651 research outputs found

    The Size Relationship of 12 Days Post-Exodus Larvae with 56 Day Post-Exodus Fingerlings Regarding Growth and Survival in Bluegill (Lempomis macrochirus)

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    Low survival and quality of early life-stage bluegill is an obstacle to viable production where size may influence weaning efficiency. Herein, we investigate through two trials the effects of fry size 12-d post-exodus on total length, weight, production and survival through 56-d post-exodus. Full sibling broods (trial 1=10, trial 2=6) were reared with feedings of brine shrimp Artemia sp. nauplii (BS) through 12-d post-exodus (PE). Broods of trial 1 were visual sorted 12 d PE into small and large size groups. Fry (n = 25) from each size group were sampled for measured total length (TL) and weight. Starting 14 d PE, a 7-d co-feeding period with a commercial dry feed (#0 crumb) that was continued through 27 d PE with subsequent feedings using a larger version (#1 crumb) of the same diet continuing through 56 d PE (trial end). Broods of trial 2 were split 4 d post-conception into two gorups of pro-larvae (n = 400). Slow growing groups were fed hourly 0800-1700 while fast growing were fed additionally at 0400 and 2200 through 12 d PE. Surviving fish from each size gorup were collected, with random samples (n = 25 fish) measured for TL and weight. Fry (n = 100 where possible) were placed into 151-L aqauriums with slow and fast growing feed regimens maintained through 13-d PE. Culture regimen thereafter was same as trial 1. Fish of both trials were harvested, measured for TL, weight, and survival. The Wilcoxon Signed Rank Test was run one-tailed using SAS. Results of trial 1 indicate size at 12 d was a predictor of TL, weight and survival through 56 d PE (p ≀ 0.156). Size variation at 12 d as a function of genetics is a predictor of growth and survival through 56 d while at least some size variation resulting from early growth rate differences can be overcome by compensatory growth.https://bluetigercommons.lincolnu.edu/lucer-pubs/1007/thumbnail.jp

    Current situation of rapid multiplication techniques for early generation seed potato production in Sub-Saharan Africa

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    This paper provides insights on the principal actors in producing in vitro plantlets, cuttings, and minitubers, with emphasis on the technologies used, the production capacity in place, and challenges. One of the key findings is that the total production of minitubers in the seven countries increased tenfold from 2008 to 2017. In this regard, Kenya and Rwanda turn out to be the major investors and producers of EGS potato in SSA. Schematic representations are used to depict the organizational structures of national formal seed systems. Rapid multiplication techniques used, including aeroponics, hydroponics, and rooted apical cuttings, are described and their comparative advantages to the conventional technique outlined. We also provide an overview on the germplasm used in seed systems, with a special focus on end-users’ preferences. The paper also provides contextualized suggestions on how to improve the efficiency of the seed systems analyzed

    Ten questions on the soundscapes of the built environment

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    Soundscape research represents a paradigm shift from noise control policies towards a new multidisciplinary approach as it involves not only physical measurements but also the cooperation of humanity and social sciences to account for the diversity of soundscapes across countries and cultures, with more focus on how people actually experience the acoustic environments; and it considers environmental sounds as a ‘resource’ rather than a ‘waste’. The ten questions presented in this paper range from the very basic definitions underlying the emerging soundscape ‘science’, to more applied topics about how to use soundscape as a design approach for the planning and management of the built environments. Although significant research activity has been conducted so far, there is still a need to systematically provide the underpinning science and practical guidance in soundscaping. Thus, the last question aims to identify the most crucial gaps in soundscape research and set the agenda for future advancements in the field

    Damage detection and location in woven fabric CFRP laminate panels

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    The need for multifunctional carbon fibre composite laminates has emerged to improve the reliability and safety of carbon fibre composite components and decrease costs. The development of an electrical selfsensing system for woven fabric carbon fibre composite laminate panels which can detect and locate damage due to impact events is presented. The electrical sensing system uses a four probe electrical resistance method. Two different sensing mats are investigated, the main difference between them are the surface area of the electrodes and the distance between the electrodes. To investigate the damage sensitivity of the sensing system for woven fabric carbon fibre composite laminate panels, panels are produced with various thicknesses from 0.84 to 3.5 mm and are impacted at energies from 1 to 10 J to generate barely visible impact damage. Damage is detected using global electrical resistance changes, the changes in electrical resistance vary depending on carbon fibre volume fraction, spacing distance between the sensing electrodes in the sensing mats, the surface area of the electrodes, damage size, and damage type; it is found that the thicker the panel, the less sensitive the electrical resistance system is. The effect of the surface area of the sensing electrodes is high on the electrical resistance baseline, where the baseline increases by up to 55% when the surface area of the sensing electrodes increases from 100 mm2 to 400 mm2; while spacing distance between electrodes has a greater effect on damage sensitivity of the electrical resistance sensing system than the surface area of the sensing electrodes

    The threat of the COVID-19 pandemic on reversing global life-saving gains in the survival of childhood cancer: A call for collaborative action from SIOP, IPSO, PROS, WCC, CCI, st jude global, UICC and WHPCA

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    The COVID-19 pandemic poses an unprecedented health crisis in all socio-economic regions across the globe. While the pandemic has had a profound impact on access to and delivery of health care by all services, it has been particularly disruptive for the care of patients with life-threatening noncommunicable diseases (NCDs) such as the treatment of children and young people with cancer. The reduction in child mortality from preventable causes over the last 50 years has seen childhood cancer emerge as a major unmet health care need. Whilst survival rates of 85% have been achieved in high income countries, this has not yet been translated into similar outcomes for children with cancer in resource-limited settings where survival averages 30%. Launched in 2018, by the World Health Organization (WHO), the Global Initiative for Childhood Cancer (GICC) is a pivotal effort by the international community to achieve at least 60% survival for children with cancer by 2030. The WHO GICC is already making an impact in many countries but the disruption of cancer care during the COVID-19 pandemic threatens to set back this global effort to improve the outcome for children with cancer, wherever they may live. As representatives of the global community committed to fostering the goals of the GICC, we applaud the WHO response to the COVID-19 pandemic, in particular we support the WHO's call to ensure the needs of patients with life threatening NCDs including cancer are not compromised during the pandemic. Here, as collaborative partners in the GICC, we highlight specific areas of focus that need to be addressed to ensure the immediate care of children and adolescents with cancer is not disrupted during the pandemic; and measures to sustain the development of cancer care so the long-term goals of the GICC are not lost during this global health crisis.Fil: Pritchard Jones, Kathy. University College London; Estados UnidosFil: de Abib, Simone C.V.. International Society Of Paediatric Surgical Oncology; Surinam. Universidade Federal de Sao Paulo; BrasilFil: Esiashvili, Natia. University of Emory; Estados UnidosFil: Kaspers, Gertjan J.L.. Princess MĂĄxima Center for Pediatric Oncology; PaĂ­ses BajosFil: Rosser, Jon. No especifĂ­ca;Fil: van Doorninck, John A.. Rocky Mountain Hospital for Children; Estados UnidosFil: Braganca, JoĂŁo M.L.. No especifĂ­ca;Fil: Hoffman, Ruth I.. No especifĂ­ca;Fil: Rodriguez Galindo, Carlos. St Jude Children’s Research Hospital; Estados UnidosFil: Adams, Cary. Union for International Cancer Control; SuizaFil: Connor, Stephen R.. Worldwide Hospice Palliative Care Alliance; Estados UnidosFil: Abdelhafeez, Abdelhafeez H.. International Society of Paediatric Surgical Oncology; Suiza. St. Jude Children’s Research Hospital; Estados UnidosFil: Bouffet, Eric. University Of Toronto. Hospital For Sick Children; CanadĂĄ. International Society of Paediatric Surgical Oncology; SuizaFil: Howard, Scott C.. International Society of Paediatric Surgical Oncology; Suiza. University of Tennessee; Estados UnidosFil: Challinor, Julia M.. International Society of Paediatric Surgical Oncology; Suiza. University of California; Estados UnidosFil: Hessissen, Laila. Children Hospital of Rabat; Marruecos. International Society of Paediatric Surgical Oncology; SuizaFil: Dalvi, Rashmi B.. Bombay Hospital Institute of Medical Sciences; India. International Society of Paediatric Surgical Oncology; SuizaFil: Kearns, Pamela. International Society of Paediatric Surgical Oncology; SuizaFil: Chantada, Guillermo Luis. International Society of Paediatric Surgical Oncology; Suiza. Consejo Nacional de Investigaciones CientĂ­ficas y TĂ©cnicas; ArgentinaFil: Frazier, Lindsay A.. International Society of Paediatric Surgical Oncology; Suiza. Dana-Farber Cancer Institute; Estados UnidosFil: Sullivan, Michael J.. University of Melbourne; Australia. International Society of Paediatric Surgical Oncology; SuizaFil: Schulte, Fiona S.M.. University of Calgary; CanadĂĄ. International Society of Paediatric Surgical Oncology; SuizaFil: Morrissey, Lisa K.. Boston Children’s Hospital; Estados Unidos. International Society of Paediatric Surgical Oncology; SuizaFil: Kozhaeva, Olga. European Society for Paediatric Oncology; BĂ©lgicaFil: Luna Fineman, Sandra. Children’s Hospital Colorado; Estados Unidos. International Society of Paediatric Oncology; SuizaFil: Khan, Muhammad S.. Tawam Hospital; Emiratos Arabes Unido

    The exposure of the hybrid detector of the Pierre Auger Observatory

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    The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays. It consists of a surface array to measure secondary particles at ground level and a fluorescence detector to measure the development of air showers in the atmosphere above the array. The "hybrid" detection mode combines the information from the two subsystems. We describe the determination of the hybrid exposure for events observed by the fluorescence telescopes in coincidence with at least one water-Cherenkov detector of the surface array. A detailed knowledge of the time dependence of the detection operations is crucial for an accurate evaluation of the exposure. We discuss the relevance of monitoring data collected during operations, such as the status of the fluorescence detector, background light and atmospheric conditions, that are used in both simulation and reconstruction.Comment: Paper accepted by Astroparticle Physic

    All-particle cosmic ray energy spectrum measured with 26 IceTop stations

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    We report on a measurement of the cosmic ray energy spectrum with the IceTop air shower array, the surface component of the IceCube Neutrino Observatory at the South Pole. The data used in this analysis were taken between June and October, 2007, with 26 surface stations operational at that time, corresponding to about one third of the final array. The fiducial area used in this analysis was 0.122 km^2. The analysis investigated the energy spectrum from 1 to 100 PeV measured for three different zenith angle ranges between 0{\deg} and 46{\deg}. Because of the isotropy of cosmic rays in this energy range the spectra from all zenith angle intervals have to agree. The cosmic-ray energy spectrum was determined under different assumptions on the primary mass composition. Good agreement of spectra in the three zenith angle ranges was found for the assumption of pure proton and a simple two-component model. For zenith angles {\theta} < 30{\deg}, where the mass dependence is smallest, the knee in the cosmic ray energy spectrum was observed between 3.5 and 4.32 PeV, depending on composition assumption. Spectral indices above the knee range from -3.08 to -3.11 depending on primary mass composition assumption. Moreover, an indication of a flattening of the spectrum above 22 PeV were observed.Comment: 38 pages, 17 figure
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