Cycle variation of Coronal Bright Points (CBPs) number from EIT/SOHO data

Temporal variations of coronal bright points number in EIT/SoHO data from 195 pass band for 1996−2008 are studied. For identification of CBPs the method developed by authors is used. It is found that: cycle variation of CBPs number is complete by July 2008; cycle variations of CBPs number are different at different latitudes.

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