Coronal Bright Points at the Minimum of Sunspot Activity

Details Coronal Bright Points at the Minimum of Sunspot Activity Coronal Bright Points at the Minimum of Sunspot Activity

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp22a..02p&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SP22A-02

Physics

7509 Corona, 7524 Magnetic Fields

Scientific paper

We will present the results of our study of coronal bright points (XBPs) using SoHO/EIT data and an automatic identification procedure. The latitude-longitude distribution of XBPs obtained during the period of very low sunspot activity (March-April 1996) is not uniform; it exhibits structures reminiscent of active longitudes and large-scale circular patterns. We also find XBPs associated with emergence of ephemeral active regions. We interpret these results as a possible indication of two types of XBPs that are characteristic of quiet and active Sun.

Affiliated with

Also associated with

No associations

Rating

Coronal Bright Points at the Minimum of Sunspot Activity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Coronal Bright Points at the Minimum of Sunspot Activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Coronal Bright Points at the Minimum of Sunspot Activity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1697663