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The Bafoussam area in west Cameroon is located within the Cameroon Neoproterozoic orogenic belt (north of the Congo craton) which is part of the Central African Fold Belt (CAFB).The evolution of the CAFB is related to the collision between the convergent West African craton, the São Francisco – Congo cratons and the Sahara Metacraton. The outcrop area stretches over a surface of ~1000 km2 and dominantly consists of granitoids which intruded wall-rocks of gneiss and migmatite during the Pan-African orogeny. The Bafoussam granitoid emplacement was influenced by the N 30 °E strike-slip shear zone in the prolongation of the Cameroon Volcanic Line, but also by the N 70 °E Central Cameroon Shear Zone. In the field, these two shear directions are expressed in the schistosity and foliation trajectories, fault orientation and the alignment of the volcanic cones as well. In the Bafoussam area, four types of granitoids can be distinguished, including: (i) the biotite granitoid, (ii) the deformed biotite granitoid, (iii) the mega feldspar granitoid, and (iv) the two-mica granitoid. These granitoids occur as elongated plutons hosting irregular mafic enclaves (amphibole-bearing, biotite-rich, and metagabbroic types) and are frequently cut by late pegmatites, aplite dykes and quartz veins. Petrographically, they range in composition from syenogranite (major), alkali-feldspar granite, granodiorite, monzogranite, quartz-syenite, quartzmonzonite to quartz-monzodiorite. Potassium feldspar, quartz, plagioclase and biotite are the principal phases, in cases accompanied by amphibole and accessory minerals such as apatite,zircon, monazite, titanite, allanite, ilmenite and magnetite. Sericite, epidote and chlorite are secondary minerals. In addition, the two-mica granitoid contains primary muscovite and sometimes igneous garnet. In the granitoids, potassium feldspar is orthoclase (microcline and orthoclase: Or81–97Ab19–3), and plagioclase is mainly oligoclase with some albite and andesine (An3–35Ab96–64).Biotite is Fe-rich (meroxene and lepidomelane, with some siderophyllite), having high Fe2+/(Fe2+ + Mg) ratios of 0.40–0.80. It is a re-equilibrated primary biotite and suggests calc-alkaline and peraluminous nature of the host granitoids. Amphibole is edenitic and magnesian hastingsitic hornblende, with high Mg/(Mg + Fe2+) ratios of 0.50–0.62. The evolution of the hornblende was dominated by the edenitic, tschermakitic, pargasitic and hastingsitic substitution types. Primary muscovite is iron-rich [Fe2+/(Fe2+ + Mg) = 0.52–0.82] and has experienced celadonite and paragonite substitutions. Igneous garnet is almandine–spessartine (XFe = 0.99 and XMn = 0.46–0.56). The euhedral grain shapes of garnet crystals and the absence of inclusions coupled with the high Mn and Fe2+contents (2.609–3.317 a.p.f.u and 2.646–3.277 a.p.f.u,respectively) and low Mg contents (0.012–0.038 a.p.f.u) clearly point to its plutonic origin. The Mn-depletion crystallization model is suggested for the origin of the analyzed garnet, i.e. initial crystallization of garnet inducing early decrease of Mn in the original melt. Aluminum-in-hornblende and phengite barometric estimates show that the granitoids crystallized at 4.2 ± 1.1 to 6.6 ± 1.0 kbar, corresponding to emplacement depths of 15–24 km.Zircon and apatite saturation temperature calibrations and hornblende–plagioclase thermometry yielded emplacement temperatures between 772 ± 41 and 808 ± 34 °C. Except the two-mica granitoid, the titanite–magnetite–quartz assemblage gives oxygen fugacities ranging from 10–17 to 10–13, suggesting that the granitoids were produced by an oxidized magma. Since the twomica granitoid lacks magnetite, it was originated from a magma under reducing conditions, below the quartz–fayalite–magnetite buffer. Fluid inclusions in quartz from hydrothermal veins are secondary in nature and are found in trails along healed microcracks or in clusters. Two types of fluid inclusion have been recognized, mixed aqueous–non-aqueous volatile fluid inclusions subdivided into aqueous-rich mixed and non-aqueous volatile-rich mixed fluid inclusions, and pure aqueous fluid inclusions.The non-aqueous volatile-rich mixed fluid inclusions are one-, two-, or three-phase inclusions, whereas the aqueous-rich mixed fluid inclusions are exclusively three-phase inclusions. Both have similar low to moderate salinities (1 to 10 equiv. wt. %). The total homogenization temperatures of the aqueous-rich mixed fluid inclusions are slightly lower than those of the nonaqueous volatile-rich mixed fluid inclusions, ranging from 150 to 250 °C and 170 to 300 °C,respectively. They contain nearly pure CO2, or CO2 with addition of 4.1–13.5 mole % CH4 as volatile constituents. Pure aqueous fluid inclusions are two-phase with lower total homogenization temperatures (130–150 °C) and salinities ranging from 3 to 8 equiv. wt. %. They display mixing salt system characteristics, having NaCl as the dominant salt and considerable amounts of other divalent cations. Aqueous-rich mixed fluid inclusions and pure aqueous fluid inclusions exhibit a low geothermal gradient value of 18 °C/km, whereas the non-aqueous volatiles-rich mixed fluid inclusions have a high density which correspond to high geothermal gradient of 68 °C/km. The studied granitoids are intermediate to felsic in compositions (56.9–74.6 wt. % SiO2)and have high contents of alkalis K2O (1.73–7.32 wt. %) and Na2O (1.25–5.13 wt. %) but low abundances in MnO (0.01–0.20 wt. %), MgO (0.10–3.97 wt. %), CaO (0.37–4.85 wt. %), P2O5(up to 0.90 wt. %). They display variable contents in TiO2 (0.07–0.91 wt. %), Fe2O3* (total Fe = 0.96–7.79 wt. %) and Al2O3 (12.0–17.6 wt. %) contents. The granitoids show a wide range of high-field-strength elements (HFSE) and large ion lithophile elements (LILE) contents, with felsic granitoids being enriched in HFSE and the intermediate granitoids displaying in contrast high LILE concentrations. They exhibit chemical characteristics of non-alkaline to mid-alkaline, alkali-calcic, calc-alkaline, K-rich to shoshonitic, ferriferous affinities. Chondrite-normalized rare earth element (REE) patterns are characterized by a strong enrichment in light compared to heavy REEs [(La/Sm)N = 3.23–9.65 and (Ga/Lu)N = 1.45–5.54, respectively], with small to significant negative Eu anomalies (Eu/Eu* = 0.28–1.08). Ocean ridge granites (ORG)normalized multi-elements spidergrams display typical collision-related granites pattern, with characteristic negative anomalies of Ba, Nb and Y, and positive anomalies in Rb, Th and Sm. The granitoids under study are genetically I-type granitoids (biotite granitoid, deformed biotite granitoid and mega feldspar granitoid) and one S-type granitoid (two-mica granitoid). The I-type granitoids are metaluminous (ASI: 0.70–1.00) or moderately peraluminous if highly fractionated (ASI: 1.01–1.06). The geochemistry and petrological features of these I-type granitoids argue for close genetic relationships and it is suggest that they originated from a single parent magma. The observed variability in mineralogy and major and trace element compositions in these granitoids are then the reflection of the fractional crystallization that evolved separation of plagioclase, biotite, K-feldspar and accessory minerals at the level of emplacement. The two mica S-type granitoid is exclusively peraluminous (ASI: 1.07–1.25) and classified as a peraluminous leucocratic granitoid or leucogranite. It is marked in its CIPW normative composition by the permanent presence of corundum, ranging between 0.12 and 3.03. The Bafoussam granitoids were emplaced in a syn- to post-collisional tectonic environment. The observed deformational features and the concentrations in Y, less than 40 ppm, confirm that they are related to an orogenesis. Whole-rock Rb–Sr isochrons defines an igneous crystallization ages of 540 ± 27 Ma for the biotite granitoid and 587 ± 41 Ma for the mega feldspar granitoid. These ages fit with the range of Pan-African granitoid ages (650–530 Ma) in West Cameroon and correspond to the Pan-African D2 deformation event in the Neoproterozoic Cameroon orogenic belt. The two-mica granitoid yields an older Rb–Sr isochron age of 663 ± 62 Ma which is considered to be probably a mixing age. The Nd–Sr isotopic compositions indicate that the I-type granitoids have been produced by partial melting of a tonalite–granodiorite source in the lower crust. This is supported by their initial 87Sr/86Sr(600 Ma) ratios (0.705–0.709) and by their WNd(600 Ma) values (0.2 to –6.3, mainly < 0). The two-mica granitoid was generated by partial melting of a greywacke-dominated source involving biotite-limited, biotite dehydration melting. Chemical data of the two-mica granitoid that support this hypothesis are low CaO/Na2O (0.11–0.38) and Sr/Ba (0.20–0.30), the high Rb/Sr (2.26–7.00), the high initial 87Sr/86Sr(600 Ma) ratios ranging from 0.708 to 0.720, the large range in Al2O3/TiO2 (47–204) and the negative WNd(600 Ma) values (–9.9 to –14.0). Moreover,the higher initial 87Sr/86Sr(600 Ma) ratios of the two-mica granitoid are consistent with an upper crust origin. The depleted mantle Nd model ages (TDM) of 1.3–2.3 Ga indicate that the studied granitoids originated by partial melting of Paleoproterozoic and Mesoproterozoic crust, with limited mantle-derived magma contribution. The high initial 87Sr/86Sr(600 Ma) ratios of these granitoids coupled with the wide negative WNd(600 Ma) values strongly suggest a very long residence time in the crust of their protoliths before the melting event. The petrologic signatures of the Bafoussam granitoids are similar to those described in other Pan-African belts of western Gondwanaland such as the neighbouring provinces of Nigeria and the Central African Republic, as well as in the Borborema Province of northeastern Brazil. This supports the previous hypothesis that the Central African fold Belt including Cameroon, Nigeria and the Central African Republic provinces has a continuation in Brazil.
Two phases of reef sampling were carried out. The first included regular samples taken along the coastline of Aqaba (27km long) at depths of 4-15m, and used to determine spatial distribution of pollution. The second phase included three 20cm-deep cores obtained from within the industrial zone. These cores were drilled from pre-dated communities, where the growth rate was determined earlier to be 10mm y-1, therefore the core obtained represented a period of 20 years (i.e. 1980-2000). The cores were used to reconstruct the metal pollution history at the most heavily used site along the coast (industrial zone).All samples were examined with respect to their metal content of Cd, Pb, Cu, Zn, Ni, and Cr. Almost all of them have shown records above the calculated background values. Mean values of Cd, Pb, Cu, Zn, Ni and Cr recorded along the coast were 1,25; 4,26; 9,76; 11,40; 2,29 and 10,522, µg g-1 respectively, and for core samples 1.4; 4.2; 5.7; 6.4; 2.3 and 8.21 µg g-1 respectively. Spatial distribution of metal enrichment in reef samples have shown a general and clear increasing trend towards the south. Same increasing trend was also in core samples where the six metals have shown a prominent increasing trend towards the core surface indicating an increase of coastal activities during the last twenty years. High and relatively high values were recorded at the oil port, the industrial area and main port, and thus categorized as highly impacted areas. Intermediate metal content were recorded in samples of the north beach, and thus classified as being relatively impacted, where the lowest metal concentrations were observed at the marine reserve, the least impacted site along the coast. The high enrichment of metal is attributed mainly to anthropogenic impacts. The natural inputs of the six metals studied in the Gulf of Aqaba are generally very low, due to the geographic positions and the absence of wadi discharge and as a result of low rainfall. Several potential sources of heavy metals were investigated. The industrial-related activities, port operations and phosphate dust were among the main sources currently threatening the marine ecosystem in Aqaba. Applying the Principle Components Analysis method (PCA) to all samples taken along the coastline has resulted in categorizing three different groups according to their metal enrichment, the first is composed of samples taken from the north beach and the main port with intermediate to high enrichment, the second joined the samples of the marine park and the marine reserve with low and relatively low enrichment, and the last group joined samples of the industrial zone and the oil port with high enrichment. The Principle Component Scores were also utilized to confirm the spatial distribution and relationships of the examined heavy metals along the coast. Two models (interpolated by SURFER  7.0 and ArcView 3.2a) were developed, the first was based on the PC scores of the first component, and shows clearly the positive anomalies in metal concentrations along the coast. The second model was developed by plotting the second factor scores on a landuse map of Aqaba. According to these models, it has shown that the positive anomalies are associated with three different zones; industrial area, the main port and the oil port. The results have shown that coral reefs can be used as good environmental indicator for assessments and monitoring processes, and they can provide data and information on both the spatial distribution of pollution and their history. The present work is the first to document the environmental status along the whole coast of Aqaba and the first to use coral reef as a tool/ indicator.
Die Dornbusch-Savannen Zentralnamibias unterliegen großen Veränderungen. Teilweise handelt es sich dabei um Degradationsprozesse, die zu einem Verlust an Artenvielfalt und auch ökonomischem Wert dieser überwiegend als Rinderweide genutzten Systeme führen. Die Degradation drückt sich in der Savannenlandschaft zum einen durch Verkahlung aus (Desertifikation), vor allem aber durch die massive Ausbreitung einzelner Dornbuscharten wie Acacia mellifera, die zur Umwandlung gemischter Savannenvegetation in artenarme Dominanzbestände führt (Verbuschung). Andere Veränderungen erfolgen spontan und stellen eine Reaktion der Vegetation auf aktuelle Niederschlagsereignisse dar. Diese phänologischen Änderungen sind in der Regel reversibel. Als typische Veränderungsmechanismen konnten nutzungsbedingter und natürlicher reversibler oder irreversibler Vegetationsverlust und die Wiederbesiedelung verkahlter Flächen identifiziert werden. Des Weiteren gibt es moderate Schwankungen der Vegetationsdichte, zu denen die Verbuschungsprozesse und die Buschsterbe gehören. Die Buschsterbe ist eine Pilzerkrankung, die zum flächenhaften Absterben von Akazienbüschen, vor allem von Ac. mellifera führt. Auch der Einfluss von Feuer kann eine Ursache für Veränderungen sein. Um insbesondere das Ausmaß der Degradationsprozesse in Zentralnamibia zu erfassen und zu quantifizieren, wurde in dieser Arbeit ein fernerkundliches Change-Detection-Verfahren auf der Basis von Landsat-TM und ETM-Daten entwickelt. Die methodische Basis hierfür stellten das Image-Differencing und die modifizierte selektive Hauptkomponentenanalyse (sPCA) dar. Um auch Formparameter der veränderten Flächen zur Unterscheidung von Veränderungstypen heranziehen zu können, wurden die Ergebnisse des Differencings segmentiert und das Maß der Kompaktheit(Compactness) der Segmente extrahiert. Die Klassifikation der charakteristischen Veränderungen erfolgte über Ratios und Schwellenwerte von Einzelkanälen dieser Change-Datendatensätze und der Compactness, die aus charakteristischen Veränderungssignaturen abgeleitet wurden. Diese wurden anhand von Referenzflächen ermittelt, die auf Felddaten basierten. Als Referenz zur Ableitung der Signaturen diente dabei der Veränderungsdatensatz aus dem Vergleich der Landsat- Szenen von Mai 2000 und April 2003. Diese bitemporale Change-Detection-Methode wurde für das Hauptuntersuchungsgebiet (A) in Zentralnamibia auf insgesamt 8 Kombinationen aus 7 Landsat-Szenen im Zeitraum von 1984 bis 2003 angewendet. Damit wurde die Übertragbarkeit der Methode auf verschiedene Zeitschnitte getestet. Zur Abschätzung der Übertragbarkeit auf andere Naturräume wurde die Methode zudem auch auf jeweils ein Szenenpaar in der ariden zwergstrauchdominierten Nama-Karoo in Südnamibia und in einem feuchteren Dornsavannen-Trockenwaldgebiet in der Kavango-Region Nordnamibias angewendet. Die Klassifikatoren zur Trennung der einzelnen Veränderungsklassen lieferten unterschiedlich gute Ergebnisse. Die Verkahlungs- und Wiederbesiedelungsprozesse wurden sehr zuverlässig detektiert, wobei allerdings die Unterscheidung von natürlicher und nutzungsbedingter Verkahlung anhand der Compactness-Werte den Anteil an anthropogen veränderten Flächen auffällig unterschätzte. Die Validierung anhand von Farmerauskünften bzw. vergleichenden Fotos zum Aufnahmezeitpunkt lieferte dabei in allen drei Untersuchungsgebieten ähnliche Ergebnisse. Moderate Veränderungen der Vegetationsdichte wurden in allen drei Untersuchungsgebieten überwiegend gut erkannt. Eine eindeutige Zuordnung auf Veränderungen des Busch- oder des Grasstratums war allerdings nicht immer möglich. Die Detektion von rezenten Brandflächen in Zentral- und Nordnamibia verlief zufrieden stellend. Mehrere Monate alte Brandflächen ließen sich mit dem dazu entwickelten Klassifikator jedoch nicht von anderen phänologisch und nutzungsbedingten Veränderungen trennen. Zur Analyse der Signifikanz der Change-Detektion-Ergebnisse wurden verschiedene Niederschlagsdaten und NDVI-Zeitreihen für den jeweiligen Beobachtungszeitraum hinzugezogen. Es zeigte sich, dass die Change-Detection-Ergebnisse stark mit den Niederschlagssummen korrelierten, die in der jeweiligen Regenzeit bis zum Aufnahmezeitpunkt der einzelnen Landsat-Szenen gefallen waren. War die Regenzeit zum ersten Vergleichszeitpunkt ergiebiger als zum zweiten, wurde überwiegend Vegetationsrückgang detektiert. War die zweite Regenzeit hingegen feuchter als die erste, wurde überwiegend Vegetationszunahme detektiert. Die Größe der Niederschlagsdifferenz zwischen beiden Zeitpunkten spiegelte sich zudem im Flächenanteil der einzelnen Veränderungsklassen wider. Durch diesen starken phänologischen, d.h. niederschlagsbedingten Veränderungsanteil wurden „echte“ Veränderungen z.T. verschleiert oder verstärkt. Dieses Ergebnis korrespondiert mit den Ergebnissen vieler anderer Change-Detection-Arbeiten im semiariden Raum. Als relevante Veränderungen wurden daher nur solche bewertet, die dem allgemeinen phänologischen Trend im Vergleichszeitraum entgegenstanden. So konnten z.B. Flächen, auf denen Vegetationszuwachs detektiert wurde, obwohl die Regenzeit zum zweiten Aufnahmezeitpunkt schwächer war als die erste, als tatsächlich verbuscht gelten. Unter Berücksichtigung dieser niederschlagsbedingten Einflüsse wurden im Untersuchungsgebiet in Zentralnamibia die Flächenanteile bestimmt, für die Degradation detektiert wurde. Demnach hat im Vergleich der Szenen von 1984 und 2003 auf etwa 681 km², entsprechend 2,8 % der Gesamtfläche des Untersuchungsgebietes, eine niederschlagsunabhängige Verdichtung der Vegetation, d.h. eine Verbuschung stattgefunden. Die Lage der betroffenen Gebiete korrespondiert mit der in der Literatur genannten Region (vgl. BESTER 1998/99). Des Weiteren wurde im Untersuchungszeitraum von 1984 bis 2003 auf ca. 0,53 km², entsprechend 0,002 % der Gesamtfläche des Untersuchungsgebietes irreversible Verkahlung, d.h. Desertifikation detektiert. Damit stellt in Zentralnamibia die Veränderung durch Verbuschung die flächenmäßig größte Bedrohung für Artenvielfalt und landwirtschaftliche Tragkraft der Savannen dar. Aufgrund der starken phänologischen Einflüsse konnten von der Buschsterbe betroffene Regionen im Untersuchungsgebiet nicht sicher erkannt und quantifiziert werden. Kleinräumig konnten im Untersuchungsgebiet in Zentralnamibia Farmen identifiziert werden, die in einem oder mehreren Ergebnisbildern durch besondere Veränderungsmuster auffielen. Zumeist handelte es sich um Degradationserscheinungen wie Verbuschung und Verkahlung, für die bei der Besichtigung während der Feldkampagne im Jahr 2004 oft ein Zusammenhang mit ungünstigen Landnutzungspraktiken, d.h. vor allem Überweidung hergestellt werden konnte. Des Weiteren wurden starke Veränderungen durch Entbuschungsmaßnahmen, kurzzeitige Weideeinflüsse und auch einzelne wiederhergestellte Bestände detektiert. Nutzungsbedingte Degradationserscheinungen treten im Untersuchungsgebiet in Zentralnamibia insgesamt nur kleinräumig auf einzelnen Farmen auf. Für das Untersuchungsgebiet in Südnamibia lagen zwei Landsat-Szenen für den kurzen Vergleichszeitraum von 2001 zu 2002 vor. Anhand dieser konnten unter Zuhilfenahme von Niederschlagsdaten stark degradierte Flächen identifiziert werden. Während auf den intakten Flächen aufgrund der besseren Regenzeit zum zweiten Aufnahmezeitpunkt wie erwartet Vegetationszuwachs detektiert wurde, führten ebendiese reichlichen Niederschläge im degradierten Gebiet zu einer großflächigen Erosion der Vegetationsdecke. Dies ist vermutlich auf die größere Geschwindigkeit des oberflächlich abfließenden Regenwassers in der spärlichen Vegetationsdecke der degradierten Fläche zurück zu führen. In den übrigen Gebieten reduzierte hingegen die dichtere Vegetation den Oberflächenabfluss, wodurch mehr Wasser versickerte und verstärktem Pflanzenwachstum zur Verfügung stand. Im Untersuchungsgebiet in Nordnamibia wurden zwei Landsat-Szenen von April 1991 und April 2000 verglichen. Die gravierendste Veränderung in diesem Zeitraum war nutzungsbedingte Verkahlung, die auf rund 4,4 % der Gesamtfläche, entsprechend 81 km² detektiert wurde. Ursache ist hier die Umwandlung von Dornbuschsavanne in Acker- oder Siedlungsraum. Demgegenüber wurde aber nur für 1,17 % der Gesamtfläche, entsprechend 21,76 km², Wiederbesiedelung detektiert. Dies sind zumeist Agrarflächen, die (kurzzeitig) aus der Nutzung genommen wurden. Das Ergebnis dokumentiert den zunehmenden Siedlungsdruck in der Kavango-Region. Die seit den 1970er Jahren verbesserte Infrastruktur ermöglicht hier immer mehr Menschen die Landnahme, Viehhaltung und Siedlung. Die Ergebnisse dieser Arbeit zeigen, dass mit der hier entwickelten Change-Detection-Methode unter Berücksichtigung der Niederschlagshistorie in den semiariden und ariden Testgebieten signifikante Veränderungen der Vegetation in verschiedenen Landschaftsräumen detektiert werden können. Weitere Anwendungen der Methodik auf andere Testgebiete im südlichen und westlichen Afrika am Rande dieser Arbeit zeigten ebenfalls gute Ergebnisse, die allerdings bislang aus Mangel an Referenzdaten nicht validiert werden konnten. Zur zukünftigen Operationalisierung der Methodik sollte vor allem eine verbesserte Trennbarkeit von nutzungsbedingten und natürlichen Verkahlungsprozessen angestrebt werden. Des Weiteren wird eine Anpassung der Klassifikatoren auf andere Sensoren wie z.B. ASTER angedacht, um auch nach dem Ausfall von Landsat 7 im Jahr 2003 aktuelle Daten vergleichen zu können. Um den phänologischen Einfluss von unterschiedlichen Niederschlagshistorien im Vorfeld der Eingangsdaten zu minimieren, wäre zudem die Implementierung eines Kalibrierungsfaktors denkbar, der auf Niederschlags- oder auch MODIS-NDVI-Daten der entsprechenden Zeit- und Untersuchungsräume basiert. Das Ergebnis wäre eine sichere Methode zur Detektion von regionalen Veränderungen im semiariden Raum. Die Identifizierung dieser Veränderungen, speziell von Degradationserscheinungen stellt die Basis dar, dort gezielt nach den Ursachen zu suchen und Handlungsempfehlungen zu entwickeln, um einer fortschreitenden Zerstörung von Lebensraum, Artenvielfalt und ökonomischem Potenzial der betroffenen Flächen entgegen zu wirken.
New urbanism in US-amerikanischen Stadtregionen : ein effektives Planungskonzept gegen Urban Sprawl?
(2005)
The research project examines Urban Sprawl in the United States and evaluates the alternative planning concept New Urbanism on a regional and local scale. The combination of qualitative and quantitative data sources explores the effectiveness of regional planning agencies on a macro level, as well as the success of mixed-use neighborhoods on a micro level. The results are based on three cities of the United States (Atlanta, Denver, and Portland), 80 qualitative interviews with urban experts, and over 160 questionnaires with residents of three New Urbanism neighborhoods (Riverside, Atlanta; Prospect, Denver; Orenco Station, Portland). The thesis shows and explains the challenges facing contemporary metropolitan areas and neighborhood development projects, the role and impact that public administrations and other policy makers have in this field, as well as how economic decisions on a local, regional, and global level can shape, change and develop urban landscapes. A central argument is that only superordinated regional planning authorities will be able to contain urban sprawl and to face its related complex socio-economic, administrative, and environmental problems. Also, New Urbanism neighborhoods can only be successful on a micro level when they are embedded in an all-embracing and socially well-balanced regional plan. This integrative two-way perspective from a macro and a micro level can enable us to understand urban structures, processes and problems in a more comprehensive way.
This study explores and examines the geomorphology of a large endorheic basin, approximately twice the size of Luxemburg, situated in the Etosha National Park, Namibia. The main focus is directed on how and when this depression, known as Etosha Pan, came into being. Geomorphological investigation was complemented and guided primarily by the application and interpretation of satellite-derived information. Etosha Pan has attracted scientific investigations for nearly a century. Unfortunately, their efforts resulted into two diverging and mutually exclusive views with respect to its development. The first and oldest view dates back to the 1920s. It hypothesized Etosha Pan as a desiccated palaeolake which was abandoned following the river capture of its major fluvial system, the Kunene River. The river capture was assumed to have taken place in the Pliocene/Early Pleistocene. In spite of the absence of fluvial input that the Kunene contributed, the original lake was thought to have persisted until some 35 ka ago, long after the Kunene severed its ties with the basin. The current size of the basin and its playa status was interpreted to have resulted from deteriorating climatic conditions. The opposing view emerged in the 1980s and gained prominence in the 1990s. This view assumed that there were an innumerable number of small pans on the then surface of what later to become Etosha Pan. Since the turn of the Pliocene to Early Pleistocene, these individual pans started to experience a combined effect of fluvial erosion during the rainy season and wind deflation during the dry period. The climatic regime during that entire period was postulated to be semi-arid as today. This climatic status was used to rule out any existence of a perennial lake within the boundary of Etosha since the Quaternary. Ultimately, these denudational processes, taking place in a seasonal rhythm, caused the individual pans to deepen and widen laterally into each other and formed a super-pan that we call Etosha today. Thus the Kunene River had no role to play in the development of the Etosha Pan according to this model. However, proponents of this model acknowledged that the Kunene once fed into the Owambo Basin and assigned the end of the Tertiary to the terminal phase of that inflow. Findings of this study included field evidence endorsing the postulation that the Kunene River had once flowed into the Owambo Basin. Its infilled valley, bounding with the contemporary valley of the Kunene near Calueque, was identified and points towards the Etosha Pan. It is deliberated that a large lake, called Lake Kunene, existed in the basin during the time. Following the deflection of the Kunene River to the coast under the influence of river incision and neo-tectonic during the Late Pliocene, new dynamics were introduced over the Owambo Basin surface. After the basin was deprived of its major water and sediment budget that the Kunene River contributed, it was left with only smaller rivers, most notably the Cuvelai System, as the only remaining supplier. This resulted in the Cuvelai System concentrating and limiting its collective load deposition to a lobe of Lake Kunene basin floor. The accident of that lobe is unclear, but it is likely that it constituted the deepest part of the basin at the time or it was influenced by neo-tectonic that helped divert the Kunene River or both. Against the backdrop of fluvial action that was initiating the new lake, most parts of the rest of the basin, then denied of lacustrine activity, were intermittently riddled with a veneer of sediment, especially during phases of intensified aeolian activity. In the mean time, the area that was regularly receiving fluvial input started to shape up as a distinct lake with the depositions of sediments around the water-body, primarily via littoral action, serving as embankment. Gradually, a shoreline is formed and assisted in fixing and delineating the spatial extent of the new and much smaller lake, called Lake Etosha. That Lake Etosha is the predecessor of the modern day Etosha Pan. Indicators for a perennial lake found in this study at Etosha include fossil fragments of Clariidae species comparable to modern species measuring some 90 cm, and those of sitatunga dated to approximately 5 ka. None of these creatures exist today at Etosha because of their ecological requirements, which among others, include permanent water. The sitatunga, in addition, is known as the only truly amphibious antelope in the world. Since its inception, the new lake underwent a number of geomorphological modifications. A prominent character amongst these modifications is the orientation of the lake, which has its long-axis oriented in the ENE-WSW direction. It resulted from wave action affected by the prevailing dominant northeasterly wind, which is believed to have been in force since the Middle Pleistocene. Lake Etosha has also witnessed phases of waning and waxing under the influence of the prevailing climatic regime. Over the last 150 ka, the available data intercepted about seven phases of high lake levels. These data are generally in agreement with regional palaeoclimatic data, particularly when compared with those obtained from neighbouring Makgadikgadi Pans in Botswana. The last recorded episode of the wet phase at Etosha was some 2,400 years before the present.