It is shown from the statistical analysis of the sunspot data and solar neutrino data that both the data exhibits 5, 10, 15, 20, 25, and 30 months period and these periods may be g-mode oscillation of the core associated with the solar activity,
On the short term variations of solar activity during solar cycle 21
✍ Scribed by Tamer Ataç
- Publisher
- Springer Netherlands
- Year
- 1989
- Tongue
- English
- Weight
- 323 KB
- Volume
- 47
- Category
- Article
- ISSN
- 1573-0794
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✦ Synopsis
Short-term variations ot the last solar activity cycle were studied by the flare and coronal indices using Gleissberg method. Systematic short-term variations are found from their course during the 21st solar activity cycle. Comparison of their autocorrelograms constructed by the new set of data obtained from the magnitude of the fluctuations showed us the existence of the phase shift between the temporal variations of the two indices.
📜 SIMILAR VOLUMES
The present paper investigates the north-south asymmetry for major flares (solar cycles 19 and 20), type II radio bursts (solar cycles 19,20 and 21), white light flares (solar cycle 19,20 and 21), and gan~na ray bursts, hard X-ray bursts and coronal mass ejections (solar cycle 21). The results are
Predicted values of some main indices of solar activity for the 21st solar cycle are given. The epoch of maximum of solar activity has been placed in 1980.8 + 0.1. The predicted peak values of the relative sunspot numbers published by other authors are also given.