Cyclic distribution of energetic X-ray flares.

Details Cyclic distribution of energetic X-ray flares. Cyclic distribution of energetic X-ray flares.

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..107..195l&link_type=abstract

Solar Physics, Volume 107, Issue 1, pp.195-199

Physics

3

Solar Activity Cycles:Solar X-Ray Flares, Solar X-Ray Flares:Solar Activity Cycles

Scientific paper

The Blackman-Tukey power spectrum of flare generated X-ray bursts ≥X1 observed from 1970 to 1982 by satellite instrumentation (SOLRAD/SMS/GOES) shows prominent peaks at 156, 4.8, 2.8, and 1.1 months. According to a statistical test of the significance of the deviation of these peaks from Markov red noise, the peaks at 2.8 and 1.1 months are significant at the 99% confidence level while the peak at 4.8 months reaches the 95% level. A replication by means of the maximum entropy spectral analysis (MEM) yields the same prominent peaks at the same frequencies.

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