10 research outputs found

    Convection in an African Easterly Wave over West Africa and the Eastern Atlantic: a Model Case Study of Hurricane Helene (2006) and its Interaction with the Saharan Air Layer

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    Convective systems over West Africa and the eastern Atlantic embedded in the African Easterly wave out of which Hurricane Helene (2006) developed are investigated by means of potential temperature and relative vorticity budgets. The tropical cyclogenesis of Helene was accompanied by several mineral dust outbreaks. The influence of the dust-radiation interaction on the processes leading to the formation of Helene is analysed. The study is based on COSMO and COSMO-ART model runs

    Mid-Level Dry Air Intrusions over the southern Maritime Continent

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    Patterns in extreme precipitation across the Maritime Continent in southeast Asia are known to be modulated by many processes, from large-scale modes of variability such as the Madden–Julian oscillation, to finer-scale mechanisms such as the diurnal cycle. Transient mid-level dry air intrusions are an example of a feature not extensively studied over the Maritime Continent, which has the potential to influence rainfall patterns. Here, we show that these dry air intrusions originate from upper level disturbances along the subtropical jet. Mid-level cyclonic circulation anomalies northwest of Australia from December to February (DJF) intensify westerlies in the southern Maritime Continent, advecting dry air eastward. In contrast, mid-level anticyclonic circulation anomalies northwest of Australia from June to August (JJA) intensify southern Maritime Continent easterlies, advecting dry air westward. The resultant transport direction of associated air parcels is also dependent on the seasonal low-level monsoon circulation. Dry air intrusions are important in influencing low-level wind and rainfall patterns, suppressing rainfall over seas near the southern Maritime Continent in both seasons, as well as over southern Maritime Continent islands in DJF and the Indian Ocean in JJA. In both seasons there is enhanced rainfall to the east of the intrusion, where there is moist return flow to the extratropics. This study highlights the importance of synoptic-scale extratropical features in influencing meteorological patterns in the Tropics

    Why is the tropical cyclone boundary layer not "well-mixed"?

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    Plausible diagnostics for the top of the tropical cyclone boundary layer include (i) the top of the layer of strong frictional inflow and (ii) the top of the “well-mixed” layer; that is, the layer over which potential temperature θ is approximately constant. Observations show that these two candidate definitions give markedly different results in practice, with the inflow layer being roughly twice the depth of the layer of nearly constant θ. Here, we will present an analysis of the thermodynamics of the tropical cyclone boundary layer derived from an axisymmetric model. We show that the marked dry static stability in the upper part of the inflow layer is due largely to diabatic effects. The radial wind varies strongly with height, and therefore so does radial advection of θ. This process also stabilizes the boundary layer, but to a lesser degree than diabatic effects. We also show that this differential vertical advection contributes to the observed superadiabatic layer adjacent to the ocean surface, where the vertical gradient of the radial wind is reversed, but that the main cause of this unstable layer is heating from turbulent dissipation. The top of the “well-mixed” layer is thus distinct from the top of the boundary layer in tropical cyclones. The top of the inflow layer is a better proxy for the top of the boundary layer, but is not without limitations. These results may have implications for boundary-layer parameterisations that diagnose the boundary layer depth from thermodynamic, or partly thermodynamic, criteria

    Revisiting gradient wind balance in tropical cyclones using dropsonde observations

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    This study diagnoses the degree of gradient wind balance (GWB) in dropsonde observations of 30 tropical cyclones (TCs) divided into 91 intense observation periods. The diagnosed GWB in these observation periods are composited to investigate which characteristics of a TC are significantly related to departures from GWB. This analysis confirms that on average the flow above the boundary layer is approximately in GWB. Supergradient flow is more common near the radius of maximum wind (RMW) in the upper boundary layer than above in the free troposphere or outside the RMW and is also more common in strong storms than in weak storms. In contrast, the degree of GWB does not differ between intensifying, steady‐state and weakening storms. Storms with a peaked wind profile have a higher probability of showing supergradient winds than those with a flat wind profile. The comparison of two commonly used functions to fit observations shows that the diagnosing GWB from dropsonde observations is highly dependent on the analysis technique. The agradient wind magnitude and even sign is shown to depend on which of these functions is used to fit the observations. The use of a polynomial fit consistently diagnoses the presence of supergradient winds far more frequently than a piece‐wise function, and also shows a marked degree of imbalance above the boundary layer. Therefore, caution is warranted when determining the degree of GWB with a polynomial fit

    The role of density currents and gravity waves in the offshore propagation of convection over Sumatra

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    The Maritime Continent experiences some of the world's most severe convective rainfall, with an intense diurnal cycle. A key feature is offshore propagation of convection overnight, having peaked over land during the evening. Existing hypotheses suggest this propagation is due to the nocturnal land breeze and environmental wind causing low-level convergence; and/or gravity waves triggering convection as they propagate. We use a convection-permitting configuration of the Met Office Unified Model over Sumatra to test these hypotheses, verifying against observations from the Japanese Years of the Maritime Continent field campaign. In selected case studies there is an organised squall line propagating wit the land breeze density current, possibly reinforced by convective cold pools, at approx. 3 m s-1 to around 150-300 km offshore. Propagation at these speeds is also seen in a composite diurnal cycle. The density current is verified by observations, with offshore low-level wind and virtual potential temperature showing a rapid decrease consistent with a density current front, accompanied by rainfall. Gravity waves are identified in the model with a typical phase speed of 16 m s-1. They trigger isolated cells of convection, usually further offshore and with much weaker precipitation than the squall line. Occasionally, the isolated convection may deepen and the rainfall intensify, if the gravity wave interacts with a substational pre-existing perturbation such as shallow cloud. The localised convection triggered by gravity waves does not generally propagate at the wave's own speed, but this phenomemon may appear as propagation along a wave trajectory in a composite that averages over many days of the diurnal cycle
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