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

  • High resolution atmospheric emission spectroscopy at 120/cm and 535/cm, with a rapid scan interferometer and 91 cm airborne telescope
    Not Available
    Anderegg, M. et al.

    Fecha de publicación:

    0
    1976
    Número de citas
    0
  • Atmospheric spectroscopy at very high resolution in the middle infrared with a rapid-scan Michelson interferometer.
    Not Available
    Anderegg, M. et al.

    Fecha de publicación:

    0
    1976
    Número de citas
    0
  • Jovian system science issues and implications for a Mariner Jupiter Orbiter mission
    Science goals for missions to Jupiter in the early 1980's are reviewed and a case is made for the science community to play the key role in assigning relative priorities for these goals. A reference set of measurement requirements and their priorities is established and those high priority goals that are most demanding on spacecraft and mission
    Beckman, J. C. et al.

    Fecha de publicación:

    9
    1975
    Número de citas
    0
  • Differential rotation and the SPOT zones
    Doppler measurements, using the Capri magnetograph, of the latitudinal fine structure of the solar differential rotation have been carried out. The positions of the photospheric lines C I 5380.32 and Fe I 5364.88 have been simultaneously recorded. In contrast to Gilman's model (1972) which predicted an equatorial deceleration of the differential
    Deubner, F.-L. et al.

    Fecha de publicación:

    7
    1975
    Número de citas
    20
  • Submillimeter brightness spike at the solar limb
    Submillimeter observations made with a rapid-scanning interferometer during the solar eclipse of June 30, 1973 are reported. Reduction, correction, and plotting of the data is described, and the obtained results show that the spike can be identified with emission from chromospheric spicules. Models of spicules from optical wavelength data indicate
    Beckman, J. E. et al.

    Fecha de publicación:

    3
    1975
    Número de citas
    18