-LWP shows a diverse relation in the models. In the GCMs, the effect of cloud microphysics is not considered while estimating the net radiative forcing. To include the effect of cloud microphysics in the radiative forcing estimates, we have proposed a statistical approach to calculate the net radiative forcing. The results show that the net radiative forcing is sensitive to the LWP change due to the aerosol perturbation. / Die marinen Stratocumulus-Wolken reagieren sehr empfindlich auf Aerosol-Störungen. In dieser Studie haben wir die Anfälligkeit der Wolken für Aerosol anhand von Satellitenbeobachtungen und Multi-Modellsimulationen über dem Südostpazifik (SEP) untersucht. Die Klimatologie der Satellitenbeobachtung zeigt, dass der SEP ein relativ sauberes Gebiet mit geringer Aerosol optischer Dicke (AOD) ist. Der SEP ist eine Region mit mariner Stratocumulus-Decke mit einer Wolkbedeckungsgrad (CF), der in vielen Regionen bis zu 90% erreicht, mit einer relativ niedrigen (140 cm−3) Wolkentröpfchenanzahlkonzentration (CDNC) über der marinen Umgebung, und sie nimmt in Richtung Küste zu. Die gemeinsame Histogramm-Analyse zeigt, dass die AOD-CDNC-Beziehung eine positive Sensitivität und eine nicht-lineare CDNC-LWP-Beziehung (Flüssigwasserpfad) aufweist; allerdings ist eine negative Sensitivität vorherrschend. Die Multi-Modellanalyse zeigt, dass die meisten Modelle eine stark positive AOD-CDNC-Empfindlichkeit aufweisen, was darauf hindeutet, dass der Wolkenalbedo-Effekt eine Nettokühlung bewirkt. Die allgemeinen Zirkulationsmodelle (GCM) zeigen einen negativen Strahlungsantrieb (-0,28 bis -1,36Wm−2) am Oberrand der Atmosphäre (TOA), wenn die Flussmethode verwendet wird. Dies unterstützt die positive AOD-CDNC-Empfindlichkeit und den daraus resultierenden negativen Strahlungsantrieb in GCMs. Der CDNC-LWP zeigt jedoch unterschiedliche Abhängigkeiten in den Modellen. In den GCMs wird die Wirkung der Wolkenmikrophysik bei der Abschätzung des Netto-Strahlungsantriebs nicht berücksichtigt. Um die Auswirkungen der Wolkenmikrophysik auf den Strahlungsantrieb einzubeziehen, haben wir einen statistischen Ansatz zur Berechnung des Nettostrahlungsantriebs gewählt. Die Ergebnisse zeigen, dass der Nettostrahlungsantrieb empfindlich auf die LWP-Änderung durch die Aerosolstörung reagiert.

Cette thèse s’intéresse aux interactions entre l’océan et l’atmosphère dans le Pacifique Sud-Est, à des échelles comprises entre 10 et 300 km ("meso-échelle" océanique). Des observations satellites et un modèle couplé à haute résolution (1/12°) sont utilisés pour mettre en évidence et caractériser la relation entre la meso-échelle de température de surface de la mer (SST) et celle de l’intensité de la tension de vent (TV). Les observations montrent qu’environ un tiers de la meso-échelle de l’intensité de la TV est expliquée par les anomalies de la SST. L’intensité de la réponse de la TV aux anomalies de SST présente des variations spatiales et un cycle saisonnier marqué, également reproduits par le modèle. Une analyse de l’ajustement de la couche limite atmosphérique aux anomalies de meso-échelle de la SST dans les simulations permet d’expliquer ce cycle saisonnier et de comprendre l'origine des variations de la TV et de la vitesse du vent. Le modèle permet également d'étudier les conséquence de la modulation des flux à l’interface air-mer par la meso-échelle de SST et de courant de surface sur la dynamique océanique du Pacifique Sud-Est. D’une part, près de la côte, la réponse de la TV à la présence du front de SST diminue l’intensité de l’upwelling et la génération d’énergie cinétique turbulente (EKE) par instabilité barocline. La réponse de l’atmosphère à la meso-échelle de SST a également une rétroaction négative sur les anomalies de SST. D’autre part, la modulation de la TV par les courants de surface diminue la génération d’EKE par le travail des anomalies de TV, et créé un pompage d’Ekman qui atténue les anomalies de meso-échelle de la hauteur du niveau de la mer. / This PhD thesis studies the air/sea interactions at the oceanic mesoscale (10-300 km) in the South-East Pacific and their consequences. Satellite observations and a high-resolution regional ocean-atmosphere coupled model are used to evidence and characterize the mesoscale Sea Surface Temperature (SST)-wind stress (WS) interactions. Offshore from 150km, observations show that one third of the WS mesoscale intensity is explained by the SST mesoscale anomalies. The intensity of the WS response intensity to the SST displays similar spatial and seasonal variability in both the model and the observations. The simulation is further analyzed to study this variations and to understand the boundary layer adjustment mechanisms. A momentum balance evidenced that the near surface wind anomalies are created by the anomalies of the turbulent mixing term. It is shown that WS intensity anomalies due to SST anomalies are are mainly forced by mixing coefficient anomalies and partially compensated by wind shear anomalies. The consequences on the oceanic dynamics of the air-sea momentum, heat and fresh water fluxes by mesoscale SST and surface current are investigated in the simulations. On one hand, near the coast, the WS response to the upwelling SST front decreases both the upwelling and the eddy kinetic energy (EKE) generation by baroclinic conversion. A negative feedback of the atmospheric response on the SST anomalies amplitude is also evidenced. On the other hand, the WS modulation by oceanic surface currents decreases the EKE generation by the mesoscale wind work. It also creates an Ekman pumping centered above the eddies and attenuating sea surface height anomalies.

Les derniers 22 kans sont marqués par des évènements climatiques rapides, non synchrones entre l‘hémisphère Sud et le Nord. Un mécanisme de bascule des températures polaires, amplifié par la capacité de l‘océan profond à stocker et à restituer une partie du CO₂ atmosphérique en fonction de l‘intensité de la circulation océanique et des upwellings le long de la divergence Australe, a été proposé pour expliquer ces évènements. L‘objectif principal de cette thèse a été de définir quel est le rôle de l‘Océan Austral durant ces variations climatiques rapides à l‘aide de 3 carottes sédimentaires marines, prélevées le long de la marge chilienne, sous l‘influence des fronts océaniques et des vents d‘Ouest. La reconstitution des températures océaniques de surface (SST) ont permis de retracer l‘évolution du gradient latitudinal de SST au cours des derniers 22 kans mettant en évidence des migrations vers le sud du front Subtropical, notamment durant la déglaciation,marqués par des changements faunistiques en foraminifères planctoniques et benthiques suggérant unapport accru de nutriments en surface, et accompagnés par un enrichissement en [O₂] dans l‘eau de fond. Ces évènements sont peut-être liés à un renforcement des upwellings au niveau de la divergence australe induisant un renforcement de la ventilation des eaux intermédiaires antarctiques. Ces variations hydrologiques se produisent durant la hausse de CO₂ atmosphérique enregistrée dans les carottes de glace antarctiques pendant la déglaciation, indiquant un lien intime entre les upwellings, l‘intensité de la ventilation des eaux intermédiaires et le transfert de CO₂ depuis l‘océan profond vers l‘atmosphère. / The last 22 kyr are marked by abrupt climatic events, non-synchronous between the southern and northern hemispheres. A see-saw mechanism of the polar temperatures, amplified by the deep oceanability to store and release a portion of atmospheric CO₂, depending on the intensity of the thermohaline circulation and the large upwellings along the southern divergence, has been proposed to explain these observations. The main aim of this thesis was to assess the role of the southern ocean during these millennial events, by studying 3 marine cores, retrieved along the Chilean margin, under the influence of oceanic fronts and the westerly winds. The reconstruction of the sea surface temperatures (SST) allowed tracing the evolution of the SST latitudinal gradient during the last 22 kyr, highlighting southward migrations of the Subtropical Front, especially during the deglaciation, marked by benthic and planktonic foraminifera faunal changes which can be interpreted as surface nutrients inputs increase, accompanied by an enrichment of the bottom water [O₂] in the bottom water. These events could be related to stronger upwellings at the southern divergence leading to an increase of the Antarctic intermediate waters ventilation. These changes occur during atmospheric CO₂ increases recorded in Antarctic ice cores, marking the deglaciation, and suggesting an intimate link between upwellings, the intensity of the intermediate waters ventilation, and deep ocean-atmosphere CO₂ transfers.