1,863,822 research outputs found

    PAMELA Overview : design goals and principles

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    The PAMELA (Particle Accelerator for MEdicaL Applications) project is to design an accelerator for proton and light ion therapy using non-scaling Fixed Field Alternating Gradient (FFAG) accelerators, as part of the CONFORM project, which is also constructing the EMMA electron model of a non-scaling FFAG at Daresbury. This paper presents an overview of the PAMELA design, and a discussion of the design goals and the principles used to arrive at a preliminary specification of the accelerator

    Cohen, Pamela and Leonard Trip to the U.S.S.R. (98 digital images)

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    Photographs within the folder were taken during Pamela B. Cohen's travels in the U.S.S.R. and during various events related to the American Soviet Jewry Movement.Digital ImageDigital finding aid

    Pamela Levy: Art Forum

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    28 May 1997. Note with tape: Pamela Levy is a figurative painter and printmaker based in Israel. Her work explores the human condition in the Middle East. While in Australia Pamela Levy is Visiting Artist in the CSA Painting Workshop, and her work is exhibited in Photospace, 16-20 June

    Pamela: development of the RF system for a non-relativistic non-scaling FFAG

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    The PAMELA project(Particle Accelerator For MEdical Applications) currently consists of the design of a particle therapy facility. The project, which is in the design phase, contains Non-Scaling FFAG, particle accelerator capable of rapid beam acceleration, giving a pulse repetition rate of 1kHz, far beyond that of a conventional synchrotron. To realise the repetition rate, a key component of the accelerator is the rf accelerating system. The combination of a high energy gain per turn and a high repetition rate is a significant challenge. In this paper, options for the rf system of the proton ring and the status of development are presented

    Pamela Gaunt

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    Cosmic-Ray Positron Energy Spectrum Measured by PAMELA

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    Precision measurements of the positron component in the cosmic radiation provide important information about the propagation of cosmic rays and the nature of particle sources in our Galaxy. The satellite-borne experiment PAMELA has been used to make a new measurement of the cosmic-ray positron flux and fraction that extends previously published measurements up to 300 GeV in kinetic energy. The combined measurements of the cosmic-ray positron energy spectrum and fraction provide a unique tool to constrain interpretation models. During the recent solar minimum activity period from July 2006 to December 2009, approximately 24 500 positrons were observed. The results cannot be easily reconciled with purely secondary production, and additional sources of either astrophysical or exotic origin may be required

    Chafe, Pamela. Portrait of Chafe.

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    Photo from Pamela Chafe; date unknown

    Azerbaijan (68 digital images)

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    Photographs within the folder were taken during Pamela B. Cohen's travels in the U.S.S.R. and during various events related to the American Soviet Jewry Movement.Digital ImageDigital finding aid
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