Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • An Investigation into the Radiation Damage of the Silicon Detectors of the H1-PLUG Calorimeter within the HERA environment
    The silicon detectors used in the H1-PLUG calorimeter have shown increasing aging effects during the '94 run period of the electron proton storage ring HERA. These effects were particularly manifest as degradation of the signal to noise level and the calibration stability. The reasons for this behaviour have been found to be correlated with
    Hildesheim, W. et al.

    Fecha de publicación:

    7
    1995
    Número de citas
    0
  • UNIFIED MODELS FOR THE ANALYSIS OF MASSIVE HOT STARS ATMOSPHERES
    SE HA DESARROLLADO UN NUEVO CODIGO DE ORDENADOR PARA MODELIZAR LA FORMACION DE LINEAS ESPECTRALES EN ATMOSFERAS ESTELARES EN EXPANSION ESFERICA. LA MEMORIA DE LA TESIS DESCRIBE EL FUNDAMENTO TEORICO, LOS METODOS NUMERICOS Y LOS PRIMEROS RESULTADOS. LAS TECNICAS NUMERICAS SON MUY EFICIENTES Y EL CODIGO HA DISEÑADO DE FORMA TAL QUE PERMITE FACILMENTE
    ANTONIO ENRIQUE SANTOLAYA REY

    Fecha de publicación:

    6
    1995
  • The Possible Ascent of a Closed Magnetic System through the Photosphere
    We present a comprehensive interpretation of the evolution of a small magnetic region observed during its entire disk passage. The vector magnetic field measurements from the Advanced Stokes Polarimeter, along with Hα and magnetogram measurements from the Lockheed SOUP instrument operating at the Swedish Solar Observatory on La Palma, and soft X
    Lites, B. W. et al.

    Fecha de publicación:

    6
    1995
    Número de citas
    230
  • The evolution of compact supernova remnants in a strongly magnetized medium
    Two-dimensional simulations of the evolution of supernova remnants in a uniform, high-density medium are presented. The medium is magnetized, and its magnetic pressure is much larger than the thermal pressure. The evolution of the remnants is followed past full thermalization of the ejecta. A mechanism of self-collimation of the flow is identified
    Rozyczka, Michal et al.

    Fecha de publicación:

    6
    1995
    Número de citas
    7