868 resultados para spatial resolution


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Up to now, high-resolution mapping of surface water extent from satellites has only been available for a few regions, over limited time periods. The extension of the temporal and spatial coverage was difficult, due to the limitation of the remote sensing technique e.g., the interaction of the radiation with vegetation or cloud for visible observations or the temporal sampling with the synthetic aperture radar (SAR)]. The advantages and the limitations of the various satellite techniques are reviewed. The need to have a global and consistent estimate of the water surfaces over long time periods triggered the development of a multi-satellite methodology to obtain consistent surface water all over the globe, regardless of the environments. The Global Inundation Extent from Multi-satellites (GIEMS) combines the complementary strengths of satellite observations from the visible to the microwave, to produce a low-resolution monthly dataset () of surface water extent and dynamics. Downscaling algorithms are now developed and applied to GIEMS, using high-spatial-resolution information from visible, near-infrared, and synthetic aperture radar (SAR) satellite images, or from digital elevation models. Preliminary products are available down to 500-m spatial resolution. This work bridges the gaps and prepares for the future NASA/CNES Surface Water Ocean Topography (SWOT) mission to be launched in 2020. SWOT will delineate surface water extent estimates and their water storage with an unprecedented spatial resolution and accuracy, thanks to a SAR in an interferometry mode. When available, the SWOT data will be adopted to downscale GIEMS, to produce a long time series of water surfaces at global scale, consistent with the SWOT observations.

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As part of a multibeam and side scan sonar (SSS) benthic survey of the Marine Conservation District (MCD) south of St. Thomas, USVI and the seasonal closed areas in St. Croix—Lang Bank (LB) for red hind (Epinephelus guttatus) and the Mutton Snapper (MS) (Lutjanus analis) area—we extracted signals from water column targets that represent individual and aggregated fish over various benthic habitats encountered in the SSS imagery. The survey covered a total of 18 km2 throughout the federal jurisdiction fishery management areas. The complementary set of 28 habitat classification digital maps covered a total of 5,462.3 ha; MCDW (West) accounted for 45% of that area, and MCDE (East) 26%, LB 17%, and MS the remaining 13%. With the exception of MS, corals and gorgonians on consolidated habitats were significantly more abundant than submerged aquatic vegetation (SAV) on unconsolidated sediments or unconsolidated sediments. Continuous coral habitat was the most abundant consolidated habitat for both MCDW and MCDE (41% and 43% respectively). Consolidated habitats in LB and MS predominantly consisted of gorgonian plain habitat with 95% and 83% respectively. Coral limestone habitat was more abundant than coral patch habitat; it was found near the shelf break in MS, MCDW, and MCDE. Coral limestone and coral patch habitats only covered LB minimally. The high spatial resolution (0.15 m) of the acquired imagery allowed the detection of differing fish aggregation (FA) types. The largest FA densities were located at MCDW and MCDE over coral communities that occupy up to 70% of the bottom cover. Counts of unidentified swimming objects (USOs), likely representing individual fish, were similar among locations and occurred primarily over sand and shelf edge areas. Fish aggregation school sizes were significantly smaller at MS than the other three locations (MCDW, MCDE, and LB). This study shows the advantages of utilizing SSS in determining fish distributions and density.

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Following the miniaturization of photonic devices and the increase in data rates, the issues of self heating and heat removal in active nanophotonic devices should be considered and studied in more details. In this paper we use the approach of Scanning Thermal Microscopy (SThM) to obtain an image of the temperature field of a silicon micro ring resonator with sub-micron spatial resolution. The temperature rise in the device is a result of self heating which is caused by free carrier absorption in the doped silicon. The temperature is measured locally and directly using a temperature sensitive AFM probe. We show that this local temperature measurement is feasible in the photonic device despite the perturbation that is introduced by the probe. Using the above method we observed a significant self heating of about 10 degrees within the device.

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A full-ring PET insert device should be able to enhance the image resolution of existing small-animal PET scanners. Methods: The device consists of 18 high-resolution PET detectors in a cylindric enclosure. Each detector contains a cerium-doped lutetium oxyorthosilicate array (12 x 12 crystals, 0.72 x 1.51 x 3.75 mm each) coupled to a position-sensitive photomultiplier tube via an optical fiber bundle made of 8 x 16 square multiclad fibers. Signals from the insert detectors are connected to the scanner through the electronics of the disabled first ring of detectors, which permits coincidence detection between the 2 systems. Energy resolution of a detector was measured using a Ge-68 point source, and a calibrated 68Ge point source stepped across the axial field of view (FOV) provided the sensitivity profile of the system. A Na-22 point source imaged at different offsets from the center characterized the in-plane resolution of the insert system. Imaging was then performed with a Derenzo phantom filled with 19.5 MBq of F-18-fluoride and imaged for 2 h; a 24.3-g mouse injected with 129.5 MBq of F-18-fluoride and imaged in 5 bed positions at 3.5 h after injection; and a 22.8-g mouse injected with 14.3 MBq of F-18-FDG and imaged for 2 h with electrocardiogram gating. Results: The energy resolution of a typical detector module at 511 keV is 19.0% +/- 3.1 %. The peak sensitivity of the system is approximately 2.67%. The image resolution of the system ranges from 1.0- to 1.8-mm full width at half maximum near the center of the FOV, depending on the type of coincidence events used for image reconstruction. Derenzo phantom and mouse bone images showed significant improvement in transaxial image resolution using the insert device. Mouse heart images demonstrated the gated imaging capability of the device. Conclusion: We have built a prototype full-ring insert device for a small-animal PET scanner to provide higher-resolution PET images within a reduced imaging FOV. Development of additional correction techniques are needed to achieve quantitative imaging with such an insert.

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Land use and land cover change as the core of coupled human-environment systems has become a potential field of land change science (LCS) in the study of global environmental change. Based on remotely sensed data of land use change with a spatial resolution of 1 km x 1 km on national scale among every 5 years, this paper designed a new dynamic regionalization according to the comprehensive characteristics of land use change including regional differentiation, physical, economic, and macro-policy factors as well. Spatial pattern of land use change and its driving forces were investigated in China in the early 21st century. To sum up, land use change pattern of this period was characterized by rapid changes in the whole country. Over the agricultural zones, e.g., Huang-Huai-Hai Plain, the southeast coastal areas and Sichuan Basin, a great proportion of fine arable land were engrossed owing to considerable expansion of the built-up and residential areas, resulting in decrease of paddy land area in southern China. The development of oasis agriculture in Northwest China and the reclamation in Northeast China led to a slight increase in arable land area in northern China. Due to the "Grain for Green" policy, forest area was significantly increased in the middle and western developing regions, where the vegetation coverage was substantially enlarged, likewise. This paper argued the main driving forces as the implementation of the strategy on land use and regional development, such as policies of "Western Development", "Revitalization of Northeast", coupled with rapidly economic development during this period.

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The relationships between ecological diversity and ecosystem functions such as stability and productivity have long been debated and have no final conclusion until now. It is ignored that the debate should be firstly based on the same diversity index, which should be theoretically complete, and on same observation scale. For the issue on the scale of ecotope observation, ecosystems should be distinguished according to intensity of human disturbance. For the issue on the scale of species observation, either number diversity or biomass diversity should be identified. This paper takes grassland ecosystems located within the Bayin Xile grassland of Xilin Gol League of Inner Mongolia Autonomous Region as an example to analyze effects of different diversity indices and spatial scales on the conclusions of ecological diversity and its relationships with ecosystem functions. The analysis results both on the scale of ecotope observation and on the scale of species observation show that different diversity indices might give different conclusions and spatial resolution has a great effect on the relative conclusions. (c) 2005 Elsevier B.V. All rights reserved.

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Quantification of areal evapotranspiration from remote sensing data requires the determination of surface energy balance components with support of field observations. Much attention should be given to spatial resolution sensitivity to the physics of surface heterogeneity. Using the Priestley-Taylor model, we generated evapotranspiration maps at several spatial resolutions for a heterogeneous area at Haibei, and validated the evapotranspiration maps with the flux tower data. The results suggested that the mean values for all evapotranspiration maps were quite similar but their standard deviations decreased with the coarsening of spatial resolution. When the resolution transcended about 480 m, the standard deviations drastically decreased, indicating a loss of spatial structure information of the original resolution evapotranspiration map. The absolute values of relative errors of the points for evapotranspiration maps showed a fluctuant trend as spatial resolution of input parameter data layers coarsening, and the absolute value of relative errors reached minimum when pixel size of map matched up to measuring scale of eddy covariance system. Finally, based on the analyses of the semi-variogram of the original resolution evapotranspiration map and the shapes of spatial autocorrelation indices of Moran and Geary for evapotranspiration maps at different resolutions, an appropriate resolution was suggested for the areal evapotranspiration simulation in this study area.

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We examined the taxonomic resolution of zooplankton data required to identify ocean basin scale biogeographic zonation in the Southern Ocean. A 2,154 km transect was completed south of Australia. Sea surface temperature (SST) measured at 1 min intervals showed that seven physical zones were sampled. Zooplankton were collected at a spatial resolution of similar to 9.2 km with a continuous plankton recorder, identified to the highest possible taxonomic resolution and enumerated. Zooplankton assemblage similarity between samples was calculated using the Bray-Curtis index for the taxonomic levels of species, genus, family, order and class after first log(10)(x + 1) (LA) and then presence/absence (PA) transformation of abundance data. Although within and between zone sample similarity increased with decreasing taxonomic resolution, for both data transformations, cluster analysis demonstrated that the biogeographic separation of zones remained at all taxonomic levels when using LA data. ANOSIM confirmed this, detecting significant differences in zooplankton assemblage structure between all seven a priori determined physical zones for all taxonomic levels when using the LA data. In the case of the PA data for the complete data set, and both LA and PA data for a crustacean only data set, no significant differences were detected between zooplankton assemblages in the Polar frontal zone (PFZ) and inter-PFZ at any taxonomic level. Loss of information at resolutions below the species level, particularly in the PA data, prevented the separation of some zones. However, the majority of physical zones were biogeographically distinct from species level to class using both LA and PA transformations. Significant relationships between SST and zooplankton community structure, summarised as NMDS scores, at all taxonomic levels, for both LA and PA transformations, and complete and crustacean only data sets, highlighted the biogeographic relevance of low resolution taxonomic data. The retention of biogeographic information in low taxonomic resolution data shows that data sets collected with different taxonomic resolutions may be meaningfully merged for the post hoc generation of Southern Ocean time series.

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Globally, priority areas for biodiversity are relatively well known, yet few detailed plans exist to direct conservation action within them, despite urgent need. Madagascar, like other globally recognized biodiversity hot spots, has complex spatial patterns of endemism that differ among taxonomic groups, creating challenges for the selection of within-country priorities. We show, in an analysis of wide taxonomic and geographic breadth and high spatial resolution, that multitaxonomic rather than single-taxon approaches are critical for identifying areas likely to promote the persistence of most species. Our conservation prioritization, facilitated by newly available techniques, identifies optimal expansion sites for the Madagascar government's current goal of tripling the land area under protection. Our findings further suggest that high-resolution multitaxonomic approaches to prioritization may be necessary to ensure protection for biodiversity in other global hot spots.

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A novel type of microwave probes based on the loaded aperture geometry has been proposed and experimentally evaluated for dielectrics characterisation and high-resolution near-field imaging. Experimental results demonstrate the possibility of very accurate microwave spectroscopic characterisation of thin lossy dielectric samples and biological materials containing water. High-resolution images of the subwavelength lossy dielectric strips and wet and dry leaves have been obtained with amplitude contrast around 10-20 dB and spatial resolution better than one-tenth of a wavelength in the near-field zone. A microwave imaging scenario for the early-stage skin cancer identification based on the artificial dielectric model has also been explored. This model study shows that the typical resolution of an artificial malignant tumour with a characteristic size of one-tenth of a wavelength can be discriminated with at least 6 dB amplitude and 50° phase contrast from the artificial healthy skin and with more than 3 dB contrast from a benign lesion of the same size. It has also been demonstrated that the proposed device can efficiently deliver microwave energy to very small, subwavelength, focal areas which is highly sought in the microwave hyperthermia applications.

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The development of a compact gamma camera with high spatial resolution is of great interest in Nuclear Medicine as a means to increase the sensitivity of scintigraphy exams and thus allow the early detection of small tumours. Following the introduction of the wavelength-shifting fibre (WSF) gamma camera by Soares et al. and evolution of photodiodes into highly sensitive silicon photomultipliers (SiPMs), this thesis explores the development of a WSF gamma camera using SiPMs to obtain the position information of scintillation events in a continuous CsI(Na) crystal. The design is highly flexible, allowing the coverage of different areas and the development of compact cameras, with very small dead areas at the edges. After initial studies which confirmed the feasibility of applying SiPMs, a prototype with 5 5 cm2 was assembled and tested at room temperature, in an active field-of-view of 10 10 mm2. Calibration and characterisation of intrinsic properties of this prototype were done using 57Co, while extrinsic measurements were performed using a high-resolution parallel-hole collimator and 99mTc. In addition, a small mouse injected with a radiopharmaceutical was imaged with the developed prototype. Results confirm the great potential of SiPMs when applied in a WSF gamma camera, achieving spatial resolution performance superior to the traditional Anger camera. Furthermore, performance can be improved by an optimisation of experimental conditions, in order to minimise and control the undesirable effects of thermal noise and non-uniformity of response of multiple SiPMs. The development and partial characterisation of a larger SiPM WSF gamma camera with 10 10 cm2 for clinical application are also presented.

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Contexte & Objectifs : La manométrie perfusée conventionnelle et la manométrie haute résolution (HRM) ont permis le développement d’une variété de paramètres pour mieux comprendre la motilité de l'œsophage et quantifier les caractéristiques de la jonction œsophago-gastrique (JOG). Cependant, l'anatomie de la JOG est complexe et les enregistrements de manométrie détectent à la fois la pression des structures intrinsèques et des structures extrinsèques à l'œsophage. Ces différents composants ont des rôles distincts au niveau de la JOG. Les pressions dominantes ainsi détectées au niveau de la JOG sont attribuables au sphincter œsophagien inférieur (SOI) et aux piliers du diaphragme (CD), mais aucune des technologies manométriques actuelles n’est capable de distinguer ces différents composants de la JOG. Lorsqu’on analyse les caractéristiques de la JOG au repos, celle ci se comporte avant tout comme une barrière antireflux. Les paramètres manométriques les plus couramment utilisés dans ce but sont la longueur de la JOG et le point d’inversion respiratoire (RIP), défini comme le lieu où le pic de la courbe de pression inspiratoire change de positif (dans l’abdomen) à négatif (dans le thorax), lors de la classique manœuvre de « pull-through ». Cependant, l'importance de ces mesures reste marginale comme en témoigne une récente prise de position de l’American Gastroenterology Association Institute (AGAI) (1) qui concluait que « le rôle actuel de la manométrie dans le reflux gastro-œsophagien (RGO) est d'exclure les troubles moteurs comme cause des symptômes présentés par la patient ». Lors de la déglutition, la mesure objective de la relaxation de la JOG est la pression de relaxation intégrée (IRP), qui permet de faire la distinction entre une relaxation normale et une relaxation anormale de la JOG. Toutefois, puisque la HRM utilise des pressions moyennes à chaque niveau de capteurs, certaines études de manométrie laissent suggérer qu’il existe une zone de haute pression persistante au niveau de la JOG même si un transit est mis en évidence en vidéofluoroscopie. Récemment, la manométrie haute résolution « 3D » (3D-HRM) a été développée (Given Imaging, Duluth, GA) avec le potentiel de simplifier l'évaluation de la morphologie et de la physiologie de la JOG. Le segment « 3D » de ce cathéter de HRM permet l'enregistrement de la pression à la fois de façon axiale et radiale tout en maintenant une position fixe de la sonde, et évitant ainsi la manœuvre de « pull-through ». Par conséquent, la 3D-HRM devrait permettre la mesure de paramètres importants de la JOG tels que sa longueur et le RIP. Les données extraites de l'enregistrement fait par 3D-HRM permettraient également de différencier les signaux de pression attribuables au SOI des éléments qui l’entourent. De plus, l’enregistrement des pressions de façon radiaire permettrait d’enregistrer la pression minimale de chaque niveau de capteurs et devrait corriger cette zone de haute pression parfois persistante lors la déglutition. Ainsi, les objectifs de ce travail étaient: 1) de décrire la morphologie de la JOG au repos en tant que barrière antireflux, en comparant les mesures effectuées avec la 3D-HRM en temps réel, par rapport à celle simulées lors d’une manœuvre de « pull-through » et de déterminer quelles sont les signatures des pressions attribuables au SOI et au diaphragme; 2) d’évaluer la relaxation de la JOG pendant la déglutition en testant l'hypothèse selon laquelle la 3D-HRM permet le développement d’un nouveau paradigme (appelé « 3D eSleeve ») pour le calcul de l’IRP, fondé sur l’utilisation de la pression radiale minimale à chaque niveau de capteur de pression le long de la JOG. Ce nouveau paradigme sera comparé à une étude de transit en vidéofluoroscopie pour évaluer le gradient de pression à travers la JOG. Méthodes : Nous avons utilisé un cathéter 3D-HRM, qui incorpore un segment dit « 3D » de 9 cm au sein d’un cathéter HRM par ailleurs standard. Le segment 3D est composé de 12 niveaux (espacés de 7.5mm) de 8 capteurs de pression disposés radialement, soit un total de 96 capteurs. Neuf volontaires ont été étudiés au repos, où des enregistrements ont été effectués en temps réel et pendant une manœuvre de « pull-through » du segment 3D (mobilisation successive du cathéter de 5 mm, pour que le segment 3D se déplace le long de la JOG). Les mesures de la longueur du SOI et la détermination du RIP ont été réalisées. La longueur de la JOG a été mesurée lors du « pull-through » en utilisant 4 capteurs du segment 3D dispersés radialement et les marges de la JOG ont été définies par une augmentation de la pression de 2 mmHg par rapport à la pression gastrique ou de l’œsophage. Pour le calcul en temps réel, les limites distale et proximale de la JOG ont été définies par une augmentation de pression circonférentielle de 2 mmHg par rapport à la pression de l'estomac. Le RIP a été déterminée, A) dans le mode de tracé conventionnel avec la méthode du « pull-through » [le RIP est la valeur moyenne de 4 mesures] et B) en position fixe, dans le mode de représentation topographique de la pression de l’œsophage, en utilisant l’outil logiciel pour déterminer le point d'inversion de la pression (PIP). Pour l'étude de la relaxation de la JOG lors de la déglutition, 25 volontaires ont été étudiés et ont subi 3 études de manométrie (10 déglutitions de 5ml d’eau) en position couchée avec un cathéter HRM standard et un cathéter 3D-HRM. Avec la 3D-HRM, l’analyse a été effectuée une fois avec le segment 3D et une fois avec une partie non 3D du cathéter (capteurs standard de HRM). Ainsi, pour chaque individu, l'IRP a été calculée de quatre façons: 1) avec la méthode conventionnelle en utilisant le cathéter HRM standard, 2) avec la méthode conventionnelle en utilisant le segment standard du cathéter 3D-HRM, 3) avec la méthode conventionnelle en utilisant le segment « 3D » du cathéter 3D-HRM, et 4) avec le nouveau paradigme (3D eSleeve) qui recueille la pression minimale de chaque niveau de capteurs (segment 3D). Quatorze autres sujets ont subi une vidéofluoroscopie simultanée à l’étude de manométrie avec le cathéter 3D-HRM. Les données de pression ont été exportés vers MATLAB ™ et quatre pressions ont été mesurées simultanément : 1) la pression du corps de l’œsophage, 2cm au-dessus de la JOG, 2) la pression intragastrique, 3) la pression radiale moyenne de la JOG (pression du eSleeve) et 4) la pression de la JOG en utilisant la pression minimale de chaque niveau de capteurs (pression du 3D eSleeve). Ces données ont permis de déterminer le temps permissif d'écoulement du bolus (FPT), caractérisé par la période au cours de laquelle un gradient de pression existe à travers la JOG (pression œsophagienne > pression de relaxation de la JOG > pression gastrique). La présence ou l'absence du bolus en vidéofluoroscopie et le FPT ont été codés avec des valeurs dichotomiques pour chaque période de 0,1 s. Nous avons alors calculé la sensibilité et la spécificité correspondant à la valeur du FPT pour la pression du eSleeve et pour la pression du 3D eSleeve, avec la vidéofluoroscopie pour référence. Résultats : Les enregistrements avec la 3D-HRM laissent suggérer que la longueur du sphincter évaluée avec la méthode du « pull-through » était grandement exagéré en incorporant dans la mesure du SOI les signaux de pression extrinsèques à l’œsophage, asymétriques et attribuables aux piliers du diaphragme et aux structures vasculaires. L’enregistrement en temps réel a permis de constater que les principaux constituants de la pression de la JOG au repos étaient attribuables au diaphragme. L’IRP calculé avec le nouveau paradigme 3D eSleeve était significativement inférieur à tous les autres calculs d'IRP avec une limite supérieure de la normale de 12 mmHg contre 17 mmHg pour l’IRP calculé avec la HRM standard. La sensibilité (0,78) et la spécificité (0,88) du 3D eSleeve étaient meilleurs que le eSleeve standard (0,55 et 0,85 respectivement) pour prédire le FPT par rapport à la vidéofluoroscopie. Discussion et conclusion : Nos observations suggèrent que la 3D-HRM permet l'enregistrement en temps réel des attributs de la JOG, facilitant l'analyse des constituants responsables de sa fonction au repos en tant que barrière antireflux. La résolution spatiale axiale et radiale du segment « 3D » pourrait permettre de poursuivre cette étude pour quantifier les signaux de pression de la JOG attribuable au SOI et aux structures extrinsèques (diaphragme et artéfacts vasculaires). Ces attributs du cathéter 3D-HRM suggèrent qu'il s'agit d'un nouvel outil prometteur pour l'étude de la physiopathologie du RGO. Au cours de la déglutition, nous avons évalué la faisabilité d’améliorer la mesure de l’IRP en utilisant ce nouveau cathéter de manométrie 3D avec un nouveau paradigme (3D eSleeve) basé sur l’utilisation de la pression radiale minimale à chaque niveau de capteurs de pression. Nos résultats suggèrent que cette approche est plus précise que celle de la manométrie haute résolution standard. La 3D-HRM devrait certainement améliorer la précision des mesures de relaxation de la JOG et cela devrait avoir un impact sur la recherche pour modéliser la JOG au cours de la déglutition et dans le RGO.

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Super Resolution problem is an inverse problem and refers to the process of producing a High resolution (HR) image, making use of one or more Low Resolution (LR) observations. It includes up sampling the image, thereby, increasing the maximum spatial frequency and removing degradations that arise during the image capture namely aliasing and blurring. The work presented in this thesis is based on learning based single image super-resolution. In learning based super-resolution algorithms, a training set or database of available HR images are used to construct the HR image of an image captured using a LR camera. In the training set, images are stored as patches or coefficients of feature representations like wavelet transform, DCT, etc. Single frame image super-resolution can be used in applications where database of HR images are available. The advantage of this method is that by skilfully creating a database of suitable training images, one can improve the quality of the super-resolved image. A new super resolution method based on wavelet transform is developed and it is better than conventional wavelet transform based methods and standard interpolation methods. Super-resolution techniques based on skewed anisotropic transform called directionlet transform are developed to convert a low resolution image which is of small size into a high resolution image of large size. Super-resolution algorithm not only increases the size, but also reduces the degradations occurred during the process of capturing image. This method outperforms the standard interpolation methods and the wavelet methods, both visually and in terms of SNR values. Artifacts like aliasing and ringing effects are also eliminated in this method. The super-resolution methods are implemented using, both critically sampled and over sampled directionlets. The conventional directionlet transform is computationally complex. Hence lifting scheme is used for implementation of directionlets. The new single image super-resolution method based on lifting scheme reduces computational complexity and thereby reduces computation time. The quality of the super resolved image depends on the type of wavelet basis used. A study is conducted to find the effect of different wavelets on the single image super-resolution method. Finally this new method implemented on grey images is extended to colour images and noisy images

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Accurate data of the natural conditions and agricultural systems with a good spatial resolution are a key factor to tackle food insecurity in developing countries. A broad variety of approaches exists to achieve precise data and information about agriculture. One system, especially developed for smallholder agriculture in East Africa, is the Farm Management Handbook of Kenya. It was first published in 1982/83 and fully revised in 2012, now containing 7 volumes. The handbooks contain detailed information on climate, soils, suitable crops and soil care based on scientific research results of the last 30 years. The density of facts leads to time consuming extraction of all necessary information. In this study we analyse the user needs and necessary components of a system for decision support for smallholder farming in Kenya based on a geographical information system (GIS). Required data sources were identified, as well as essential functions of the system. We analysed the results of our survey conducted in 2012 and early 2013 among agricultural officers. The monitoring of user needs and the problem of non-adaptability of an agricultural information system on the level of extension officers in Kenya are the central objectives. The outcomes of the survey suggest the establishment of a decision support tool based on already available open source GIS components. The system should include functionalities to show general information for a specific location and should provide precise recommendations about suitable crops and management options to support agricultural guidance on farm level.

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The entropy budget is calculated of the coupled atmosphere–ocean general circulation model HadCM3. Estimates of the different entropy sources and sinks of the climate system are obtained directly from the diabatic heating terms, and an approximate estimate of the planetary entropy production is also provided. The rate of material entropy production of the climate system is found to be ∼50 mW m−2 K−1, a value intermediate in the range 30–70 mW m−2 K−1 previously reported from different models. The largest part of this is due to sensible and latent heat transport (∼38 mW m−2 K−1). Another 13 mW m−2 K−1 is due to dissipation of kinetic energy in the atmosphere by friction and Reynolds stresses. Numerical entropy production in the atmosphere dynamical core is found to be about 0.7 mW m−2 K−1. The material entropy production within the ocean due to turbulent mixing is ∼1 mW m−2 K−1, a very small contribution to the material entropy production of the climate system. The rate of change of entropy of the model climate system is about 1 mW m−2 K−1 or less, which is comparable with the typical size of the fluctuations of the entropy sources due to interannual variability, and a more accurate closure of the budget than achieved by previous analyses. Results are similar for FAMOUS, which has a lower spatial resolution but similar formulation to HadCM3, while more substantial differences are found with respect to other models, suggesting that the formulation of the model has an important influence on the climate entropy budget. Since this is the first diagnosis of the entropy budget in a climate model of the type and complexity used for projection of twenty-first century climate change, it would be valuable if similar analyses were carried out for other such models.