155,209 research outputs found

    Newton D. Kelly Civil War letter

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    This collection contains a letter written by Newton D. Kelly of the 1st Nebraska Cavalry while serving at DeValls Bluff, Arkansas

    Louie D. Newton papers

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    The Louie D. Newton collection includes correspondence, clippings, printed material, photographs, ephemera, and a scrapbook (1939) of clippings pertaining to the Baptist World Alliance. The materials document Newton's pastorate at Druid Hills Baptist Church (Atlanta, Ga.), his activities with the Southern Baptist Convention, and his broadcasts on WSB radio.The Louie D. Newton collection includes correspondence, clippings, printed material, photographs, ephemera, and a scrapbook (1939) of clippings pertaining to the Baptist World Alliance. The materials document Newton's pastorate at Druid Hills Baptist Church (Atlanta, Ga.), his activities with the Southern Baptist Convention, and his broadcasts on WSB radio

    Newton D. Baker portrait

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    Newton Baker (1871-1937) was born in Martinsburg, West Virginia, in 1871. Baker moved to Cleveland, Ohio, sometime around the turn of the century. He set up a law practice in the town and, in 1903, was appointed the city's Director of Law. Baker served as Democratic mayor of Cleveland from 1912 to 1916. He stepped down to serve as Secretary of War under President Woodrow Wilson. He appointed General John Pershing to head the American Expeditionary Force in the First World War. In 1921 he stepped down to return to his law practice but remained active in the Democratic Party. He died on December 25, 1937

    Transforming the built environment through construction

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    Achieving sustainable urban development for a projected global population of 9.2 billion in 2050, 70 per cent of whom will be living in urban settings (United Nations 2008), represents one of the principal challenges of the twenty-first century. Australia, as one of the world's most urbanized societies, led this global transition 125 years ago. Its cities are classed among the world's most liveable. Liveability, however, does not equate to sustainability. Indeed the current trajectory of Australia's urban development has been classed as unsustainable (Newton 2006, 2007a)

    [Letter from Louie D. Newton to T. N. Carswell - June 15, 1946]

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    A letter written to Mr. T. N. Carswell, Abilene, Texas, from Louie D. Newton, Pastor, Druid Hills Baptist Church, Atlanta, Georgia, dated June 15, 1946. Newton expresses to Carswell his appreciation for the gracious letter of June 11th and asks that Carswell remember him in his prayers

    Letter From Newton D. Baker to Francis Mairs Huntington-Wilson, January 8, 1918

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    A typed letter from Newton D. Baker to Francis Mairs Huntington-Wilson, dated January 8, 1918. Within, Baker writes in response to Wilson\u27s renewed offer of service to the War Department.https://digitalcommons.ursinus.edu/fmhw_firstworldwar_documents/1050/thumbnail.jp

    D. Hiden Ramsey and Frank P. Graham

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    The Golden Anniversary and Golden Jubilee on Saturday October 28, 1939, celebrated the 50th anniversary of Western Carolina Teachers College, homecoming, and the opening of six new buildings on campus. Officials and educators from across the state were present. This photograph taken by W. Newton Turner (1910-1995) shows (left to right) D. Hiden Ramsey (1891-1966) and president of the North Carolina University system Frank P. Graham (1886-1972). Turner began teaching as an assistant professor of geology and geography in 1937 and filled a variety of roles before retiring on December 29, 1971 as Vice President of Western Carolina University

    Métodos de Krylov-Newton aplicados à simulação numérica de reservatórios de petróleo

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    Dissertação (mestrado) - Universidade Federal de Santa Catarina, Centro Tecnológico.A simulação do processo de extração de óleo em um reservatório de petróleo é um problema complexo que envolve o escoamento multifásico em um meio poroso de geometria arbitrária, podendo conter falhas geológicas e outras irregularidades. A modelagem numérica implícita deste problema requer a solução de um complexo sistema de equações não-lineares que pode ser resolvido de diversas formas, mais ou menos eficientes. A forma mais comum de solução deste sistema emprega o método de linearização de Newton ou alguma de suas variantes. O foco deste trabalho está na análise de uma extensa classe de métodos de Newton conhecidos como métodos de Newton inexatos. Estes métodos empregam um segundo método iterativo na solução da equação linearizada resolvendo-a até uma certa tolerância; daí serem chamados de inexatos. Os métodos inexatos abordados neste trabalho concentram-se na escolha de processos iterativos baseados em métodos de projeção no espaço de Krylov, tais como: GMRES, BICGSTAB, TFQMR. Estes métodos, que formam uma subclasse dos métodos de Newton inexatos, são conhecidos como métodos de Krylov-Newton. São abordados também métodos quase-newtonianos baseados na aproximação da matriz Jacobiana considerando apenas os termos ortogonais da discretização em sistemas curvilíneos não-ortogonais. Vários problemas com diferentes graus de não-ortogonalidade da malha e não-linearidades são resolvidos e comparados usando os diferentes métodos implementados

    Latest results on Jovian disk X-rays from XMM-Newton

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    We present the results of a spectral study of the soft X-ray emission (0.2–2.5 keV) from low-latitude (‘disk’) regions of Jupiter. The data were obtained during two observing campaigns with XMM-Newton in April and November 2003. While the level of the emission remained approximately the same between April and the first half of the November observation, the second part of the latter shows an enhancement by about 40% in the 0.2–2.5 keV flux. A very similar, and apparently correlated increase, in time and scale, was observed in the solar X-ray and EUV flux. The months of October and November 2003 saw a period of particularly intense solar activity, which appears reflected in the behavior of the soft X-rays from Jupiter's disk. The X-ray spectra, from the XMM-Newton EPIC CCD cameras, are all well fitted by a coronal model with temperatures in the range 0.4–0.5 keV, with additional line emission from Mg XI (1.35 keV) and Si XIII (1.86 keV): these are characteristic lines of solar X-ray spectra at maximum activity and during flares. The XMM-Newton observations lend further support to the theory that Jupiter's disk X-ray emission is controlled by the Sun, and may be produced in large part by scattering, elastic and fluorescent, of solar X-rays in the upper atmosphere of the planet

    Death Registration for Ann McAuliff Dalton

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    text document the City of Newton, Massachusetts death register line 83 for Ann McAuliff Dalton date of death February 24,1896Converted from .jpg to .pdf for compatibilit
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