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  • 1
    Electronic Resource
    Electronic Resource
    Marie Unna hereditary hypotrichosis: report of a Chinese family and evidence for genetic heterogeneity (2004)
    Oxford, UK : Blackwell Science Ltd
    Clinical and experimental dermatology 29 (2004), S. 0 
    Details
    ISSN: 1365-2230
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Medicine
    Notes: Marie Unna hereditary hypotrichosis (MUHH) is a rare autosomal dominant disorder with progressive hair loss starting in early childhood and aggravating at puberty. Several studies have mapped the MUHH gene to chromosome 8p21. Here we report a Chinese MUHH family with variable phenotypes. All affected individuals have anomalies affecting both hair density and hair shafts. Major clinical characteristics, disease history and histological examination support the diagnosis of MUHH, but the features of scarring in this kindred are modest and none of the patients have vertex hair loss, which is in contrast with typical MUHH. We now report genotyping and linkage analysis using 11 polymorphic microsatellite markers spanning the MUHH locus at 8p. Two-point linkage analysis using these markers revealed significant exclusion of this locus (log of the odds scores 〈 − 2) at θ = 0 indicating that there is a range of clinical presentations in MUHH, and that more than one genetic locus is responsible for the disorder.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1111/j.1365-2230.2004.01570.x
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    Paper (German National Licenses)
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  • 2
    Electronic Resource
    Electronic Resource
    Coupling phases and amplitudes of minor constituents with temperature perturbations in the lower thermosphere (1994)
    Springer
    Annales geophysicae 12 (1994), S. 438-447 
    Details
    ISSN: 0992-7689
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Based on the linearized theory of atmospheric gravity waves (AGW) and considering the effects of temperature perturbation on the chemical rate coefficients, the formulae of coupling relations between nj/nj and T′/T driven by AGW (nj and T denote the background quantities) are described, the coupling phases and amplitudes of minor constituents O3, NO, H, OH, and O are analyzed in detail for the mesopause (86 km) and just upside of the O layer (100 km) at daytime. A general principle is outlined: the coupling phases are strongly dependent on density scale heights and perturbation scales, while the amplitudes are little affected by these two factors. A criterion to distinguish the coupling behavior is given: when the minor constituent number density scale height Hj satisfies 1-〈Gamma〉Hm/Hj〉0 (Hm denotes the scale height of the major constituent), the dynamical perturbation process always keeps the nj/nj in phase with T’/T, i.e. keeps the nj/nj in antiphase with that of the major constituent. The results obtained indicate that both the temperature dependence of reaction rate coefficients and the profile slopes of the O distribution may have a major influence on the behavior of the coupling relations.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/s00585-994-0438-0
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    Paper (German National Licenses)
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  • 3
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    Transverse field muon-spin rotation signature of the skyrmion-lattice phase in Cu_{2}OSeO_{3} (2015)
    American Physical Society (APS)
    Details
    Publication Date: 2015-06-09
    Description: Author(s): T. Lancaster, R. C. Williams, I. O. Thomas, F. Xiao, F. L. Pratt, S. J. Blundell, J. C. Loudon, T. Hesjedal, S. J. Clark, P. D. Hatton, M. Ciomaga Hatnean, D. S. Keeble, and G. Balakrishnan We present the results of transverse field (TF) muon-spin rotation ( μ + SR ) measurements on Cu 2 OSeO 3 , which has a skyrmion-lattice (SL) phase. We measure the response of the TF μ + SR signal in that phase along with the surrounding ones, and suggest how the phases might be distinguished using the result... [Phys. Rev. B 91, 224408] Published Fri Jun 05, 2015
    Keywords: Magnetism
    Print ISSN: 1098-0121
    Electronic ISSN: 1095-3795
    Topics: Physics
    Published by American Physical Society (APS)
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