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adsabs.harvard.edu/full/1968SoPh....4...58K
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A strong S-component of solar radiation was identified during the total solar .... Figure 6 shows the reduced spectra for the radio plage studied in this paper.
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adsabs.harvard.edu/full/1969PASAu...1..192C
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These localized sources, known as radio plage regions, take part in the general solar rotation. Because of an electron density gradient within each source they ...
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www.publish.csiro.au/?act=view_file&file_id=PH570491.pd...
www.publish.csiro.au/?act=view_file&file_id=PH570491.pdf
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These regions are responsible for the slowly varying component ... The radio sources appear always to be associated with plages faculaires and, during ...
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www.publish.csiro.au/?act=view_file&file_id=PH610403.pd...
www.publish.csiro.au/?act=view_file&file_id=PH610403.pdf
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as a guide to the location of the main radio plages. In order to do this it is necessary to separate the quiet-Sun and the slowly varying component in some way.
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www.springerlink.com/index/LW4044787X71L556.pdf
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sufficient for the S-component radio emission (because the contribution of the ' cold' component to radio emission is negligible). For plage regions, however, the ...
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www.springerlink.com/index/h5q3617632343235.pdf
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plages) of solar activity. The results of a comparative study of these components of CI with those of 10.7 cm radio flux are presented and discussed. 2. Data ...
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www.gao.spb.ru/english/publ-s/viii-rfs/p040.pdf
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Firstly, radio emission of slowly varying component is generated ... from Nobeyama maps: a wide source that can be associated with plage emission and a ...
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onlinelibrary.wiley.com/doi/10.1002/asna.2113060312/pdf
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As it is widely accepted, tlie interpretation of tlie S-component radio cinissioii is .... Tlie height z of tlie density peak is quite different for the sunspot, plage, and ...
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www.spaceacademy.net.au/spacelink/solrfi/solrfi.htm
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This note reviews the nature of solar radio emissions and provides appropriate ... This component is due to the uneven longitudinal distribution of plage.
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