Résumé
Large-scale gridded population datasets are usually produced for the year of input census data using a top-down approach and projected backward and forward in time using national growth rates. Such temporal projections do not include any subnational variation in population distribution trends and ignore changes in geographical covariates such as urban land cover changes. Improved predictions of population distribution changes over time require the use of a limited number of covariates that are time-invariant or temporally explicit. Here we make use of recently released multi-temporal high-resolution global settlement layers, historical census data and latest developments in population distribution modelling methods to reconstruct population distribution changes over 30 years across the Kenyan Coast. We explore the methodological challenges associated with the production of gridded population distribution time-series in data-scarce countries and show that trade-offs have to be found between spatial and temporal resolutions when selecting the best modelling approach. Strategies used to fill data gaps may vary according to the local context and the objective of the study. This work will hopefully serve as a benchmark for future developments of population distribution time-series that are increasingly required for population-at-risk estimations and spatial modelling in various fields.
langue originale | Anglais |
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Pages (de - à) | 1017-1029 |
Nombre de pages | 13 |
journal | International Journal of Digital Earth |
Volume | 10 |
Numéro de publication | 10 |
Les DOIs | |
Etat de la publication | Publié - 3 oct. 2017 |
Financement
This work was supported by the Belgian Science Policy (BELSPO) under the Research programme for Earth Observation \u201CSTEREO III\u201D [grant number SR/00/304]. AJT is supported by a Wellcome Trust Sustaining Health Grant (106866/Z/15/Z). AJT, AS, AEG and FRS are supported by funding from the Bill and Melinda Gates Foundation [grant number OPP1106427], [grant number 1032350], [grant number OPP1134076]. AMN is supported by the Wellcome Trust, UK as an intermediate fellow [grant number 095127]; RWS is supported by the Wellcome Trust as Principal Research Fellow [grant number 103602], that also supported CWK. CWK is also grateful to the KEMRI Wellcome Trust Overseas Programme Strategic Award [grant number 084538] for additional support. This work was supported by the Belgian Science Policy (BELSPO) under the Research programme for Earth Observation ?STEREO III? [grant number SR/00/304]. AJT is supported by a Wellcome Trust Sustaining Health Grant (106866/Z/15/Z). AJT, AS, AEG and FRS are supported by funding from the Bill and Melinda Gates Foundation [grant number OPP1106427], [grant number 1032350], [grant number OPP1134076]. AMN is supported by the Wellcome Trust, UK as an intermediate fellow [grant number 095127]; RWS is supported by the Wellcome Trust as Principal Research Fellow [grant number 103602], that also supported CWK. CWK is also grateful to the KEMRI Wellcome Trust Overseas Programme Strategic Award [grant number 084538] for additional support.
Bailleurs de fonds | Numéro du bailleur de fonds |
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KEMRI Wellcome Trust | |
Wellcome Trust | 084538, 106866, 095127 |
Belgian Science Policy Office | SR/00/304 |
Bill and Melinda Gates Foundation | 1032350, OPP1106427, OPP1134076 |
Wellcome Trust Sustaining Health | 106866/Z/15/Z |
UK Research and Innovation | 103602 |