AbstractUsing full disk SOHO/EIT data from 1996 to 2006, we study latitudinal distribution of coronal bright points over a period of one solar cycle. We confirm the presence of two distinct types of coronal bright points, and find that the number of “quiet corona” bright points in high latitudes anticorrelate with solar activity as defined by the sunspot numbers.
On anticorrelation of number of coronal bright points with sunspot number during 1996–2006
Advances in Space Research ; 39 , 11 ; 1777-1780
2007-01-24
4 pages
Article (Journal)
Electronic Resource
English
On anticorrelation of number of coronal bright points with sunspot number during 1996–2006
Online Contents | 2007
|NTIS | 1984
|Lifetimes and distribution of coronal bright points observed with Yohkoh
Elsevier | 1993
|Emission heights of coronal bright points on Fe XII radiance map
Online Contents | 2007
|Emission heights of coronal bright points on Fe XII radiance map
Elsevier | 2007
|