๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

On theRz-sunspot relative number variations

โœ Scribed by M. R. Attolini; M. Galli; G. Cini Castagnoli


Publisher
Springer
Year
1985
Tongue
English
Weight
243 KB
Volume
95
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

โœฆ Synopsis


The Zfirich sunspot relative number R z series has been analysed by the cyclogram method. The amplitude and the frequency variations of the Fourier 11 yr component between 1700-1983 A.D., were determined in a continuous way.

Four distinct time intervals with significantly different characteristics of the periodicities are observed and discussed.

Their second harmonics are also considered. The periodicity changes are contemporary to those of the 11 yr cycles.

Around the year 1903 it seems that an important event has happened in the Sun. In fact the 11.4 yr cycle periodicity, that was very stable since at least 1825 started to change gradually to smaller values and similarly it happened to the second harmonic which also stopped and abruptly changed of phase of 90~


๐Ÿ“œ SIMILAR VOLUMES


On forecasting the sunspot numbers
โœ J. Kurths; A. A. Ruzmaikin ๐Ÿ“‚ Article ๐Ÿ“… 1990 ๐Ÿ› Springer ๐ŸŒ English โš– 199 KB
Can variations of sunspot number be rela
โœ Y. V. Vandakurov ๐Ÿ“‚ Article ๐Ÿ“… 1991 ๐Ÿ› Springer ๐ŸŒ English โš– 397 KB

We consider a hypothesis that nondissipating wave-bound beam structures may be created in plasma due to interaction between energetic charged particles and undamped waves. This hypothesis, if correct, might account for several phenomena observed in the Sun. For instance, on entering the atmosphere