Tipo de publicación: Sin árbitro

  • Publicación
    The M(17)SW molecular source - Internally or externally heated?
    From a measurement of the J = 3 - 2 rotational emission line of hydrogen isocyanide, and a literature value for that J = 1 - 0 line (Snell, 1979), the...
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    The Magellanic Clouds Chemical Enrichment History via Ca II Triplet Spectroscopy
    Not Available
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    The Magellanic Clouds Field Population Chemical Enrichment History
    We report the results of our project devoted to study the chemical enrichment history of the field population in the Magellanic Clouds using Ca 0 triplet...
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    The MAGIC Telescope and the Observation of Gamma Ray Bursts
    The MAGIC telescope, with many technological innovations which allow the telescope to have a low energy threshold and a very fast slewing time, could be one of...
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    The MAGIC telescope for gamma-ray astronomy above 30 GeV
    The MAGIC telescope, presently at its commissioning phase, will become fully operative by the end of 2003. Placed at the Roque de los Muchachos Observatory (ORM...
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    The Magnetic Configuration in Light Bridges
    Not Available
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    The magnetic field in the convection zone as a link between the active regions on the surface and the field in the solar interior
    Recent developments in the theory of the rise of magnetic flux from the bottom of the convection zone to the surface to produce active regions are reviewed...
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    The Magnetic Field of Solar Chromospheric Spicules
    A suitable diagnostic tool for investigating the magnetism of the solar chromosphere is the observation and theoretical modeling of the Hanle and Zeeman effects...
  • Publicación
    The Magnetic Field of Solar Spicules
    Determining the magnetic field of solar spicules is vital for developing adequate models of these plasma jets, which are thought to play a key role in the...