Evolution of magnetic flux distribution of solar bipolar active regions

Details Evolution of magnetic flux distribution of solar bipolar active regions Evolution of magnetic flux distribution of solar bipolar active regions

Jan 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..191..161e&link_type=abstract

Solar Physics, v. 191, Issue 1, p. 161-169 (2000).

Physics

1

Scientific paper

In this paper the magnetic flux distribution of bipolar active regions at the sunspot development stage is analyzed. It is shown that the ratio of the total sunspot area in an active region to the maximum one can be used as a characteristic of the development phase. Such a procedure allows combining the data attributed to different active regions for studying evolutionary changes. The expressions describing the evolution of magnetic flux distribution of bipolar active region were obtained and their interpretation with rise and descent of loop like magnetic flux tube leading to active region formation was justified.

Affiliated with

Also associated with

No associations

Rating

Evolution of magnetic flux distribution of solar bipolar active regions 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 Evolution of magnetic flux distribution of solar bipolar active regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of magnetic flux distribution of solar bipolar active regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-811143