4,127 research outputs found

    A comparison of the moss floras of Chile and New Zealand

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    Chile and New Zealand share a common stock of 181 species of mosses in 94 genera and 34 families. This number counts for 23.3% of the Chilean and 34.6% of the New Zealand moss flora. If only species with austral distribution are taken into account, the number is reduced to 113 species in common, which is 14.5% of the Chilean and 21.6% of the New Zealand moss flora. This correlation is interpreted in terms of long distance dispersal resp. the common phytogeographical background of both countries as parts of the palaoaustral floristic region and compared with disjunct moss floras of other continents as well as the presently available molecular data

    Senator Frank E. Moss (D., Utah) on "Opinion: Washington," Sunday, January 22, at 9:30 P.M. in color, on WTTG-Channel 5

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    Typed press release (13 pages) with a transcript of an interview with Utah Senator Frank E. Moss on a television program of Washington, D.C., Channel 5, WTTG, on 22 January 1967. Mark Evans, Vice President for Public Affairs at Metromedia, Inc., along with guest reporter Frank Hewlett of the Salt Lake Tribune, questioned Senator Moss on such subjects as public broadcasting, warning labels on cigarettes, legislation on consumer protection, the Vietnam War, and his concern about right-wing extremism

    ploewe/MOSS: v1.0

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    This is the first release of the MOSS codebase in its transient GitHub repository to ensure long term preservation of the codebase, scientific citation and due credit to the original authors (including Carl N Reed III and Sol Katz)

    022. Romans 11:25-32

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    Chapel Sermon by Mark Moss from Romans 11:25-32 on Tuesday, September 24, 2024. Para obtener una versión de subtítulos en español, vaya a CC en la parte inferior derecha del video y elija 2

    The moss Bryum argenteum var. muticum Brid. is well adapted to cope with high light in continental Antarctica

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    The net photosynthetic rate (NP), chlorophyll fluorescence, carotenoid content and chlorophyll content of the cosmopolitan moss Bryum argenteum were measured in the field at Botany Bay, southern Victoria Land, continental Antarctica (77°S). Comparisons were made between sun- and shade-adapted forms, and changes were followed as the moss emerged from under the snow and during exposure of shade and sun forms to ambient light. Shade forms had lower light compensation and saturation values for NP but little difference in maximal NP rates. Shade forms exposed to ambient light changed rapidly (within five days) towards the performance of the sun forms. Surprisingly, this change was not by acclimation of shoots but by the production of new shoots. Chlorophyll and carotenoid levels measured on a molar chlorophyll basis showed no difference between sun and shade forms and also little change during emergence. The constant molar relationship between carotenoids and chlorophyll plus the high levels of the xanthophyll cycle pigments suggest that protection of the chlorophyll antenna was constitutive. This is an adaptation to the very high light levels that occur when the plants are active in continental Antarctica and contrasts to the situation in more temperate areas where high light is normally avoided by desiccation

    Molecular support for Pleistocene persistence of the continental Antarctic moss Bryum argenteum

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    We examined sequence variation of ITS and phy2 for Bryum argenteum from Antarctica, sub-Antarctic, New Zealand and Australia to understand better taxonomic delimitations and resolve relationships between these geographic regions. Bryum argenteum has been recorded as two species, B. argenteum and B. subrotundifolium, in all four regions with the latter now referred to as B. argenteum var. muticum. We found disagreement between taxon delimitations (based on morphology) and molecular markers. All continental Antarctic specimens consistently formed a monophyletic sister group that consisted of both morphologically identified B. argenteum varieties, separate to all non-Antarctic specimens (also consisting of both varieties). We suggest, contrary to previous records, that all continental Antarctic (Victoria Land) populations are referable to B. argenteum var. muticum, while sub-Antarctic, Australian and New Zealand populations included here are B. argenteum var. argenteum. Additionally, since there was less genetic diversity within Victoria Land, Antarctica, than observed between non-Antarctic samples, we suggest that this is, in part, due to a potentially lower rate of DNA substitution and isolation in northern and southern refugia within Victoria Land since the Pleistocene.Simon F. K. Hills, Mark I. Stevens and Chrissen E. C. Gemmil

    Mark Kimber

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    This book encapsulates the photographic career to date of Mark Kimber, whose track record as an artist has its origins in the early 1980s when, only one year after graduating from art school, six of his prints were collected by the Art Gallery of South Australia. Since that time his photographs have been collected nationally and internationally and his curriculum vitae is evidence of a rich photographic legacy, spanning a fascinating time in the history of the medium.The essay by Jim Moss that accompanies Mark Kimber's photographs relates episodes from Mark's youth and early adulthood, drawing an animated profile of a complex and motivated individual. As a photographic artist Kimber is able to reap the fields of his imagination that were sown in the western suburbs of Adelaide, demographic aspects of which he has recreated with an uncanny, crepuscular precision. Other territories and citizens come under Mark's gaze and in more recent work he displays a proclivity for the creation of fictive worlds.Jim Moss's essay also sketches in a sense of the critical and technological evolution that has permeated photographic discourse and practice in the years since Mark Kimber first peered through a viewfinder. Throughout this period of change, a sensibility that has remained constant at the heart of Mark's repertoire is his battle of wits with what has been described as 'the uncontrollable intrusion of reality' that is intrinsic to the photograph.The age of the photograph as a discreet object unto itself has passed, but in the world of art the photographic image persists as an intriguing and often complex document. This book bears witness to an ongoing fascination with photography as a medium of creative expression, while simultaneously it celebrates the contribution of Mark Kimber to photographic art

    IBM PC Data Acquisition and Processing Software Evaluation

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    Commercially available software packages for IBM PC-compatibles are evaluated to use for data acquisition and processing work. Moss Landing Marine Laboratories (MLML) acquired computers since 1978 to use on shipboard data acquisition (Le. CTD, radiometric, etc.) and data processing. First Hewlett-Packard desktops were used then a transition to the DEC VAXstations, with software developed mostly by the author and others at MLML (Broenkow and Reaves, 1993; Feinholz and Broenkow, 1993; Broenkow et al, 1993). IBM PC were at first very slow and limited in available software, so they were not used in the early days. Improved technology such as higher speed microprocessors and a wide range of commercially available software made use of PC more reasonable today. MLML is making a transition towards using the PC for data acquisition and processing. Advantages are portability and available outside support

    Hawking-Moss transition with a black hole seed

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    \ua9 2020, The Author(s).We extend the concept of Hawking-Moss, or up-tunnelling, transitions in the early universe to include black hole seeds. The black hole greatly enhances the decay amplitude, however, order to have physically consistent results, we need to impose a new condition (automatically satisfied for the original Hawking-Moss instanton) that the cosmological horizon area should not increase during tunnelling. We motivate this conjecture physically in two ways. First, we look at the energetics of the process, using the formalism of extended black hole thermodynamics; secondly, we extend the stochastic inflationary formalism to include primordial black holes. Both of these methods give a physical substantiation of our conjecture
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