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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Space science reviews 87 (1999), S. 141-144 
    ISSN: 1572-9672
    Keywords: plasma diagnostics ; coronal holes ; radio observations
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract An equatorial coronal hole has been observed on 18 and 19 October 1996 with SOHO-CDS and with the Nancąy Radioheliograph (RH). The CDS EUV line intensities are used to determine the coronal hole Differential Emission Measure (DEM); in turn this is used to compute the radio brightness temperature Tb at the observed frequencies, leaving the coronal electron temperature and density as free parameters. EUV line intensities, calculated from the derived models, show a good agreement with EUV observations.
    Type of Medium: Electronic Resource
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