Academic literature on the topic 'Meteorology Southern Hemisphere'

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Journal articles on the topic "Meteorology Southern Hemisphere"

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Salinger, Jim. "Meteorology of the Southern Hemisphere." Agricultural and Forest Meteorology 116, no. 1-2 (2003): 113–15. http://dx.doi.org/10.1016/s0168-1923(02)00250-2.

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Karoly, David J., and Dayton G. Vincent. "Meteorology of the Southern Hemisphere." Meteorological Monographs 49 (December 1, 1998): 1–410. http://dx.doi.org/10.1175/0065-9401-27.49.1.

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Diamond, Howard J., Neil Plummer, and Kevin Walsh. "Southern Hemisphere Meteorology and Oceanography." Bulletin of the American Meteorological Society 91, no. 2 (2010): 245–50. http://dx.doi.org/10.1175/2009bams2892.1.

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Vincent, Dayton G., and Johan van Heerden. "Fifth International Conference on Southern Hemisphere Meteorology and Oceanography." Bulletin of the American Meteorological Society 78, no. 10 (1997): 2227–31. http://dx.doi.org/10.1175/1520-0477-78.10.2227.

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Fletcher, Jennifer, Shannon Mason, and Christian Jakob. "The Climatology, Meteorology, and Boundary Layer Structure of Marine Cold Air Outbreaks in Both Hemispheres*." Journal of Climate 29, no. 6 (2016): 1999–2014. http://dx.doi.org/10.1175/jcli-d-15-0268.1.

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Abstract A comparison of marine cold air outbreaks (MCAOs) in the Northern and Southern Hemispheres is presented, with attention to their seasonality, frequency of occurrence, and strength as measured by a cold air outbreak index. When considered on a gridpoint-by-gridpoint basis, MCAOs are more severe and more frequent in the Northern Hemisphere (NH) than the Southern Hemisphere (SH) in winter. However, when MCAOs are viewed as individual events regardless of horizontal extent, they occur more frequently in the SH. This is fundamentally because NH MCAOs are larger and stronger than those in the SH. MCAOs occur throughout the year, but in warm seasons and in the SH they are smaller and weaker than in cold seasons and in the NH. In both hemispheres, strong MCAOs occupy the cold air sector of midlatitude cyclones, which generally appear to be in their growth phase. Weak MCAOs in the SH occur under generally zonal flow with a slight northward component associated with weak zonal pressure gradients, while weak NH MCAOs occur under such a wide range of conditions that no characteristic synoptic pattern emerges from compositing. Strong boundary layer deepening, warming, and moistening occur as a result of the surface heat fluxes within MCAOs.
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Newman, Paul A., Leslie R. Lait, and Mark R. Schoeberl. "The morphology and meteorology of southern hemisphere spring total ozone mini-holes." Geophysical Research Letters 15, no. 8 (1988): 923–26. http://dx.doi.org/10.1029/gl015i008p00923.

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Spensberger, Clemens, and Thomas Spengler. "Feature-Based Jet Variability in the Upper Troposphere." Journal of Climate 33, no. 16 (2020): 6849–71. http://dx.doi.org/10.1175/jcli-d-19-0715.1.

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AbstractJets in the upper troposphere constitute a cornerstone of both synoptic meteorology and climate dynamics, providing a direct link between weather and midlatitude climate variability. Conventionally, jet variability is often inferred indirectly through the variability of geopotential or sea level pressure. As recent findings pointed to physical discrepancies of this interpretation for the Southern Hemisphere, this study presents a global overview of jet variability based on automated jet detections in the upper troposphere. Consistent with previous studies, most ocean basins are dominated by variability patterns comprising either a latitudinal shift of the jet or a so-called pulsing, a broadening/narrowing of the jet distribution without a change in the mean position. Whereas previous studies generally associate a mode of storm track variability with either shifting or pulsing, jet-based variability patterns frequently represent a transition from shifting to pulsing, or vice versa, across the respective ocean basin. In the Northern Hemisphere, jet variability is consistent with geopotential variability, confirming earlier analyses. In the Southern Hemisphere, however, the variability of geopotential and jets often indicates different modes of variability. Notable exceptions are the consistent dominant modes of jet and geopotential variability in the South Pacific and, to a lesser extent, the south Indian Ocean during winter, as well as the dominant modes in the South Atlantic and south Indian Ocean during summer. Finally, tropical variability is shown to modulate the jet distribution in the Northern Hemisphere, which is in line with previous results. The response in the Southern Hemispheric, however, is shown to be markedly different.
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Levy, Gad. "Southern hemisphere low level wind circulation statisticsfrom the Seasat scatterometer." Annales Geophysicae 12, no. 1 (1994): 65–79. http://dx.doi.org/10.1007/s00585-994-0065-9.

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Abstract. Analyses of remotely sensed low-level wind vector data over the Southern Ocean are performed. Five-day averages and monthly means are created and the month-to-month variability during the winter (July-September) of 1978 is investigated. The remotely sensed winds are compared to the Australian Bureau of Meteorology (ABM) and the National Meteorological Center (NMC) surface analyses. In southern latitudes the remotely sensed winds are stronger than what the weather services' analyses suggest, indicating underestimation by ABM and NMC in these regions. The evolution of the low-level jet and the major stormtracks during the season are studied and different flow regimes are identified. The large-scale variability of the meridional flow is studied with the aid of empirical orthogonal function (EOF) analysis. The dominance of quasi-stationary wave numbers 3, 4, and 5 in the winter flow is evident in both the EOF analysis and the mean flow. The signature of an exceptionally strong blocking situation is evident in July and the special conditions leading to it are discussed. A very large intraseasonal variability with different flow regimes at different months is documented.
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Huth, R., and P. O. Canziani. "Classification of hemispheric monthly mean stratospheric potential vorticity fields." Annales Geophysicae 21, no. 3 (2003): 805–17. http://dx.doi.org/10.5194/angeo-21-805-2003.

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Abstract. Monthly mean NCEP reanalysis potential vorticity fields at the 650 K isentropic level over the Northern and Southern Hemispheres between 1979 and 1997 were studied using multivariate analysis tools. Principal component analysis in the T-mode was applied to demonstrate the validity of such statistical techniques for the study of stratospheric dynamics and climatology. The method, complementarily applied to both the raw and anomaly fields, was useful in determining and classifying the characteristics of winter and summer PV fields on both hemispheres, in particular, the well-known differences in the behaviour and persistence of the polar vortices. It was possible to identify such features as sudden warming events in the Northern Hemisphere and final warming dates in both hemispheres. The stratospheric impact of other atmospheric processes, such as volcanic eruptions, also identified though the results, must be viewed at this stage as tentative. An interesting change in behaviour around 1990 was detected over both hemispheres.Key words. Meteorology and atmospheric dynamics (middle atmosphere dynamics; general circulation; climatology)
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Aghedo, A. M., S. Rast, and M. G. Schultz. "Sensitivity of tracer transport to model resolution, prescribed meteorology and tracer lifetime in the general circulation model ECHAM5." Atmospheric Chemistry and Physics 10, no. 7 (2010): 3385–96. http://dx.doi.org/10.5194/acp-10-3385-2010.

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Abstract. Atmospheric transport of traces gases and aerosols plays an important role in the distribution of air pollutants and radiatively active compounds. For model simulations of chemistry-climate interactions it is important to know how the transport of tracers depends on the geographical resolution of the general circulation model. However, this aspect has been scarcely investigated until now. Here, we analyse tracer transport in the ECHAM5 general circulation model using 6 independent idealized tracers with constant lifetimes, which are released in two different altitudes at the surface and in the stratosphere, respectively. Model resolutions from T21L19 to T106L31 were tested by performing multi-annual simulations with prescribed sea surface temperatures and sea ice fields of the 1990s. The impacts of the tracer lifetime were investigated by varying the globally uniform exponential decay time between 0.5 and 50 months. We also tested the influence of using prescribed meteorological fields (ERA40) instead of climatological sea surface temperature and sea ice fields. Meridional transport of surface tracers decreases in the coarse resolution model due to enhanced vertical mixing, with the exception of the advection into the tropical region, which shows an inconsistent trend between the resolutions. Whereas, the meridional transport of tracers released in the stratosphere was enhanced with higher model resolutions, except in the transport from tropical stratosphere to the Southern Hemisphere, which exhibits an increase trend with increasing model resolution. The idealized tracers exhibit a seasonal cycle, which is modulated by the tracer lifetime. In comparison to the run with prescribed sea surface temperature and sea ice fields, the simulation with prescribed meteorological fields did not exhibit significant change in the meridional transport, except in the exchange of stratospheric tracers between both hemispheres, where it causes about 100% increase. The import of the surface tracers into the stratosphere is increased by up to a factor of 2.5, and the export from the stratosphere into the troposphere was increased by up to 60% when prescribed meteorological fields is used. The ERA40 simulation also showed larger interannual variability (up to 24% compared to 12% in the standard simulations). Using our surface tracers released in either the northern or Southern Hemisphere, respectively, we calculate inter-hemispheric transport times between 11 and 17 months, consistent with values reported in the literature. While this study cannot be used to relate differences in model results to specific changes in transport processes, it nevertheless provides some insight into the characteristics of tracer transport in the widely used ECHAM5 general circulation model.
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Dissertations / Theses on the topic "Meteorology Southern Hemisphere"

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Roux, David Gerhardus. "An investigation of the structure of the Southern Hemisphere radio-meteor streams." Thesis, Rhodes University, 1988. http://hdl.handle.net/10962/d1004587.

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Our current knowledge of the Solar System, with a particular emphasis on the systems of interplanetary objects, is reviewed, and the theory of meteors and the reflection of radio waves from meteoric ionization is then discussed. A description of the meteor radar is given and a method of calibrating the antenna beam is developed. The main project comprises two parts: (a) A general survey of the radar echorate for 20 major and minor meteor streams and the sporadic meteor background, conducted from Grahamstown over the period 1986 April to 1988 January, is described. Definite shower activity was observed for all of the major and some of the minor showers. (b) Based on a scheme proposed by previous workers (Morton & Jones), a method of recovering meteor radiant distributions from the distribution of echo directions is developed. We devise a technique of compensating for possible distortions of the resulting radiant maps, which may arise due to the arisotropic antenna beam. This involves a system of echo-weighting. Radiant maps which showed considerably less distortion than those of the above workers were obtained without the weighting procedure. It is concluded that, although the method in its present form introduces spurious features into the maps, the principle is sound and should eventually be refined to produce the desired compensation
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Ummenhofer, Caroline C. Mathematics &amp Statistics Faculty of Science UNSW. "Southern hemisphere regional precipitation and climate variability : extrems trends and prdictability." Awarded by:University of New South Wales. Mathematics & Statistics, 2008. http://handle.unsw.edu.au/1959.4/41253.

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This PhD thesis investigates the relative importance of oceanic and atmospheric influences on extremes, long-term trends, and seasonal to interannual variability of precipitation for different regions in the Southern Hemisphere in observations, reanalysis data, and output from general circulation models (GCM). Examination of interannual rainfall extremes over southwest Western Australia (SWWA) reveals a characteristic dipole pattern of Indian Ocean sea surface temperature anomalies (SSTA). This coincides with a large-scale reorganization of the wind field over the tropical/subtropical Indian Ocean changing SSTA, via anomalous Ekman transport in the tropical Indian Ocean and via anomalous air-sea heat fluxes in the subtropics, and altering moisture advection onto SWWA. The potential impact of these Indian Ocean SSTA in driving modulations of mid-latitude precipitation across southern and western regions of Australia is assessed in atmospheric GCM simulations. The SSTA give rise to changes in the thermal properties of the atmosphere, meridional thickness gradient, subtropical jet, thermal wind, and baroclinicity over southern regions of Australia, thus modulating precipitation. In addition, links between anomalous wet conditions over East Africa and these characteristic Indian Ocean SSTA are explored during the "short rain" season in October-November. Interannual extremes m New Zealand rainfall and their modulation by modes of Southern Hemisphere climate variability, namely the Southern Annular Mode (SAM) and El Nino-Southern Oscillation (ENSO), are investigated. Late twentieth Century trends in New Zealand precipitation are examined for the period 19792006 to quantify the relative impact of recent changes in the large-scale atmospheric circulation related to the SAM and ENSO. Increasingly drier conditions over much of New Zealand can be partially explained by the SAM and ENSO. Cool season rainfall variability in southeastern Australia is investigated via a classification and characterization of the predominant types of synoptic systems occurring in the region, focusing on frontal and cutoff low systems. Two definitions of the autumn break developed for northwestern Victoria are employed to produce a synoptic climatology of the break phenomenon. Trends in characteristics of the autumn break indicate that the most recent drought in southeastern Australia is comparable in severity with the two major droughts in the twentieth Century.
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Cao, Jing. "An investigation of transport during minor stratospheric warmings in the Southern Hemisphere." Diss., Georgia Institute of Technology, 1995. http://hdl.handle.net/1853/25964.

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Clark, Logan N. "Southern Hemisphere Pressure Relationships during the 20th Century - Implications for Climate Reconstructions and Model Evaluation." Ohio University / OhioLINK, 2020. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1586778291377432.

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Widlansky, Matthew J. "Climate dynamics of the South Pacific Convergence Zone and similarities with other subtropical convergence zones in the Southern Hemisphere." Diss., Georgia Institute of Technology, 2010. http://hdl.handle.net/1853/37095.

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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.
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Sleinkofer, Amanda M. "Antarctic Sea Ice Extent Reconstructions Throughout the 20th Century." Ohio University / OhioLINK, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1620313247537371.

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Silva, Alex Santos da. "Clima do Hemisfério Sul há 1,080 milhão de anos: impacto do derretimento da geleira Antártica." Universidade Federal de Viçosa, 2013. http://locus.ufv.br/handle/123456789/5262.

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Made available in DSpace on 2015-03-26T13:50:13Z (GMT). No. of bitstreams: 1 texto completo.pdf: 2950242 bytes, checksum: 87a3fed7b278be1081be57b42f6f0be6 (MD5) Previous issue date: 2013-07-24<br>Conselho Nacional de Desenvolvimento Científico e Tecnológico<br>The Earth s climate system is influenced by the topography configuration, whose importance is based on the characterization of the dynamic and thermodynamic aspects of the atmosphere and ocean. In this sense, the study aims to investigate the oceanic and atmospheric processes associated with the western Antarctic ice sheet collapse, which occurred 1.080 million years (ka) ago. Thus, two simulations were performed with the coupled climate model SPEEDO: a) the control simulation (CTRL) under current conditions and, b) forced simulation (1080ka), inserting the topography of 1.080 ka ago. Both simulations are conducted in the 2 CO atmospheric concentration of 380 ppmV. In the ocean circulation, the 1080ka simulation results show variations of salinity and temperature in relation to CTRL, at all ocean levels. Forcing contributed to an increase of approximately 1.4 °C and 1.6 °C in the sea surface temperature of the Ross and eastern Antarctic seas, plus the intensification of oceanic heat flux in the South Atlantic Ocean. On the other hand, there was an increase of 20 TW heat flow towards the north Pacific Ocean. These oceanic variations lead to changes in atmospheric circulations. The air temperature in the 1080ka simulation was 6.5 °C higher than CTRL in the Ross Sea region, contrary to the eastern region of Antarctic, where there was a decrease of 4.5 °C. In the precipitation field, there were an increase of approximately 160 mm/year in the Antarctic Peninsula and a decrease near 80 mm/year in the South Atlantic Ocean. The wind, at low levels, intensified in the South Atlantic anticyclone, moving towards South America continent. At high levels, the westward fluxes were weakened by the lower thermal gradient in the extratropical region. Although an intermediate complexity climate model was used, it was able to represent the main mass conservation mechanisms of the atmosphere and oceans.<br>O sistema climático da Terra é influenciado pela configuração da topografia, cuja importância fundamenta-se na caracterização dos aspectos dinâmicos e termodinâmicos da atmosfera e do oceano. Neste sentido, o objetivo do estudo é investigar os processos oceânicos e atmosféricos associados ao colapso das geleiras continentais da região oeste da Antártica, referente ao período de 1,080 milhão de anos (ka) passados. Para tal fim, foram realizadas duas simulações com o modelo climático acoplado SPEEDO: a) simulação controle (CTRL), sob condições atuais e; b) simulação forçada (1080ka), inserindo a topografia de 1,080 ka passados. Ambas as simulações são conduzidas com a concentração atmosférica de 2 CO em 380 ppmV. Na circulação oceânica, os resultados da simulação 1080ka mostram variações de salinidade e temperatura em relação à CTRL, em todos os níveis oceânicos. A forçante contribuiu para um aumento de aproximadamente 1,4 °C e 1,6 °C na temperatura da superfície do mar dos mares de Ross e a leste da Antártica, somados a intensificação do fluxo de calor oceânico ao sul do oceano Atlântico. Por outro lado, houve um acréscimo de 20 TW no fluxo de calor em direção ao norte do oceano Pacífico. Estas variações oceânicas conduzem a mudanças na circulação atmosférica. A temperatura do ar na simulação 1080ka foi 6,5 °C maior a CTRL na região do mar de Ross, inversamente a região leste da Antártica, onde ocorreu um decréscimo de 4,5 °C. No campo de precipitação, houve um aumento de aproximadamente 160 mm/ano na Península Antártica e uma diminuição próxima a 80 mm/ano no sul do Oceano Atlântico. O vento, em baixos níveis, foi intensificado no Anticiclone do Atlântico Sul, deslocando-se em direção ao continente sul-americano. Em altos níveis, os fluxos de oeste foram enfraquecidos, devido ao menor gradiente térmico meridional na região extratropical. Embora se tenha utilizado um modelo climático de complexidade intermediária, o mesmo foi capaz de representar os principais mecanismos de conservação de massa da atmosfera e dos oceanos.
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Tomas, Robert A. "Subseasonal variability in the Southern Hemisphere as simulated by a two-level atmospheric general circulation model." Thesis, 1987. http://hdl.handle.net/1957/29076.

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The dynamical nature of atmospheric disturbances in the Southern Hemisphere simulated by a two-level general circulation (GCM) model is studied. Time series of the dependent variables and diabatic heating components from 10 Southern Hemisphere winters (JJA) and summers (DJF) simulated by the Oregon State University two-level GCM are used. The time mean fields are presented and discussed. Variance and covariance analyses are performed to determine the geographical distribution, intensities and transport properties of high-frequency (periods between 2.5 and 10 days) and low-frequency (periods between 10 days and a season) transient eddies. These are discussed in terms of dynamical consistency with the time-mean circulation. It is found that the behavior of the high-frequency eddies at mid and high-latitudes is consistent with baroclinic instability theory, i.e., the eddies have properties similar to observed migratory weather disturbances. The low-frequency eddies appear to be quasi-stationary Rossby waves originating at middle latitudes. They seem to disperse energy in a manner consistent with arguments based on simple linear wave dynamics. During wintertime, the time mean flow directs eddies poleward where they grow by baroclinic processes. Also during wintertime, the slow phase velocity, fast group velocity and cyclic domain lead to quasi-resonant behavior on a hemispheric scale.<br>Graduation date: 1988
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Xulu, Nkosinathi Goodman. "Impact of spatio-temporal variability of the Mascarene High on weather and climate over Southern Africa." Diss., 2017. http://hdl.handle.net/11602/677.

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MENVSC (Climatology)<br>Department of Geography and Geo-Information Sciences<br>Subtropical anticyclones locate and modulate weather and climate over subtropical belts for both the Northern and Southern Hemispheres. This study investigates the spatio-temporal variability of the Mascarene High over the South Indian Ocean on (anomalous) weather and climate over southern Africa at intraseasonal, seasonal, interannual, multidecadal and event time-scales. The Mascarene High is located 25-35°S, 40-110°E, playing a vital role in day-to-day weather and climate patterns conditions over southern Africa. Spatio-temporal characteristics of the Mascarene High investigated in this study span the period 1985-2014 and 2071-2100, using NCEP-NCAR reanalysis datasets for present-day climate observations and the Conformal-Cubic Atmospheric Model (CCAM) for future projections. The Mascarene High is analysed using mean sea level pressure (MSLP) extracted from ECMWF ERA-interim monthly reanalysis data. The Mascarene High is also subjected to Principal Components Analysis, depicting eastern displacements of the weather system to be dominant for weather and climate fluctuations over southern Africa. The Mascarene High migrates south (north) during austral summer (winter) and is centred over the eastern Indian Ocean in summer in connection with the Indian Ocean Subtropical Dipole. Event scale analysis is also employed for investigating Mascarene High blocking and induced anomalous weather. Mascarene High blocking leads to anomalous rainfall events over southern Africa associated with tropical cyclones, cut-off lows and cloud bands. There is also a vital geographical variability of the Mascarene High development, distribution and movement in the South Indian Ocean at the different time-scales. Projections of the Mascarene High indicate a shift in mean location as a result of future expansion and intensification. This projected expansion and intensification is expected to shift tropical cyclone trajectories equatorward, with the baroclinic structure of cold fronts expected to shift poleward affecting changes in the weather and climate of southern Africa. This finding is important as it projects changes in weather and climate conditions over southern Africa in a changing climate due to increased greenhouse gas emissions.
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Books on the topic "Meteorology Southern Hemisphere"

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Karoly, David J., and Dayton G. Vincent, eds. Meteorology of the Southern Hemisphere. American Meteorological Society, 1998. http://dx.doi.org/10.1007/978-1-935704-10-2.

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NATO Advanced Research Workshop on Dynamics, Transport, and Photochemistry in the Middle Atmosphere of the Southern Hemisphere (1989 San Francisco, Calif.). Dynamics, transport, and photochemistry in the middle atmosphere of the Southern Hemisphere. Kluwer Academic Publishers, 1990.

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Linacre, Edward. Climates and weather explained: An introduction from a southern perspective. Routledge, 1996.

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Linacre, Edward. Climates and Weather Explained. Taylor & Francis Inc, 2003.

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Linacre, Edward. Climates and weather explained. Routledge, 1997.

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J, Karoly David, Vincent Dayton G, and Cooperative Research Centre for Southern Hemisphere Meteorology (Australia), eds. Meteorology of the Southern Hemisphere. American Meteorological Society, 1998.

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Second International Conference on Southern Hemisphere Meteorology. Amer Meteorological Society, 1986.

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Cooperative Research Centre for Southern Hemisphere Meteorology (Corporate Author), David J. Karoly (Editor), and Dayton G. Vincent (Editor), eds. Meteorology of the Southern Hemisphere (Meteorological Monographs (Amer Meteorological Soc)). Amer Meteorological Society, 1998.

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Tomas, Robert A. Subseasonal variability in the Southern Hemisphere as simulated by a two-level atmospheric general circulation model. 1987.

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R, Jeffries W., and United States. National Aeronautics and Space Administration. Scientific and Technical Information Branch., eds. A new NASA-MSFC mission analysis global cloud cover data base. National Aeronautics and Space Administration, Scientific and Technical Information Branch, 1985.

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Book chapters on the topic "Meteorology Southern Hemisphere"

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Reeder, Michael J., and Roger K. Smith. "Mesoscale Meteorology." In Meteorology of the Southern Hemisphere. American Meteorological Society, 1998. http://dx.doi.org/10.1007/978-1-935704-10-2_8.

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Bromwich, David H., and Thomas R. Parish. "Meteorology of the Antarctic." In Meteorology of the Southern Hemisphere. American Meteorological Society, 1998. http://dx.doi.org/10.1007/978-1-935704-10-2_7.

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Randel, William J., and Paul A. Newman. "The Stratosphere in the Southern Hemisphere." In Meteorology of the Southern Hemisphere. American Meteorological Society, 1998. http://dx.doi.org/10.1007/978-1-935704-10-2_9.

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McBride, John. "Indonesia, Papua New Guinea, and Tropical Australia: The Southern Hemisphere Monsoon." In Meteorology of the Southern Hemisphere. American Meteorological Society, 1998. http://dx.doi.org/10.1007/978-1-935704-10-2_3.

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Hurrell, James W., Harry van Loon, and Dennis J. Shea. "The Mean State of the Troposphere." In Meteorology of the Southern Hemisphere. American Meteorological Society, 1998. http://dx.doi.org/10.1007/978-1-935704-10-2_1.

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Godfrey, J. Stuart, and Stephen R. Rintoul. "The Role of the Oceans in Southern Hemisphere Climate." In Meteorology of the Southern Hemisphere. American Meteorological Society, 1998. http://dx.doi.org/10.1007/978-1-935704-10-2_10.

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Kiladis, George N., and Kingtse C. Mo. "Interannual and Intraseasonal Variability in the Southern Hemisphere." In Meteorology of the Southern Hemisphere. American Meteorological Society, 1998. http://dx.doi.org/10.1007/978-1-935704-10-2_11.

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Jones, Philip D., and Robert J. Allan. "Climatic Change and Long-Term Climatic Variability." In Meteorology of the Southern Hemisphere. American Meteorological Society, 1998. http://dx.doi.org/10.1007/978-1-935704-10-2_12.

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Meehl, Gerald A. "Climate Modeling." In Meteorology of the Southern Hemisphere. American Meteorological Society, 1998. http://dx.doi.org/10.1007/978-1-935704-10-2_13.

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Karoly, David J., Dayton G. Vincent, and Jon M. Schrage. "General Circulation." In Meteorology of the Southern Hemisphere. American Meteorological Society, 1998. http://dx.doi.org/10.1007/978-1-935704-10-2_2.

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