Short periodicities in solar activity
β Scribed by K. Ramanuja Rao
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 261 KB
- Volume
- 29
- Category
- Article
- ISSN
- 0038-0938
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β¦ Synopsis
Several indices of solar activity are subjected to a high pass filter and power spectral analysis to verify the existance of shorter per~di.cit~j..n...solar act iviLy:yhgu~h all these indices show the presence of short periodicities, above 95 ~ confidence level, the common indices like sunspot number, fail to show these periodicities when a stringest statistical test is applied based on a percentage of the Z2/v distribution that is appropriately higher than the 95 % point (Mitchell[ et al., 1966). The basic parameters given by Kopeck3~ (1967), however, reveal the presence of 5.6-and 3.5-yr periodicities even when this stringent statistical test is applied.
OK--K! (q -K)! '
where K is the term number.
π SIMILAR VOLUMES
The presence of intermediate-term periodicities in solar activity, at approximately 323 and 540 days, has been claimed by different authors. In this paper, we have performed a search for them in the historical records of two main indices of solar activity, namely, the daily sunspot areas (cycles 12-