552 research outputs found

    Dietary practices and xenophthalmia in under-fives in Jimma town, Southwest Ethiopia

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    Objectives: To assess parent’s knowledge about children’s need for plant sources of vitamin A; to determine the dietary practice with regard to vitamin A intake; to estimate the prevalence of xerophthalmia and; to forward appropriate recommendations.Design: A cross-sectional study.Setting: The study was conducted in Jimma town, southwest Ethiopia, with a total population of about 88,867 from February to April 1995.Participants: Eight hundred and thirty one randomly selected children between the ages of six and 59 months formed the study population.Main outcome measures: The dietary intake of cheap and easily available vitamin A rich foods is assessed and prevalence of xerophthalmlia determined.Results: Only eighty per cent of the children were getting green vegetables, fruits or carrots once weekly or more. The major reasons given for not including vegetables, fruits and carrots in the diet were “cannot afford” (39%), “not available” (33%), and “child too young” (16%). Out of 628 children examined, four (0.6%) were found to have xerophthalmia; three (0.48%) classified as XlB and one (0.16%) as X2.Conclusion: The dietary intake of plant sources of vitamin A in the studied community is far from adequate. Moreover, vitamin A deficiency is found to be a significant public health problem in young children in Jimma town. Periodic vitamin A supplementation, preferablycombined with immunisation, should be a priority action, and parents need to be educated about vitamin A deficiency and its prevention

    Multi-Level Analysis and Spatial Interpolation of Distributions and Predictors of Childhood Diarrhea in Nigeria.

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    Background: Diarrhea is one of the health problems contributing to Nigeria's under-5 mortality rate, ranked as the eighth highest globally. As our search is concerned, there is limited evidence on the spatial distribution of childhood diarrhea in Nigeria. Therefore, this study aimed to examine the spatial distribution and predictors of diarrhea among under-5 children in Nigeria. Materials and Methods: Using data from the child's recode file of the 2018 Nigeria Demographic and Health Survey, a sample of 28 583 children of women of reproductive age was considered as the sample size for this study. The outcome variable used in this study was childhood diarrhea. We employed both multilevel and spatial analyses to ascertain the factors associated with childhood diarrhea as well as its spatial clustering. Results: The regional distribution of the prevalence of diarrhea among children in Nigeria ranged from 0% to 62%. The hotspots for childhood diarrhea were in Yobe, Bauchi, Gombe, Kano, Sokoto, Imo, and Taraba. The likelihood of a child having diarrhea in Nigeria was higher among women whose partners have secondary education and above [aOR = 1.18; 95%CI = 1.05-1.33], women currently working [aOR = 1.24; 95%CI = 1.13-1.35], women practicing Islam [aOR = 1.24; 95%CI = 1.04-1.46], and women who were exposed to mass media [aOR = 1.29; 95%CI = 1.18-1.42], compared to women whose partners had no formal education, women not currently working, women practicing Christianity, and those who were not exposed to mass media. Children born to mothers who reside in North East [aOR = 2.55; 95%CI = 2.10-3.10], and communities with medium socioeconomic status [aOR = 1.44; 95%CI = 1.09-1.91] were more likely to experience diarrhea compared to those born to mothers residing in the North Central and in communities with low socioeconomic status. Conclusion: High proportions of childhood diarrhea among under-5 children in Nigeria were located in Yobe, Bauchi, Gombe, Kano, Sokoto, Imo, and Taraba. Policies and interventions that seek to reduce or eliminate diarrhea diseases among under-5 children in Nigeria should take a keen interest in the factors identified as predictors of childhood diarrhea in this study as this will help in achieving the aims of WASH, ORT corners, and SDG 3 by the year 2030

    Oestrus synchronization for accelerated delivery of improved dairy genetics in Ethiopia: Results from action research and development interventions

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    Oestrous synchronization is the manipulation of the oestrous cycle or induction of oestrus to bring a large percentage of a group of females cattle into oestrus at a short, predetermined time. The first field trial on hormonal oestrous synchronization regime and mass artificial insemination was conducted by the Improving Productivity and Market Success (IPMS) project in Tigray and Southern Nations, Nationalities, and Peoples' Region (SNNP) regions. The objective was to improve access to improved dairy genetics by smallholder farmers and to kick-start market-oriented smallholder dairy development in Ethiopia. Following the field trial, the synchronization technology was adopted and scaled up by the Ministry of Agriculture (MoA) and regional Bureaus of Agriculture (BoAs) in collaboration with the IPMS and Livestock and Irrigation Value Chains for Ethiopian Smallholders (LIVES) projects of the International Livestock Research Institute (ILRI)) and the national research system. Performance of the scaled up project was inconsistent in the application of the technology and the results achieved. This working paper synthesizes results of action research activities and performance of the technology at larger scale, discuss implications of the results and draw recommendations for effective and sustained application of the technology in Ethiopia

    Magnetic Connectivity between Active Regions 10987, 10988, and 10989 by Means of Nonlinear Force-Free Field Extrapolation

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    Extrapolation codes for modelling the magnetic field in the corona in cartesian geometry do not take the curvature of the Sun's surface into account and can only be applied to relatively small areas, \textit{e.g.}, a single active region. We apply a method for nonlinear force-free coronal magnetic field modelling of photospheric vector magnetograms in spherical geometry which allows us to study the connectivity between multi-active regions. We use vector magnetograph data from the Synoptic Optical Long-term Investigations of the Sun survey (SOLIS)/Vector Spectromagnetograph(VSM) to model the coronal magnetic field, where we study three neighbouring magnetically connected active regions (ARs: 10987, 10988, 10989) observed on 28, 29, and 30 March 2008, respectively. We compare the magnetic field topologies and the magnetic energy densities and study the connectivities between the active regions(ARs). We have studied the time evolution of magnetic field over the period of three days and found no major changes in topologies as there was no major eruption event. From this study we have concluded that active regions are much more connected magnetically than the electric current.Comment: Solar Physic

    Nitrogen response functions targeted to technology extrapolation domains in Ethiopia using CERES-maize

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    The profitability of fertilizer-N use can be optimized using N response functions specific to climate-based technology extrapolation domains (TED). Crop growth simulation can complement field research for targeting of response functions. The objective of this study was to target maize (Zea mays L.) N response functions to seven TED in Ethiopia through CERES-Maize simulation of continuous maize over 30 yr. The complete factorial set of treatments included seven levels of N in 25 kg ha−1 increments under no-till (NT) and conventional tillage (CT) systems. The CERES-Maize simulated experiments were done for two or three sites per TED. Nitrogen response functions were generated for each TED with tillage-specific functions for three TED with tillage × N interactions. The N rate responses for all TED fit curvilinear to plateau functions but with differing magnitudes and shapes of response. The mean yield with NT was 6% less than with CT, but the difference declined with increased N rate. The economically optimum N rate (EONR) ranged from 65 to 179 and 103 to 243 kg ha−1 for high and low-cost fertilizer-N, respectively. The EONR was 6% less and the profit cost ratio was 11% higher with CT compared to NT, indicating greater fertilizer-N need with NT than with CT. The application of N for maize was highly profitable for all TED. The EONR from CERES-Maize were higher than past field research results. This suggests that the CERES-Maize N response functions were most appropriate for well-managed crop production situations in Ethiopia

    3D Coronal Density Reconstruction and Retrieving the Magnetic Field Structure during Solar Minimum

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    Measurement of the coronal magnetic field is a crucial ingredient in understanding the nature of solar coronal phenomena at all scales. We employed STEREO/COR1 data obtained during a deep minimum of solar activity in February 2008 (Carrington rotation CR 2066) to retrieve and analyze the three-dimensional (3D) coronal electron density in the range of heights from 1.5 to 4 Rsun using a tomography method. With this, we qualitatively deduced structures of the coronal magnetic field. The 3D electron density analysis is complemented by the 3D STEREO/EUVI emissivity in the 195 A band obtained by tomography for the same CR. A global 3D MHD model of the solar corona was used to relate the reconstructed 3D density and emissivity to open/closed magnetic field structures. We show that the density maximum locations can serve as an indicator of current sheet position, while the locations of the density gradient maximum can be a reliable indicator of coronal hole boundaries. We find that the magnetic field configuration during CR 2066 has a tendency to become radially open at heliocentric distances greater than 2.5 Rsun. We also find that the potential field model with a fixed source surface (PFSS) is inconsistent with the boundaries between the regions with open and closed magnetic field structures. This indicates that the assumption of the potential nature of the coronal global magnetic field is not satisfied even during the deep solar minimum. Results of our 3D density reconstruction will help to constrain solar coronal field models and test the accuracy of the magnetic field approximations for coronal modeling.Comment: Published in "Solar Physics
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