Active Longitudes in Distribution of EIT Bright Points

Details Active Longitudes in Distribution of EIT Bright Points Active Longitudes in Distribution of EIT Bright Points

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..346..395s&link_type=abstract

Large-scale Structures and their Role in Solar Activity ASP Conference Series, Vol. 346, Proceedings of the Conference held 18-2

Physics

3

Scientific paper

Using a previously developed automatic procedure for identifying coronal bright points (BPs) in EIT/Fe XII 195 Å data, we study longitudinal and latitudinal distributions of EUV BPs on solar surface near the minimum of the solar activity cycle in 1996. Longitudinal distributions indicate the presence of active longitudes in coronal BPs. Latitudinal distributions are asymmetric relative to the equator and show secondary peaks associated with areas of emerging flux. We find this result as suggestive of two types of coronal BPs: quiet Sun and active Sun BPs.

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