Rescaled Range Analysis of the Asymmetry of Solar Activity

Details Rescaled Range Analysis of the Asymmetry of Solar Activity Rescaled Range Analysis of the Asymmetry of Solar Activity

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..169..215o&link_type=abstract

Solar Physics, Volume 169, Issue 1, pp.215-224

Physics

15

Scientific paper

Previous studies of the north-south asymmetry of solar activity (e.g., Carbonell, Oliver, and Ballester, 1993; Oliver and Ballester, 1994) suggest that the asymmetry time series can be represented by means of a multicomponent model made up of a long-term trend, a weak sinusoidal component (with a period close to 12.1 years) and a dominant random process. Here, we have used the rescaled range analysis to study the valuation of the stochastic component of the asymmetry. To avoid the influence of the trend and the sinusoidal component on the result, we have removed both from the original time series. The value obtained for the Hurst exponent (0.717 ± 0.002) suggests that the non-periodic component is a correlated random process.

Affiliated with

Also associated with

No associations

Rating

Rescaled Range Analysis of the Asymmetry of Solar 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 Rescaled Range Analysis of the Asymmetry of Solar Activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rescaled Range Analysis of the Asymmetry of Solar Activity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1752770