Computer Science
Scientific paper
Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ssrv..133..103w&link_type=abstract
Space Science Reviews, Volume 133, Issue 1-4, pp. 103-179
Computer Science
15
Solar Vuv&Mdash, Observations And Interpretations, Solar Atmosphere, Solar Plasma Processes And Parameters
Scientific paper
In Part I of this review, the concepts of solar vacuum-ultraviolet (VUV) observations were outlined together with a discussion of the space instrumentation used for the investigations. A section on spectroradiometry provided some quantitative results on the solar VUV radiation without considering any details of the solar phenomena leading to the radiation. Here, in Part II, we present solar VUV observations over the last decades and their interpretations in terms of the plasma processes and the parameters of the solar atmosphere, with emphasis on the spatial and thermal structures of the chromosphere, transition region and corona of the quiet Sun. In addition, observations of active regions, solar flares and prominences are included as well as of small-scale events. Special sections are devoted to the elemental composition of the solar atmosphere and theoretical considerations on the heating of the corona and the generation of the solar wind.
Dwivedi Bhola N.
Feldman Uri
Marsch Eckart
Wilhelm Klaus
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