Tipo de publicación: Sin árbitro

  • Publicación
    Atmospheric monitoring and model applications at the Pierre Auger Observatory
    The Pierre Auger Observatory detects high-energy cosmic rays with energies above ˜1017 eV. It is built as a multi-hybrid detector measuring extensive air...
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    Atmospheric Monitoring at the Site of the MAGIC Telescopes
    The MAGIC telescopes in La Palma, Canary Islands, measure the Cherenkov light emitted by gamma ray-induced extended air showers in the atmosphere. The good...
  • Publicación
    Atmospheric Monitoring at the Site of the MAGIC Telescopes
    The MAGIC telescopes in La Palma, Canary Islands, measure the Cherenkov light emitted by gamma ray-induced extended air showers in the atmosphere. The good...
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    Atmospheric parameters of stars for UV models (Koleva+, 2012)
    The spectral predictions of stellar population models are not as accurate in the ultra-violet (UV) as in the optical wavelength domain. One of the reasons is...
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    Atmospheric spectroscopy at very high resolution in the middle infrared with a rapid-scan Michelson interferometer.
    Not Available
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    Atmospheric turbulence profiling at the Teide Observatory: comparison and calibration of SODAR and SCIDAR measurements
    In order to characterized the vertical atmospheric structure at the Teide Observatory (Tenerife, Spain), we are using two different remote sensing technics...
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    Atmospherical wavefront phases using the plenoptic sensor (real data)
    Plenoptic cameras have been developed the last years as a passive method for 3d scanning, allowing focal stack capture from a single shot. But data recorded by...
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    Atomic Hydrogen Gas Kinematics in NGC 3359
    We present the kinematical analysis of HI and HII gases within the disk of NGC 3359. There is a strong trend of non-circular gas flow as seen in the velocity...
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    Atomic orientation in chromospheric lines.
    Observations of the Stokes I and V profiles of the Ca II H and K lines in solar magnetic regions are presented. Least-squares fits of dI/dλ to V are obtained...