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Cyclic distribution of energetic X-ray flares

โœ Scribed by T. Landscheidt


Publisher
Springer
Year
1986
Tongue
English
Weight
279 KB
Volume
107
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


The Blackman-Tukey power spectrum of flare generated X-ray bursts > X 1 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.


๐Ÿ“œ SIMILAR VOLUMES


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A new series of solar flare energetic X-ray events has been detected by an ionization chamber on the OGO-I and OGO-III satellites in free space. These X-rays lie in the range 10-50 keV, and a study has been made of their relationship to 3 and 10 cm radio bursts and with the emission of electrons and

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