/ftp/cats/A+A/491/561


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J/A+A/491/561       Plasma filling factor of coronal bright points (Dere+, 2008)
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	table2.dat
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J/A+A/491/561       Plasma filling factor of coronal bright points (Dere+, 2008)
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The plasma filling factor of coronal bright points. Coronal bright points.
    Dere K.P.
   <Astron. Astrophys. 491, 561 (2008)>
   =2008A&A...491..561D
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ADC_Keywords: Sun
Keywords: Sun: corona

Abstract:
    We determine the volumetric plasma filling factor of coronal bright
    points.

    Rastered spectra of the regions of the quiet Sun were recorded by the
    Extreme ultraviolet Imaging Spectrometer (EIS) during operations with
    the Hinode satellite. Calibrated intensities of Fe XII lines were
    obtained and images of the quiet corona were constructed. From the
    imaged spectra, the emission measures and geometrical widths of
    coronal bright points were obtained. Electron densities were
    determined from density-sensitive line ratios. A comparison of the
    emission measure and bright point widths with the electron densities
    yielded the plasma-filling factor.

Description:
    The data describe the observed and derived properties of a set of
    corona l bright points. The labeling allows the reader to correlate
    the data in Table 2 with their images in Figures 2 and 3.
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