## Abstract Duration of the extended solar cycles is taken into the consideration. The beginning of cycles is counted from the moment of polarity reversal of largeβscale magnetic field in high latitudes, occurring in the sunspot cycle n till the minimum of the cycle __n__ + 2. The connection betwee
A technique for predicting the amplitude of the solar cycle
β Scribed by R. J. Thompson
- Publisher
- Springer
- Year
- 1993
- Tongue
- English
- Weight
- 292 KB
- Volume
- 148
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Examined are associational aspects as they relate the maximum amplitude R M for the sunspot cycle to the rate of rise Ral during the ascending phase, where R M is the smoothed sunspot number at cycle maximum and Rat is the sum of the monthly mean sunspot numbers for selected 6-month intervals (At) m
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.