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The process of land degradation needs to be understood at various spatial and temporal scales in order to protect ecosystem services and communities directly dependent on it. This is especially true for regions in sub-Saharan Africa, where socio economic and political factors exacerbate ecological degradation. This study identifies spatially explicit land change dynamics in the Copperbelt province of Zambia in a local context using satellite vegetation index time series derived from the MODIS sensor. Three sets of parameters, namely, monthly series, annual peaking magnitude, and annual mean growing season were developed for the period 2000 to 2019. Trend was estimated by applying harmonic regression on monthly series and linear least square regression on annually aggregated series. Estimated spatial trends were further used as a basis to map endemic land change processes. Our observations were as follows: (a) 15% of the study area dominant in the east showed positive trends, (b) 3% of the study area dominant in the west showed negative trends, (c) natural regeneration in mosaic landscapes (post shifting cultivation) and land management in forest reserves were chiefly responsible for positive trends, and (d) degradation over intact miombo woodland and cultivation areas contributed to negative trends. Additionally, lower productivity over areas with semi-permanent agriculture and shift of new encroachment into woodlands from east to west of Copperbelt was observed. Pivot agriculture was not a main driver in land change. Although overall greening trends prevailed across the study site, the risk of intact woodlands being exposed to various disturbances remains high. The outcome of this study can provide insights about natural and assisted landscape restoration specifically addressing the miombo ecoregion.
Agricultural monitoring is necessary. Since the beginning of the Holocene, human agricultural
practices have been shaping the face of the earth, and today around one third of the ice-free land
mass consists of cropland and pastures. While agriculture is necessary for our survival, the
intensity has caused many negative externalities, such as enormous freshwater consumption, the
loss of forests and biodiversity, greenhouse gas emissions as well as soil erosion and degradation.
Some of these externalities can potentially be ameliorated by careful allocation of crops and
cropping practices, while at the same time the state of these crops has to be monitored in order
to assess food security. Modern day satellite-based earth observation can be an adequate tool to
quantify abundance of crop types, i.e., produce spatially explicit crop type maps. The resources to
do so, in terms of input data, reference data and classification algorithms have been constantly
improving over the past 60 years, and we live now in a time where fully operational satellites
produce freely available imagery with often less than monthly revisit times at high spatial
resolution. At the same time, classification models have been constantly evolving from
distribution based statistical algorithms, over machine learning to the now ubiquitous deep
learning.
In this environment, we used an explorative approach to advance the state of the art of crop
classification. We conducted regional case studies, focused on the study region of the Eifelkreis
Bitburg-Prüm, aiming to develop validated crop classification toolchains. Because of their unique
role in the regional agricultural system and because of their specific phenologic characteristics
we focused solely on maize fields.
In the first case study, we generated reference data for the years 2009 and 2016 in the study
region by drawing polygons based on high resolution aerial imagery, and used these in
conjunction with RapidEye imagery to produce high resolution maize maps with a random forest
classifier and a gaussian blur filter. We were able to highlight the importance of careful residual
analysis, especially in terms of autocorrelation. As an end result, we were able to prove that, in
spite of the severe limitations introduced by the restricted acquisition windows due to cloud
coverage, high quality maps could be produced for two years, and the regional development of
maize cultivation could be quantified.
In the second case study, we used these spatially explicit datasets to link the expansion of biogas
producing units with the extended maize cultivation in the area. In a next step, we overlayed the
maize maps with soil and slope rasters in order to assess spatially explicit risks of soil compaction
and erosion. Thus, we were able to highlight the potential role of remote sensing-based crop type
classification in environmental protection, by producing maps of potential soil hazards, which can
be used by local stakeholders to reallocate certain crop types to locations with less associated
risk.
In our third case study, we used Sentinel-1 data as input imagery, and official statistical records
as maize reference data, and were able to produce consistent modeling input data for four
consecutive years. Using these datasets, we could train and validate different models in spatially
iv
and temporally independent random subsets, with the goal of assessing model transferability. We
were able to show that state-of-the-art deep learning models such as UNET performed
significantly superior to conventional models like random forests, if the model was validated in a
different year or a different regional subset. We highlighted and discussed the implications on
modeling robustness, and the potential usefulness of deep learning models in building fully
operational global crop classification models.
We were able to conclude that the first major barrier for global classification models is the
reference data. Since most research in this area is still conducted with local field surveys, and only
few countries have access to official agricultural records, more global cooperation is necessary to
build harmonized and regionally stratified datasets. The second major barrier is the classification
algorithm. While a lot of progress has been made in this area, the current trend of many appearing
new types of deep learning models shows great promise, but has not yet consolidated. There is
still a lot of research necessary, to determine which models perform the best and most robust,
and are at the same time transparent and usable by non-experts such that they can be applied
and used effortlessly by local and global stakeholders.
Die Polargebiete sind geprägt von harschen Umweltbedingungen mit extrem kalten Temperaturen und Winden. Besonders während der polaren Nacht werden Temperaturen von bis zu -89.2°C}$ auf dem Antarktischen Plateau beobachtet. Infolge der starken Abkühlung beginnt das Ozeanwasser zu gefrieren und die Eisproduktion beginnt. Der Antarktische Ozean ist dabei von einer ausgeprägten zwischen- und innerjährlichen Variabilität geprägt und die Eisbedeckung variiert zwischen 2.07 * 10^6 km^2 im Sommer und 20.14 * 10^6 km^2 im Winter. Die Eisproduktion und Eisschmelze beeinflussen die atmosphärische und ozeanische Zirkulation. Dynamische Prozesse führen zur Bildung von Rissen im Eis und letztlich zum Entstehen von Eisrinnen (leads). Leads sind langgestreckte Risse die mindestens einige Meter breit und hunderte Meter bis hunderte Kilometer lang sein können. In diesen Eisrinnen ist das warme Ozeanwasser in Kontakt mit der kalten Atmosphäre, wodurch die Austauschraten fühlbarer und latenter Wärme, Feuchtigkeit und von Gasen stark erhöht sind. Eisrinnen tragen zur Eisproduktion in den Polargebieten bei und sind Habitat für zahlreiche Tiere. Eisrinnen, zentraler Bestandteil der präsentierten Studie, sind bis heute nur unzureichend im Südpolarmeer erforscht und beobachtet. Daher ist es Ziel einen Algorithmus zu entwickeln, um Eisrinnen in Fernerkundungsdaten automatisiert zu identifizieren. Dabei kommen thermal-Infrarot Satellitendaten des Moderate-Resolution Imaging Spectroradiometer (MODIS) zum Einsatz, welches auf den beiden Satelliten Aqua und Terra montiert ist und seit 2000 (Terra) bzw. 2002 (Aqua) Satellitenbilder bereitstellt. Die einzelnen Satellitenbilder beinhalten die Eisoberflächentemperatur des MOD/MYD 29 Produktes, welche in einem zweistufigen Algorithmus für den Zeitraum April bis September 2003 bis 2019 prozessiert werden.
Im ersten Schritt werden potentielle Eisrinnen anhand der lokalen positiven Temperaturanomalie identifiziert. Aufgrund von Artefakten werden weitere temperatur- und texturbasierte Parameter abgeleitet und zu täglichen Kompositen zusammengefügt. Diese werden in der zweiten Prozessierungsstufe verwendet, um Wolkenartefakte von echten Eisrinnen-Observationen zu trennen. Hier wird Fuzzy Logic genutzt und eine Antarktis-spezifische Konfiguration wird definiert. In diesem werden ausgewählte Eingabedaten aus dem ersten Prozessierungslevel genutzt, um einen finalen Proxy, den Lead Score (LS), zu berechnen. Der LS wird abschließend mittels manueller Qualitätskontrolle in eine Unsicherheit überführt. Die darüber identifizierten Artefakte können so zusätzlich zur MODIS-Wolkenmaske genutzt werden.
Auf Basis der Eisrinnenbeobachtungen wird ein klimatologischer Referenzdatensatz erstellt, der die repräsentative Eisrinnenverteilung im Antarktischen Ozean für die Wintermonate April bis September, 2003 bis 2019 zeigt. In diesem ist sichtbar, dass Eisrinnen in manchen Gegenden systematischer auftreten als in anderen. Das sind vor allem die Regionen entlang der Küstenregion, des kontinentalen Schelfabhangs und einigen Erhebungen und Kanälen in der Tiefsee. Dabei sind die erhöhten Frequenzen entlang des Schelfabhangs besonders interessant und der Einfluss von atmosphärischen und ozeanischen Einflüssen wird untersucht. Ein regionales Eis-Ozeanmodell wird genutzt, um ozeanische Einflüsse in Zusammenhang mit erhöhten Eisrinnenfrequenzen zu setzen.
In der vorliegenden Studie wird außerdem ein umfangreicher Überblick über die großskalige Variabilität von Antarktischem Meereis gegeben. Tägliche Eiskonzentrationsdaten, abgeleitet aus passiven Mikrowellendaten, werden aus dem Zeitraum 1979 bis 2018 für die Klassifikation genutzt. Der dk-means Algorithmus wird verwendet, um zehn repräsentative Eisklassen zu identifizieren. Die geographische Verteilung dieser Klassen wird als Karte dargestellt, in der der typische jährliche Eiszyklus je Klasse sichtbar ist.
Veränderungen in dem räumlichen Auftreten von Eisklassen werden identifiziert und qualitativ interpretiert. Positive Abweichungen hin zu höheren Eisklassen werden im Weddell- und dem Ross-Meer und einigen Regionen in der Ostantarktis identifiziert. Negative Abweichungen sind im Amundsen-Bellingshausen-Meer vorhanden. Der neu entwickelte (Climatological Sea Ice Anomaly Index) wird genutzt, um Klassenabweichungen in der Zeitreihe zu identifizieren. Damit werden drei Jahre (1986, 2007, 2014) für eine Fallstudie ausgewählt und in Relation zu atmosphärischen Daten aus ERA-Interim und Eisdrift-Daten untersucht. Für die beiden Jahre 1986 und 2007 können bestimmte atmosphärische Zirkulationsmuster identifiziert werden, die die entsprechende Eisklassifikation beeinflusst haben. Für das Jahr 2014 können keine besonders ausgeprägten atmosphärischen Anomalien ausgemacht werden.
Der Eisklassen-Datensatz kann in Zukunft als Ergänzung zu vorhandenen Studien und für die Validierung von Meereismodellen genutzt werden. Dabei sind vor allem Anwendungen in Bezug auf den Eisrinnen-Datensatz möglich.
Dry tropical forests undergo massive conversion and degradation processes. This also holds true for the extensive Miombo forests that cover large parts of Southern Africa. While the largest proportional area can be found in Angola, the country still struggles with food shortages, insufficient medical and educational supplies, as well as the ongoing reconstruction of infrastructure after 27 years of civil war. Especially in rural areas, the local population is therefore still heavily dependent on the consumption of natural resources, as well as subsistence agriculture. This leads, on one hand, to large areas of Miombo forests being converted for cultivation purposes, but on the other hand, to degradation processes due to the selective use of forest resources. While forest conversion in south-central rural Angola has already been quantitatively described, information about forest degradation is not yet available. This is due to the history of conflicts and the therewith connected research difficulties, as well as the remote location of this area. We apply an annual time series approach using Landsat data in south-central Angola not only to assess the current degradation status of the Miombo forests, but also to derive past developments reaching back to times of armed conflicts. We use the Disturbance Index based on tasseled cap transformation to exclude external influences like inter-annual variation of rainfall. Based on this time series, linear regression is calculated for forest areas unaffected by conversion, but also for the pre-conversion period of those areas that were used for cultivation purposes during the observation time. Metrics derived from linear regression are used to classify the study area according to their dominant modification processes.rnWe compare our results to MODIS latent integral trends and to further products to derive information on underlying drivers. Around 13% of the Miombo forests are affected by degradation processes, especially along streets, in villages, and close to existing agriculture. However, areas in presumably remote and dense forest areas are also affected to a significant extent. A comparison with MODIS derived fire ignition data shows that they are most likely affected by recurring fires and less by selective timber extraction. We confirm that areas that are used for agriculture are more heavily disturbed by selective use beforehand than those that remain unaffected by conversion. The results can be substantiated by the MODIS latent integral trends and we also show that due to extent and location, the assessment of forest conversion is most likely not sufficient to provide good estimates for the loss of natural resources.
The nonhydrostatic regional climate model CCLM was used for a long-term hindcast run (2002–2016) for the Weddell Sea region with resolutions of 15 and 5 km and two different turbulence parametrizations. CCLM was nested in ERA-Interim data and used in forecast mode (suite of consecutive 30 h long simulations with 6 h spin-up). We prescribed the sea ice concentration from satellite data and used a thermodynamic sea ice model. The performance of the model was evaluated in terms of temperature and wind using data from Antarctic stations, automatic weather stations (AWSs), an operational forecast model and reanalyses data, and lidar wind profiles. For the reference run we found a warm bias for the near-surface temperature over the Antarctic Plateau. This bias was removed in the second run by adjusting the turbulence parametrization, which results in a more realistic representation of the surface inversion over the plateau but resulted in a negative bias for some coastal regions. A comparison with measurements over the sea ice of the Weddell Sea by three AWS buoys for 1 year showed small biases for temperature around ±1 K and for wind speed of 1 m s−1. Comparisons of radio soundings showed a model bias around 0 and a RMSE of 1–2 K for temperature and 3–4 m s−1 for wind speed. The comparison of CCLM simulations at resolutions down to 1 km with wind data from Doppler lidar measurements during December 2015 and January 2016 yielded almost no bias in wind speed and a RMSE of ca. 2 m s−1. Overall CCLM shows a good representation of temperature and wind for the Weddell Sea region. Based on these encouraging results, CCLM at high resolution will be used for the investigation of the regional climate in the Antarctic and atmosphere–ice–ocean interactions processes in a forthcoming study.