The autocorrelation method is applied to the observed va- riation of the solar diam eter.
The results substantially agree with those obtained by M. Cimino. The period of th e variation is around 23 years, bu t this is not a period in a stric t sense. The phase shift betw een th e variations in diam eter and th e va riation in sunspot num bers is confirmed
| Primary Language | English |
|---|---|
| Subjects | Mathematical Sciences |
| Journal Section | Research Article |
| Authors | |
| Submission Date | January 1, 1956 |
| Publication Date | January 1, 1956 |
| DOI | https://doi.org/10.1501/Commua1_0000000140 |
| IZ | https://izlik.org/JA44TJ53WB |
| Published in Issue | Year 1956 Volume: 08 |
Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics
This work is licensed under a Creative Commons Attribution 4.0 International License.