Physics
Scientific paper
Jun 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.508..295h&link_type=abstract
In: Proceedings of the SOHO 11 Symposium on From Solar Min to Max: Half a Solar Cycle with SOHO, 11-15 March 2002, Davos, Switze
Physics
Sun, Corona, Solar Cycle, Bright Points
Scientific paper
The Extreme ultraviolet Imaging Telescope (EIT) of SoHO incessantly observed small coronal and transition region features: EUV bright points, ephemeral regions, brightenings, network enhancements, loop segments, etc. In this work, the small objects are extracted and characterized automatically in terms of their scale, location, peak and background intensities. We correct for the visibility bias introduced by the expansion of bright regions that develops with the solar cycle, and we plot the resulting instantaneous densities over the 1996-2001 period. The four time-series exhibit dissimilar trends. The 171 Å and 195 Å channels are found to show a moderate anti-cyclic behaviour.
Antoine Jean-Pierre
Clette Frederic
Hochedez Jean-François
Jacques Laurent
Zhukov Alexander A.
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