15,600 research outputs found

    Trump Approval Unchanged in NH; High Awareness of Mueller Investigation 8/22/18

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    New Hampshire residents\u27 assessment of Donald Trump\u27s performance as President is unchanged since April. Just over half of residents continue to say the Mueller investigation is a serious matter that should be fully investigated and few would support Trump firing Robert Mueller, though support for such an action among Republicans has increased

    Approval of Trump On the Rise in NH; Residents Support Mueller Investigation 4/23/18

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    New Hampshire residents have become somewhat more positive in their assessment of Donald Trump\u27s performance as president. Approval of his overall job performance, handling of the economy and foreign affairs, and his personal favorability have all increased since February, with the largest gains among Independents. More than half of Granite Staters say the Mueller investigation is a serious matter that should be fully investigated and few support President Trump firing Robert Mueller

    Non-spherical core collapse supernovae and nucleosynthesis

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    Motivated by observations of supernova SN 1987A, various authors have simulated Rayleigh-Taylor (RT) instabilities in the envelopes of core collapse supernovae (for a review, see Mueller 1998). The non-radial motion found in these simulations qualitatively agreed with observations in SN 1987A, but failed to explain the extent of mixing of newly synthesized 56Ni quantitatively. Here we present results of a 2D hydrodynamic simulation which re-addresses this failure and covers the entire evolution of the first 5 hours after core bounce.Comment: 4 pages, 1 figure, LaTeX, requires espcrc1.sty. To appear in Nucl. Phys. A., the proceedings of the conference "Nuclei in the Cosmos 2000", held in Aarhus, Denmark, June 27-July 1, 200

    EEOC v. Mueller Industries, Inc.,

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    Snippets Filmed Sandow´s Biography

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    Actas del Segundo Congreso Internacional de Historia y Cine organizado por el Instituto de Cultura y Tecnología Miguel de Unamuno y celebrado del 9 al 11 de septiembre de 2010 en la Universidad Carlos III de MadridLa “mirada del cine”, utilizando un término de la Profa. Gloria Camarero, no ha analizado con justicia, hasta el momento, la figura de Fredrick Mueller (Kaliningrado, 1867-Londres,1925), uno de los primeros antecedentes de los posteriormente considerados como iconos de la cultura de masas. Artísticamente Mueller adoptará el nombre de Eugen Sandow y presentará en su azarosa vida, personal y profesional, las características definitorias de los massmedia: una biografía singular, ser un número uno en su profesión, crear nuevos conceptos con valencia mundial que han trascendido a su propia época, poseer fama en varios países y continentes (Europa, América del Norte, Australia), generar un abundante material gráfico y fotográfico, incluirse en los principales medios de comunicación de su época (prensa, radio, filmaciones), ser objeto de campañas publicitarias, generar objetos de merchandaising, provocar el interés general y ser estudiado por especialistas.The "film look" using a term of Prof. Gloria Camarero, justice has not been analyzed so far, the figure of Fredrick Mueller (Kaliningrad ,1867-London, 1925), one of the early history of the later regarded as icons of mass culture. Mueller artistically take the name of Eugen Sandow and present in his eventful life, personally and professionally, the defining characteristics of the mass media: a singular biography, to be a number one in his profession, creating new global valence concepts that have transcended their own time, have known in several countries and continents (Europe, North America, Australia), generating a wealth of graphic and photographic material, included in the mainstream media of his day (newspapers, radio, films), be the subject of advertising campaigns generate merchandising items, provoke interest and be examined by specialists.Publicad

    Energetic particle flux experiment (IMP F and G)

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    The data reduction procedures and programs for analysis of the IMP F and G energetic particle flux experiments are summarized. The IMP-F experiment contained two thin-window Geiger-Mueller detectors and an ionization chamber. There were two IMP-G experiments: one with six Geiger-Mueller detectors and an ionization chamber, and the other with two funnel mouthed channeltrons in a parallel plate electrostatic analyzer. These experiments measured particles in the energy range above 20 keV (IMP-F) and above approximately 5 keV (IMP-G). A bibliography is presented of papers containing the scientific results. These data were predominantly used for the study of low energy solar particles from flares
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