Tipo de publicación: Sin árbitro

  • Publicación
    Magnetic field structures associated with chromospheric heating in a plage region
    The strongest quasi-steady heating in the solar atmosphere occurs in the active chromosphere and in particular within plage regions. Our aim is to investigate...
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    Magnetic fields and the outer rotation curve of M31
    Not Available
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    Magnetic Fields in Cool Stars (CD-ROM Directory: contribs/moreno)
    Not Available
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    Magnetic fields in Galaxies
    Magnetic fields not only provide a basic tool for observing galaxies but constitute an important clue to interpret many dynamic processes taking place in them...
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    Magnetic Fields of the Quiet Sun: A New Quantitative Perspective From Hinode
    This article summarizes results of studies presented in two papers already published: Lites et al. (2007a); Lites et al. (2007b). Please see these for further...
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    Magnetic Fields of the Quiet Sun: Distribution of Field Strengths
    The quiet Sun photospheric plasma has a variety of magnetic field strengths going from zero to 1800 G. The empirical characterization of these field strengths...
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    Magnetic Fingerprints of Solar and Stellar Oscillations
    Waves connect all the layers of the Sun, from its interior to the upper atmosphere. It is becoming clear now the important role of magnetic field on the wave...
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    Magnetic Flux Emergence and its Interaction with AN Existing Coronal Field
    Not Available
  • Publicación
    Magnetic Flux Emergence and its Interaction with AN Existing Coronal Field
    Not Available