On the existence of a low-dimensional chaotic attractor in the short-term solar UV time series

Details On the existence of a low-dimensional chaotic attractor in the short-term solar UV time series On the existence of a low-dimensional chaotic attractor in the short-term solar UV time series

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999soph..186..421c&link_type=abstract

Solar Physics, v. 186, Issue 1/2, p. 421-429 (1999).

Physics

Scientific paper

A mixture of periodic and chaotic components makes the detection of chaos difficult. The periodic components are sought in the solar UV time series by the Maximum Entropy Method and are removed by a digital notch filter. The filtered output is subjected to investigation for chaotic behavior by three different techniques. (1)Fixed-size method for attractor dimension determination; (2)sensitive initial dependence via prediction error; (3)trajectory direction estimation. All the investigation points to the existence of a chaotic attractor of fractional dimension.

Affiliated with

Also associated with

No associations

Rating

On the existence of a low-dimensional chaotic attractor in the short-term solar UV time series 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 On the existence of a low-dimensional chaotic attractor in the short-term solar UV time series, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the existence of a low-dimensional chaotic attractor in the short-term solar UV time series will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1194128