Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • 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.

    Advertised on:

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

    Advertised on:

    0
    1976
    Citations
    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.

    Advertised on:

    9
    1975
    Citations
    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.

    Advertised on:

    7
    1975
    Citations
    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.

    Advertised on:

    3
    1975
    Citations
    18