The north-south asymmetry of filaments in solar cycles 16-21

Details The north-south asymmetry of filaments in solar cycles 16-21 The north-south asymmetry of filaments in solar cycles 16-21

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010newa...15..346l&link_type=abstract

New Astronomy, Volume 15, Issue 4, p. 346-350.

Astronomy and Astrophysics

Astronomy

6

Scientific paper

In the present study, the north-south asymmetry of filaments in solar cycles 16-21 is investigated with the use of the solar filaments observed at the Observatoire de Paris, Section de Meudon from March 1919 to December 1989. Filament activity is found regularly dominated in each of cycles 16-21 in the same hemisphere as that inferred by sunspot activity, and it is found to run in a different asymmetrical behavior at different latitudinal bands, suggesting that the north-south asymmetry of filament activity should be a function of latitudes. The regularity on the north-south asymmetry of sunspot activity given by Li et al. (2002b) is demonstrated by filament activity. The periods in the north-south asymmetry of solar filament activity are 9.13, and 12.8 years without the solar cycle found.

Affiliated with

Also associated with

No associations

Rating

The north-south asymmetry of filaments in solar cycles 16-21 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 The north-south asymmetry of filaments in solar cycles 16-21, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The north-south asymmetry of filaments in solar cycles 16-21 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1189213