Title of article
Coronal manifestations of solar variability Original Research Article
Author/Authors
J. S?kora، نويسنده , , Michael J. Rybak، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2005
Pages
7
From page
393
To page
399
Abstract
This contribution is mostly about phenomenology of what we see in space–time evolution of coronal green line brightness (CGLB), including its cyclic variations. Our own database (1943–2001) of the coronal Fe XIV 530.3 nm emission line intensities is used to display different aspects of the large-scale CGLB regularities and cyclic behaviour. Hemispheric asymmetry and relation of the longitudinal CGLB distribution to the rotational characteristics of the solar corona are particularly underlined.
Keywords
Solar emission green-line corona , N-S asymmetry , Solar 11-year cycle , Active longitudes , Coronal rotation
Journal title
Advances in Space Research
Serial Year
2005
Journal title
Advances in Space Research
Record number
1130019
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