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  • 1
    In: Pediatric Blood & Cancer, Wiley, Vol. 68, No. 9 ( 2021-09)
    Abstract: The cytokine storm of secondary haemophagocytic lymphohistiocytosis (sHLH)/macrophage activation syndrome (MAS) can cause life‐threatening multiorgan failure. Interleukin‐1 (IL‐1) receptor blockade with anakinra can be effective in the management of sHLH/MAS. Subcutaneous (SC) dosing regimens are widely described; however, intravenous (IV) dosing is advantageous where time‐critical intervention is vital and where SC oedema and/or hypoperfusion limits absorption. We review three critically ill children (aged 9, 11 and 17) with sHLH and rapidly progressive multiorgan dysfunction, successfully treated with continuous IV anakinra infusion. This case series significantly enhances the incipient knowledge regarding the safety and efficacy of IV anakinra for life‐threatening sHLH.
    Type of Medium: Online Resource
    ISSN: 1545-5009 , 1545-5017
    URL: Issue
    Language: English
    Publisher: Wiley
    Publication Date: 2021
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  • 2
    In: Advances in Space Research, Elsevier BV, Vol. 21, No. 11 ( 1998-1), p. 1527-1535
    Type of Medium: Online Resource
    ISSN: 0273-1177
    Language: English
    Publisher: Elsevier BV
    Publication Date: 1998
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    SSG: 16,12
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  • 3
    Online Resource
    Online Resource
    The Electrochemical Society ; 2016
    In:  ECS Meeting Abstracts Vol. MA2016-02, No. 46 ( 2016-09-01), p. 3327-3327
    In: ECS Meeting Abstracts, The Electrochemical Society, Vol. MA2016-02, No. 46 ( 2016-09-01), p. 3327-3327
    Abstract: Alkaline water electrolysis produces H 2 gas, which can be used as a fuel in H 2 /O 2 fuel cells to generate power. The most energy intensive step in water electrolysis is the evolution of O 2 due to the large anodic overpotential of the Oxygen Evolution Reaction (OER). 1 Thus, understanding and optimizing electrocatalysts for OER remains one of the grand challenges for both physical electrochemistry and energy science. For the OER in alkaline media, the best performing electrocatalysts are thermally prepared RuO 2 and IrO 2 , which exhibit the lowest OER overpotentials to date, but these oxides are expensive and somewhat unstable in alkaline media, rendering them impractical and uneconomical. 1 First row Transition Metal Oxides (TMO), e.g. Mn, Ni, Co or Fe, show great promise as alternative materials for OER, as they exhibit low overpotentials and high stability at lower costs than those of RuO 2 or IrO 2 . However, mechanistic studies of OER at TMO electrodes in alkaline media have been sparse and the nature of catalytic sites and the mechanism leading to O 2 evolution are not well understood. 2 In this work, pure and mixed Ni/Fe materials were electrochemically deposited on Ti supports to fabricate inexpensive electrocatalysts. Their potential as OER catalysts was elucidated in NaOH electrolyte with different amounts of Fe impurities; 1 ppb, 5 ppb and 102 ppb, as determined by Inductive Coupled Plasma (ICP) spectroscopy. The results indicate that the electrocatalytic activity of the materials depends on the ratio of Ni/Fe and the concentration of Fe impurities in the electrolyte. Most of the mixed catalysts show improved OER performances compared to the pure Ni and Fe oxide materials with respect to overpotential at 10 mA cm -2 , Figure 1(a), Tafel slope values and Turnover Frequencies (TOF) numbers. Interestingly, the pure and mixed Ni/Fe materials in the NaOH electrolyte containing 5 ppb Fe impurities exhibited lower overpotentials at 10mA cm -2 compared to the same material in the NaOH containing 1 ppb and 100 ppb, Figure 1(a). This is thought to be due to the substitution of the Fe ions in the electrolyte for the Ni atoms in the material lattice, improving the OER performance. 3 Pure and mixed manganese and ruthenium oxides were also examined in this work. The OER catalytic activity of pure manganese oxide compounds displaying overpotentials between 0.74 - 0.49 V at a current density of 10 mA cm -2 . Furthermore, when combined with other compounds this overpotential value further decreases. 4 However, mechanistic studies of the OER at thermally prepared DSA ® type Mn x O y electrodes in alkaline media have been sparse. 2 Several of the mixed Mn/Ru electrode materials in this study were found to exhibit significantly improved OER activity and stability when compared with pure RuO 2 films, Figure 1(b), while lowering the cost of producing the catalyst. 5 These Mn/Ru materials could therefore offer a competitive low-cost alternative to the already commercially available OER catalysts. The composition, morphology and structure of all the aforementioned materials are thoroughly characterised by X-Ray Photoelectron Spectroscopy (XPS), Raman spectroscopy and Scanning Electron Microscopy–Energy Dispersive X-Ray (SEM-EDX).  Finally, the Ni/Fe and Mn/Ru oxides will be a compared under cost and OER performance, to help identify the most economic and practical OER catalyst in this work.  Acknowledgements We would like to thank Science Foundation Ireland (SFI) under the Grant Number SFI/10/IN.1/I2969. References                 (1)           Lyons, M. E. G.; Doyle, R. L.; Fernandez, D.; Godwin, I. J.; Browne, M. P.; Rovetta, A. Electrochem. Commun. 2014 , 45 , 56-59.                 (2)           Fernández, J. L.; Gennero De Chialvo, M. R.; Chialvo, A. C. J. Appl. Electrochem. 2002 , 32 , 513-520.                 (3)           Klaus, S.; Louie, M. W.; Trotochaud, L.; Bell, A. T. The Journal of Physical Chemistry C 2015 , 119 , 18303-18316.                 (4)           Gao, M.-R.; Xu, Y.-F.; Jiang, J.; Zheng, Y.-R.; Yu, S.-H. J. Am. Chem. Soc. 2012 , 134 , 2930-2933.                 (5)           Browne, M. P.; Nolan, H.; Duesberg, G. S.; Colavita, P. E.; Lyons, M. E. G. ACS Catalysis 2016. Figure 1
    Type of Medium: Online Resource
    ISSN: 2151-2043
    Language: Unknown
    Publisher: The Electrochemical Society
    Publication Date: 2016
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  • 4
    Online Resource
    Online Resource
    Elsevier BV ; 1966
    In:  Physics Letters Vol. 19, No. 8 ( 1966-1), p. 684-686
    In: Physics Letters, Elsevier BV, Vol. 19, No. 8 ( 1966-1), p. 684-686
    Type of Medium: Online Resource
    ISSN: 0031-9163
    RVK:
    RVK:
    Language: English
    Publisher: Elsevier BV
    Publication Date: 1966
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  • 5
    Online Resource
    Online Resource
    Institute of Electrical and Electronics Engineers (IEEE) ; 1985
    In:  IEEE Transactions on Geoscience and Remote Sensing Vol. GE-23, No. 3 ( 1985-05), p. 241-245
    In: IEEE Transactions on Geoscience and Remote Sensing, Institute of Electrical and Electronics Engineers (IEEE), Vol. GE-23, No. 3 ( 1985-05), p. 241-245
    Type of Medium: Online Resource
    ISSN: 0196-2892
    Language: Unknown
    Publisher: Institute of Electrical and Electronics Engineers (IEEE)
    Publication Date: 1985
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  • 6
    In: Pediatric Obesity, Wiley, Vol. 16, No. 11 ( 2021-11)
    Abstract: Eating in the absence of hunger (EAH), the susceptibility to eat despite satiety, may increase overweight. While EAH has been established in school‐aged children, less is known about it during toddlerhood. Objectives This study assessed to what extent 18‐month‐old children eat in the absence of hunger, the stability of this behaviour at 24 months and the association of child eating behaviours with EAH. Methods Children were presented with four palatable finger foods (total 275 kcal) after dinner. Univariate GLM's assessed the association between EAH, child satiety and eating behaviours and energy intake of dinner at 18 and 24 months (n = 206 and 103, respectively). Another GLM was run to assess the association between EAH at both time points. Results Mean (±SD) energy intakes from dinner and finger foods were 240 kcal (±117) and 40 kcal (±37), respectively. No association was found between energy intake of dinner and finger foods. Enjoyment of food was significantly related to intake of finger foods ( P  = .005). EAH at 18 months predicted EAH at 24 months. Conclusion Eighteen‐month‐old children ate in the absence of hunger, irrespective of satiety. Thus, preceding energy intake was not compensated for. Other factors, for example, enjoyment of food seem to determine finger food intake.
    Type of Medium: Online Resource
    ISSN: 2047-6302 , 2047-6310
    URL: Issue
    Language: English
    Publisher: Wiley
    Publication Date: 2021
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  • 7
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1979
    In:  Journal of Geophysical Research: Space Physics Vol. 84, No. A10 ( 1979-10), p. 5781-5791
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 84, No. A10 ( 1979-10), p. 5781-5791
    Abstract: Energetic (keV) protons and 0 + ions with field aligned pitch angle distributions and peak fluxes up to ∼ 7 × 10 7 (cm² s sr keV) −1 have been observed streaming downward in the high altitude (∼ 1 R E ) auroral ionosphere. In two examples described in detail, the correlations observed between the downward flowing and coincident trapped ion populations suggest a common origin. Downward flowing ion events are a much less frequent phenomenon than upward flowing ion events in the auroral region. The significant difference implies that the energetic upward flowing ions from the auroral ionosphere are commonly injected into the trapped population of the plasma sheet, and furthermore that parallel electric fields involving potential drops of ≳500 V are directed preferentially upward in the altitude range from 2000 km to ∼ 3 R E . Spatially localized regions of enhanced hot (∼keV) plasma density were frequently observed in the low L portion of the plasma sheet. The statistical location of these ‘plasma clouds’ correlates well with the substorm injection boundary near dusk inferred by McIlwain (1974) and with the upward flowing ion events observed at ∼ 1 R E altitude (Ghielmetti et al., 1978a, b). The downward flowing ion events occurred preferentially within such ‘plasma clouds.’ The results described in this paper suggest that upward flowing ions from the auroral acceleration regions are responsible for both the downward flowing ions and for at least some of the plasma clouds. A significant fraction of the equatorial substorm injected plasma clouds may thus result from this ionospheric source region.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1979
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  • 8
    Online Resource
    Online Resource
    Elsevier BV ; 2000
    In:  Advances in Space Research Vol. 25, No. 12 ( 2000-1), p. 2417-2420
    In: Advances in Space Research, Elsevier BV, Vol. 25, No. 12 ( 2000-1), p. 2417-2420
    Type of Medium: Online Resource
    ISSN: 0273-1177
    Language: English
    Publisher: Elsevier BV
    Publication Date: 2000
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  • 9
    Online Resource
    Online Resource
    Elsevier BV ; 1985
    In:  Advances in Space Research Vol. 5, No. 4 ( 1985-1), p. 401-410
    In: Advances in Space Research, Elsevier BV, Vol. 5, No. 4 ( 1985-1), p. 401-410
    Type of Medium: Online Resource
    ISSN: 0273-1177
    Language: English
    Publisher: Elsevier BV
    Publication Date: 1985
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  • 10
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1980
    In:  Journal of Geophysical Research: Space Physics Vol. 85, No. A1 ( 1980-01), p. 92-100
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 85, No. A1 ( 1980-01), p. 92-100
    Abstract: Intense beams of electrons with energies in the keV range have been observed streaming simultaneously both parallel and antiparallel to the magnetic field direction at altitudes between 4000 and 8000 km at auroral latitudes. The peak flux observed was 3 × 10 11 (cm² s sr keV) −1 at an energy of 160 eV. The beams are often tightly collimated with widths in pitch angle as narrow as ∼1°. Analysis of the energy spectrums of the beams and the simultaneously observed loss cones in the trapped electron population shows that the energization of the beams cannot be understood as acceleration by a simple quasi‐static parallel electric field. Alternative models include acceleration by wave‐particle interactions or by fluctuating electric fields. One candidate model consistent with the observations is outlined in which the energetic electrons in the counterstreaming electron beams are accelerated from the ambient cold plasma by multiple flickering double layers located in the 1‐ R E altitude range.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1980
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