Ground-based detection of sprites and their parent lightning flashes over Africa during the 2006 AMMA campaign

Sprites have been detected in video camera observations from Niger over mesoscale convective systems in Nigeria during the 2006 AMMA (African Monsoon Multidisciplinary Analysis) campaign The parent lightning flashes have been detected by multiple Extremely Low Frequency (ELF) receiving stations worldwide The recorded charge moments of the patent lightning flashes are often in excellent agreement between different receiving sites, and are furthermore consistent with conventional dielectric breakdown in the mesosphere as the origin of the sprites Analysis of the polarization of the horizontal magnetic field at the distant receivers provides evidence that the departure from linear magnetic polarization at ELF is caused primarily by the clay night asymmetry of the Earth-ionosphere cavity Copyright (C) 2009 Royal Meteorological Society

Características e distribuição das descargas atmosféricas e dos sistemas precipitantes produtores de raios na Amazônia Oriental

Este trabalho analisou 10 anos de distribuição espacial e temporal dos raios, dos sistemas precipitantes e suas características, como refletividade, temperatura de brilho e altura dos sistemas precipitantes amostrados pelo satélite Tropical Rainfall Measuring Mission (TRMM) através dos sensores Lightning Imaging Sensor (LIS), Precipitation Radar (PR) e TRMM Microwave Imager (TMI). Estes dados foram organizados e armazenados pelo grupo de pesquisa da convecção tropical da University of Utah no período de dezembro de 1997 a fevereiro de 2009. Também foram analisados dados de focos de queimadas detectadas pelo Instituto Nacional de Pesquisas Espaciais (INPE), no período de 1998 a 2008. Foi selecionada uma área delimitada entre 60ºW a 45ºW de longitude e 10ºS a 5ºN de latitude, a qual, posteriormente, foi dividida em nove sub-áreas para um melhor detalhamento dasinformações. Para verificar a possível influência das queimadas no número de raios, selecionaram-se oito áreas, sendo 4 com o maior número de focos de queimadas e 4 com o menor número de focos de queimadas. Os sistemas precipitantes foram classificados seguindo a metodologia de Nesbitt et. al. 2000 e obedecendo a nova definição dos dados realizado por Liu (2007). Os sistemas precipitantes amostrados pelo satélite TRMM utilizados neste trabalho são denominados ALLPFS e são definidos como aqueles que apresentam pixel de chuva estimado pelo algoritmo 2A25. Estes são classificados em PFS e OTHPFS, que respectivamente, são aqueles que apresentam e não apresentam informação de temperatura de brilho. Os PFS são sub-classificados em sistemas sem assinatura de gelo (NOICE), com assinatura de gelo (WICE) e sistemas convectivos de mesoescala (MCS), sendo que os sistemas mais intensos, dentre estes últimos, são sistemas que recebem a denominação de IMCS. Os resultados mostram que as regiões do sul do Estado do Pará, município de Belém e Ilha do Marajó foram as que apresentaram as maiores ocorrências de raios na Amazônia Oriental, com valores superiores a 20 a 35 raios/km^²/ano. Os NOICEs foram os sistemas mais frequentes em todas as regiões e os sistemas precipitantes da categoria WICE e MCS são aqueles que mais contribuem com a produção de raios sobre essas regiões. Os sistemas eletrificados apresentam grande contribuição no volume de chuva estimada sobre as áreas CENTRO e SUL, com percentuais superiores a 50% nas áreas SUL. A variação mensal dos raios na área de estudo mostrou que as maiores ocorrências de raios sobre o município de Belém são nos meses de janeiro a junho, com um pico no mês de janeiro. As maiores ocorrências no setor SUL da Amazônia Oriental concentram-se nos meses de setembro a dezembro. Nas análises sobre a interação entre os raios e as queimadas não se observou coerência, dentro das áreas de maior número de queimadas, na correlação mensal entre os raios e as queimadas, evidenciando que, apesar do grande número de queimadas observado sobre essas áreas, outros fatores interferem na produção de raios.

Análise de desempenho de índices de instabilidade atmosférica na previsão de fenômenos convectivos de mesoescala na região metropolitana de São Paulo entre 28 de janeiro e 04 de fevereiro de 2004

Discute-se o potencial prognóstico de índices de instabilidade para eventos convectivos de verão na Região Metropolitana de São Paulo. Cinco dos oito dias do período analisado foram considerados chuvosos, com observação de tempestades a partir do meio da tarde. O Índice K (IK) obteve valores abaixo de 31 nos 5 eventos, afetado pela presença de uma camada fria e seca em níveis médios da atmosfera em relação aos baixos níveis. O Índice Total Totals (ITT) falhou na detecção de severidade em 3 dos 5 eventos, apresentando valores inferiores ao mínimo limiar tabelado para fenômenos convectivos (ITT < 44) nesses dias. O Índice Levantado (IL) variou entre -4.9 e -4.3 em todos os 5 casos, valores associados a instabilidade moderada. O Índice de Showalter (IS) indicou possibilidade de tempestades severas em 4 dos 5 casos. Tanto o IS como o CAPE Tv tiveram seus valores fortemente reduzidos em uma sondagem com camada isotérmica entre 910 e 840 hPa. As séries temporais de CAPE Tv e IL mostraram significativa concordância de fase, com alta correlação linear entre ambas. CINE Tv ≈ 0 J kg-1 em associação com baixo cisalhamento vertical e com IS, IL e CAPE Tv, pelo menos moderados, parecem ser fatores comuns em dias de verão com chuvas abundantes e pequena influência da dinâmica de grande escala na área de estudo.

Relationship between Amazon biomass burning aerosols and rainfall over La Plata Basin

High aerosol loads are discharged into the atmosphere by biomass burning in Amazon and Central Brazil during the dry season. These particles can interact with clouds as cloud condensation nuclei (CCN) changing cloud microphysics and radiative properties and, thereby, affecting the radiative budget of the region. Furthermore, the biomass burning aerosols can be transported by the low level jet (LLJ) to La Plata Basin where many mesoscale convective systems (MCS) are observed during spring and summer. This work proposes to investigate whether the aerosols from biomass burning may affect the MCS in terms of rainfall over La Plata Basin during spring. Since the aerosol effect is very difficult to isolate because convective clouds are very sensitive to small environment disturbances, detailed analyses using different techniques are used. The binplot, 2D histograms and combined empirical orthogonal function (EOF) methods are used to separate certain environment conditions with the possible effects of aerosol loading. Reanalysis 2, TRMM-3B42 and AERONET data are used from 1999 up to 2012 during September-December. The results show that there are two patterns associated to rainfall-aerosol interaction in La Plata Basin: one in which the dynamic conditions are more important than aerosols to generate rain; and a second one where the aerosol particles have a role in rain formation, acting mainly to suppress rainfall over La Plata Basin.

North American Monsoon GPS Transect Experiment 2013

Ten GPS-Met stations were installed in northwest Mexico from June - September 2013. Each station included a Trimble NetR9 GPS receiver for PWV and a Vaisala WXT520 surface meteorological package measuring wind speed and direction, air temperature, humidity, pressure and precipitation. The geographic location, elevation and data period for each station are provided in Serra et al. (2016). The GPS receiver at Rayon failed on July 16, 21 days after installation, thus these data are not included in the archive but are available upon request (yserra@uw.edu). Data include 1-min surface meteorological variables, while the GPS PWV is calculated at 5-min intervals. A full description of the experiment can be found in Serra et al., 2016: Bull. Am. Meteor. Soc., doi: 10.1175/BAMS-D-14-00250.1.

Influence of the sea state on Mediterranean heavy precipitation: a case-study from HyMeX SOP1

Sea state can influence the turbulent air–sea exchanges, especially the momentum flux, by modifying the sea-surface roughness. The high-resolution non-hydrostatic convection-permitting model MESO-NH is used here to investigate the impact of a more realistic representation of the waves on heavy precipitation during the Intense Observation Period (IOP) 16a of the first HyMeX Special Observation Period (SOP1). Several quasi-stationary mesoscale convective systems developed over the western Mediterranean region, two of them over the sea, and resulted in heavy precipitation on the French and Italian coasts on 26 October 2012. Three different bulk parametrizations are tested in this study: a reference case (NOWAV) without any wave effect, a parametrization taking into account theoretical wave effects (WAV) and a last one with realistic wave characteristics from the MFWAM analyses (WAM). Using a realistic wave representation in WAM significantly increases the roughness length and the friction velocity with respect to NOWAV and WAV. The three MESO-NH sensitivity experiments of the IOP16a show that this surface-roughness increase in WAM generates higher momentum fluxes and directly impacts the low-level dynamics of the atmosphere, with a slowdown of the 10 m wind, when and where the wind speed exceeds 10 m s−1 and the sea state differs from the idealized one. The turbulent heat fluxes are not significantly influenced by the waves, these fluxes being controlled by the moisture content rather than by the wind speed in the simulations. Although the convective activity is globally well reproduced by all the simulations, the difference in the low-level dynamics of the atmosphere influences the localization of the simulated heavy precipitation. Objective evaluation of the daily rainfall amount and of the 10 m wind speed against the observations confirms the positive impact of the realistic wave representation on this simulation of heavy precipitation.

Study of different atmospheric environments associated to storms development in the Madeira Island

The study aims to improve the understanding about different atmospheric environments leading to the development of storms associated with heavy precipitation in Madeira Island. For this purpose, four main goals have been considered: 1) To document the synoptic and mesoscale environments associated with heavy precipitation. 2) To characterize surface precipitation patterns that affected the island during some periods of significant accumulated precipitation using numerical modelling. 3) To study the relationship between surface precipitation patterns and mesoscale environments. 4) To highlight how the PhD findings obtained in the first three goals can be translated into an operational forecast context. Concerning the large scale environment, precipitation over the island was favoured by weather systems (e.g, mesoscale convective systems and low pressure systems), as well as by the meridional transport of high amount of moisture from a structure denominated as “Atmospheric River”. The tropical origin of this moisture is underscored, however, their impact on the precipitation in Madeira was not so high during the 10 winter seasons [2002 – 2012] studied. The main factor triggering heavy precipitation events over the island is related to the local orography. The steep terrain favours orographically-induced stationary precipitation over the highlands, although maximum of precipitation at coastal region may be produced by localized blocking effect. These orographic precipitating systems presented different structures, associated with shallow and deep convection. Essentially, the study shows that the combination of airflow dynamics, moist content, and orography is the major mechanism that produces precipitation over the island. These factors together with the event duration act to define the regions of excessive precipitation. Finally, the study highlights two useful points for the operational sector, regarding the meridional water vapour transport and local effects causing significant precipitation over the Island; RESUMO: O estudo procura melhorar o entendimento sobre os diferentes ambientes atmosféricos que favorecem o desenvolvimento de tempestades associadas com precipitação intensa na ilha da Madeira. Nesse sentido foram definidos quatro objetivos: 1) Documentar os ambientes sinópticos e de mesoescala associados com precipitação intensa; 2) Caracterizar padrões de precipitação na superfície, em eventos de elevada precipitação acumulada, utilizando modelação numérica; 3) Estudar as relações entre os padrões de precipitação e ambientes de mesoescala; 4) Mostrar como tais resultados podem ser utilizados num contexto operacional de previsão do tempo. Em relação a ambientes de larga escala, verificou-se que a ocorrência de eventos de precipitação intensa sobre a ilha foi favorecida por sistemas meteorológicos, assim como pelo transporte meridional de humidade por meio de estruturas atualmente denominadas Rios atmosféricos. Neste último caso é de destacar a origem tropical de humidade, no entanto, o seu impacto na precipitação sobre a Madeira durante os 10 invernos estudados [2002-2012] não foi tão elevada. O principal fator que favorece os eventos de precipitação intensa está relacionado com a orografia local. O terreno complexo da ilha favorece a ocorrência de precipitação estacionária induzida orograficamente sobre as terras mais altas, embora a precipitação nas zonas costeiras possa ser produzida por um efeito localizado de bloqueio. Estes sistemas orográficos precipitantes apresentaram diferentes estruturas, associados a convecção pouco profunda e profunda. O estudo mostra que a combinação entre as características do escoamento, a quantidade de humidade, e a orografia são os condimentos essenciais para o desenvolvimento da precipitação sobre a ilha, atuando de maneira a definir as regiões de precipitação excessiva. Por fim, o estudo destaca dois pontos que podem ser úteis na previsão do tempo operacional, ligados a larga escala e aos efeitos locais, os quais podem levar ao desenvolvimento de tempestades e precipitação intensa sobre a ilha.

Does convective aggregation need to be represented in cumulus parameterizations?

Tropical deep convection exhibits a variety of levels of aggregation over a wide range of scales. Based on a multisatellite analysis, the present study shows at mesoscale that different levels of aggregation are statistically associated with differing large-scale atmospheric states, despite similar convective intensity and large-scale forcings. The more aggregated the convection, the dryer and less cloudy the atmosphere, the stronger the outgoing longwave radiation, and the lower the planetary albedo. This suggests that mesoscale convective aggregation has the potential to affect couplings between moisture and convection and between convection, radiation, and large-scale ascent. In so doing, aggregation may play a role in phenomena such as “hot spots” or the Madden-Julian Oscillation. These findings support the need for the representation of mesoscale organization in cumulus parameterizations; most parameterizations used in current climate models lack any such representation. The ability of a cloud system-resolving model to reproduce observed relationships suggests that such models may be useful to guide attempts at parameterizations of convective aggregation.

Deep Convective System Evolution over Africa and the Tropical Atlantic

In the tropical African and neighboring Atlantic region there is a strong contrast in the properties of deep convection between land and ocean. Here, satellite radar observations are used to produce a composite picture of the life cycle of convection in these two regions. Estimates of the broadband thermal flux from the geostationary Meteosat-8 satellite are used to identify and track organized convective systems over their life cycle. The evolution of the system size and vertical extent are used to define five life cycle stages (warm and cold developing, mature, cold and warm dissipating), providing the basis for the composite analysis of the system evolution. The tracked systems are matched to overpasses of the Tropical Rainfall Measuring Mission satellite, and a composite picture of the evolution of various radar and lightning characteristics is built up. The results suggest a fundamental difference in the convective life cycle between land and ocean. African storms evolve from convectively active systems with frequent lightning in their developing stages to more stratiform conditions as they dissipate. Over the Atlantic, the convective fraction remains essentially constant into the dissipating stages, and lightning occurrence peaks late in the life cycle. This behavior is consistent with differences in convective sustainability in land and ocean regions as proposed in previous studies. The area expansion rate during the developing stages of convection is used to provide an estimate of the intensity of convection. Reasonable correlations are found between this index and the convective system lifetime, size, and depth.

Perturbation growth at the convective scale for CSIP IOP18

The Met Office Unified Model is run for a case observed during Intensive Observation Period 18 (IOP18) of the Convective Storms Initiation Project (CSIP). The aims are to identify the physical processes that lead to perturbation growth at the convective scale in response to model-state perturbations and to determine their sensitivity to the character of the perturbations. The case is strongly upper-level forced but with detailed mesoscale/convective-scale evolution that is dependent on smaller-scale processes. Potential temperature is perturbed within the boundary layer. The effects on perturbation growth of both the amplitude and typical scalelength of the perturbations are investigated and perturbations are applied either sequentially (every 30 min throughout the simulation) or at specific times. The direct effects (within one timestep) of the perturbations are to generate propagating Lamb and acoustic waves and produce generally small changes in cloud parameters and convective instability. In exceptional cases a perturbation at a specific gridpoint leads to switching of the diagnosed boundary-layer type or discontinuous changes in convective instability, through the generation or removal of a lid. The indirect effects (during the entire simulation) are changes in the intensity and location of precipitation and in the cloud size distribution. Qualitatively different behaviour is found for strong (1K amplitude) and weak (0.01K amplitude) perturbations, with faster growth after sunrise found only for the weaker perturbations. However, the overall perturbation growth (as measured by the root-mean-square error of accumulated precipitation) reaches similar values at saturation, regardless of the perturbation characterisation.

Finite departure from convective quasi-equilibrium: periodic cycle and discharge-recharge mechanism

A simple self–contained theory is proposed for describing life cycles of convective systems as a discharge–recharge process. A closed description is derived for the dynamics of an ensemble of convective plumes based on an energy cycle. The system consists of prognostic equations for the cloud work function and the convective kinetic energy. The system can be closed by intro ducing a functional relationship between the convective kinetic energy and the cloud–base mass flux. The behaviour of this system is considered under a bulk simplification. Previous cloud–resolving mo delling as well as bulk statistical theories for ensemble convective systems suggest that a plausible relationship would be to assume that the convective kinetic energy is linearly proportional to the cloud–base mass flux. As a result, the system reduces to a nonlinear dynamical system with two dependent variables, the cloud–base mass flux and the cloud work function. The fully nonlinear solution of this system always represents a periodic cycle regardless of the initial condition under constant large–scale forcing. Importantly, the inclusion of energy dissipation in this model does not in itself lead the system to an equilibrium.

Case-to-case variability of predictability of deep convection in a mesoscale model

Successful quantitative precipitation forecasts under convectively unstable conditions depend on the ability of the model to capture the location, timing and intensity of convection. Ensemble forecasts of two mesoscale convective outbreaks over the UK are examined with a view to understanding the nature and extent of their predictability. In addition to a control forecast, twelve ensemble members are run for each case with the same boundary conditions but with perturbations added to the boundary layer. The intention is to introduce perturbations of appropriate magnitude and scale so that the large-scale behaviour of the simulations is not changed. In one case, convection is in statistical equilibrium with the large-scale flow. This places a constraint on the total precipitation, but the location and intensity of individual storms varied. In contrast, the other case was characterised by a large-scale capping inversion. As a result, the location of individual storms was fixed, but their intensities and the total precipitation varied strongly. The ensemble shows case-to-case variability in the nature of predictability of convection in a mesoscale model, and provides additional useful information for quantitative precipitation forecasting.

Photochemie der Troposphäre in niedrigen und mittleren Breiten: Die Rolle von Konvektion

Ozon (O3) ist in der Atmosphäre ein wichtiges Oxidanz und Treibhausgas. Während die höchsten Konzentrationen in der Stratosphäre beobachtet werden und die vor der gefährlichen UV-Strahlung schützende Ozonschicht bilden, können sich signifikante Änderungen der Ozon-Konzentration in der Region der Tropopause auf das Klima der Erde auswirken. Des Weiteren ist Ozon eine der Hauptquellen für das Hydroxylradikal (OH) und nimmt damit entscheidend Einfluss auf die Oxidationskraft der Atmosphäre. Der konvektive Transport von Ozon und seinen Vorläufergasen aus Regionen nahe der Erdoberfläche in die freie Troposphäre beeinflusst das Budget dieser Spezies in der Tropopausenregion.rnDie Datengrundlage der Studie in der vorliegenden Arbeit basiert auf den flugzeuggetragenen Messkampagnen GABRIEL 2005 (Suriname, Südamerika) sowie HOOVER I 2006 und HOOVER II 2007 (beide in Europa). Mit dem zur Verfügung stehenden Datensatz wird das Ozonbudget in der freien, unbelasteten Hintergrundatmosphäre und in der durch hochreichende Konvektion gestörten, oberen Troposphäre untersucht. Anhand der auf in-situ Messungen von O3, NO, OH, HO2 und dem aktinischen Strahlungsfluss basierten Berechnung der Netto-Ozonproduktionsrate (NOPR) werden für das Messgebiet Ozontendenzen in der unbelasteten Troposphäre abgeleitet und mit Simulationen des globalen Chemie-Transport-Modells MATCH-MPIC verglichen. Mit Hilfe zweier Fallstudien in den Tropen in Südamerika und den mittleren Breiten in Europa werden die Auswirkungen von hochreichender Konvektion auf die obere Troposphäre quantifiziert.rnDie Ergebnisse zeigen für die Grenzschicht in niedrigen und mittleren Breiten eine eindeutige Tendenz zur Produktion von Ozon, was für den tropischen Regenwald in der Messregion nicht der allgemeinen Erwartung entsprach, nach der diese Region durch die Zerstörung von Ozon charakterisiert sein sollte. In der oberen Troposphäre ab etwa 7 km wird für die beiden Regionen eine leichte Tendenz zur Ozonproduktion beobachtet. Signifikante Unterschiede zeigen die Ergebnisse für die mittlere Troposphäre. Während die Tropen in dieser Region durch eine eindeutige Tendenz zur Zerstörung von Ozon charakterisiert sind, lässt sich über den mittleren Breiten zwar eine hohe photochemische Aktivität aber keine derart klare Tendenz feststellen. Die hohen Breiten zeichnen sich durch eine neutrale Troposphäre in Bezug auf die Ozontendenz aus und weisen kaum photochemische Aktivität auf. Der Vergleich dieser Ergebnisse mit dem MATCH-MPIC Modell zeigt in weiten Teilen der Messregionen eine grundlegende Übereinstimmung in der Tendenz zur Produktion oder Zerstörung von Ozon. Die absoluten Werte werden vom Modell aber generell unterschätzt. Signifikante Unterschiede zwischen in-situ Daten und Modellsimulationen werden in der Grenzschicht über dem tropischen Regenwald identifiziert.rnDer Einfluss der Konvektion ist durch eine signifikant erhöhte NOPR gekennzeichnet. In dieser Arbeit wird in den Tropen mit einem Median-Wert von 0.20 ppbv h−1 eine um den Faktor 3.6 erhöhte NOPR im Vergleich zur ungestörten oberen Troposphäre abgeschätzt. In den mittleren Breiten führt die um eine Größenordnung höhere NO-Konzentration zu einem Wert von 1.89 ppbv h−1, was einer Überhöhung um einen Faktor 6.5 im Vergleich zum ungestörten Zustand entspricht. Diese Ergebnisse zeigen für beide Regionen in der oberen Troposphäre eine erhöhte Ozonproduktion als Folge konvektiver Aktivität. rnrnHochreichende Konvektion ist zudem ein sehr effektiver Mechanismus für den Vertikaltransport aus der Grenzschicht in die obere Troposphäre. Die schnelle Hebung in konvektiven Wolken führt bei Spurengasen mit Quellen an der Erdoberfläche zu einer Erhöhung ihrer Konzentration in der oberen Troposphäre. Die hochgradig löslichen Spurenstoffe Formaldehyd (HCHO) und Wasserstoffperoxid (H2O2) sind wichtige Vorläufergase der HOx-Radikale. Es wird angenommen, dass sie aufgrund ihrer Löslichkeit in Gewitterwolken effektiv ausgewaschen werden.rnIn der vorliegenden Arbeit wird eine Fallstudie von hochreichender Konvektion im Rahmen des HOOVER II Projekts im Sommer 2007 analysiert. Am 19.07.2007 entwickelten sich am Nachmittag am Südostrand eines in nordöstlicher Richtung ziehenden mesoskaligen konvektiven Systems drei zunächst isolierte konvektive Zellen. Flugzeuggetragene Messungen in der Aus- und der Einströmregion einer dieser Gewitterzellen stellen einen exzellenten Datensatz bereit, um die Auswirkungen von hochreichender Konvektion auf die Verteilung verschiedener Spurengase in der oberen Troposphäre zu untersuchen. Der Vergleich der Konzentrationen von Kohlenstoffmonoxid (CO) und Methan (CH4) zwischen der oberen Troposphäre und der Grenzschicht deutet auf einen nahezu unverdünnten Transport dieser langlebigen Spezies in der konvektiven Zelle hin. Die Verhältnisse betragen (0.94±0.04) für CO und (0.99±0.01) für CH4. Für die löslichen Spezies HCHO und H2O2 beträgt dieses Verhältnis in der Ausströmregion (0.55±0.09) bzw. (0.61±0.08). Dies ist ein Indiz dafür, dass diese Spezies nicht so effektiv ausgewaschen werden wie angenommen. Zum besseren Verständnis des Einflusses der Konvektion auf die Budgets dieser Spezies in der oberen Troposphäre wurden im Rahmen dieser Arbeit Boxmodell-Studien für den Beitrag der photochemischen Produktion in der Ausströmregion durchgeführt, wobei die gemessenen Spezies und Photolysefrequenzen als Randbedingungen dienten. Aus den Budgetbetrachtungen für HCHO und H2O2 wird eine Auswascheffizienz von (67±24) % für HCHO und (41±18) % für H2O2 abgeschätzt. Das für H2O2 überraschende Ergebnis lässt darauf schließen, dass dieses Molekül in einer Gewitterwolke deutlich effektiver transportiert werden kann, als aufgrund seiner hohen Löslichkeit aus der Henry-Konstanten zu erwarten wäre. Das Ausgasen von gelöstem H2O2 beim Gefrieren eines Wolkentropfens, d.h. ein Retentionskoeffizient kleiner 1, ist ein möglicher Mechanismus, der zum beobachteten Mischungsverhältnis dieser löslichen Spezies in der Ausströmregion beitragen kann.

Topographic and meteorological influences on spatial scaling of heavy convective rainfall in mountainous regions

Characterizing the spatial scaling and dynamics of convective precipitation in mountainous terrain and the development of downscaling methods to transfer precipitation fields from one scale to another is the overall motivation for this research. Substantial progress has been made on characterizing the space-time organization of Midwestern convective systems and tropical rainfall, which has led to the development of statistical/dynamical downscaling models. Space-time analysis and downscaling of orographic precipitation has received less attention due to the complexities of topographic influences. This study uses multiscale statistical analysis to investigate the spatial scaling of organized thunderstorms that produce heavy rainfall and flooding in mountainous regions. Focus is placed on the eastern and western slopes of the Appalachian region and the Front Range of the Rocky Mountains. Parameter estimates are analyzed over time and attention is given to linking changes in the multiscale parameters with meteorological forcings and orographic influences on the rainfall. Influences of geographic regions and predominant orographic controls on trends in multiscale properties of precipitation are investigated. Spatial resolutions from 1 km to 50 km are considered. This range of spatial scales is needed to bridge typical scale gaps between distributed hydrologic models and numerical weather prediction (NWP) forecasts and attempts to address the open research problem of scaling organized thunderstorms and convection in mountainous terrain down to 1-4 km scales.

Dinâmica das configurações de formação e inibição das chuvas no Rio Grande do Norte: caracterização hidroclimática do estado

This study aimed to evaluate the influence of the main meteorological mechanisms trainers and inhibitors of precipitation, and the interactions between different scales of operation, the spatial and temporal variability of the annual cycle of precipitation in the Rio Grande do Norte. Além disso, considerando as circunstâncias locais e regionais, criando assim uma base científica para apoiar ações futuras na gestão da demanda de água no Estado. Database from monthly precipitation of 45 years, ranging between 1963 and 2007, data provided by EMPARN. The methodology used to achieve the results was initially composed of descriptive statistical analysis of historical data to prove the stability of the series, were applied after, geostatistics tool for plotting maps of the variables, within the geostatistical we opted for by Kriging interpolation method because it was the method that showed the best results and minor errors. Among the results, we highlight the annual cycle of rainfall the State which is influenced by meteorological mechanisms of different spatial and temporal scales, where the main mechanisms cycle modulators are the Conference Intertropical Zone (ITCZ) acting since midFebruary to mid May throughout the state, waves Leste (OL), Lines of instability (LI), breeze systems and orographic rainfall acting mainly in the Coastal strip between February and July. Along with vortice of high levels (VCANs), Complex Mesoscale Convective (CCMs) and orographic rain in any region of the state mainly in spring and summer. In terms of larger scale phenomena stood out El Niño and La Niña, ENSO in the tropical Pacific basin. In La Niña episodes usually occur normal or rainy years, as upon the occurrence of prolonged periods of drought are influenced by EL NIÑO. In the Atlantic Ocean the standard Dipole also affects the intensity of the rainfall cycle in State. The cycle of rains in Rio Grande do Norte is divided into two periods, one comprising the regions West, Central and the Western Portion of the Wasteland Potiguar mesoregions of west Chapada Borborema, causing rains from midFebruary to mid-May and a second period of cycle, between February-July, where rains occur in mesoregions East and of the Wasteland, located upwind of the Chapada Borborema, both interspersed with dry periods without occurrence of significant rainfall and transition periods of rainy - dry and dry-rainy where isolated rainfall occur. Approximately 82% of the rainfall stations of the state which corresponds to 83.4% of the total area of Rio Grande do Norte, do not record annual volumes above 900 mm. Because the water supply of the State be maintained by small reservoirs already are in an advanced state of eutrophication, when the rains occur, act to wash and replace the water in the reservoirs, improving the quality of these, reducing the eutrophication process. When rain they do not significantly occur or after long periods of shortages, the process of eutrophication and deterioration of water in dams increased significantly. Through knowledge of the behavior of the annual cycle of rainfall can have an intimate knowledge of how it may be the tendency of rainy or prone to shortages following period, mainly observing the trends of larger scale phenomena