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
Birincil Dil | İngilizce |
---|---|
Konular | Matematik |
Bölüm | Research Article |
Yazarlar | |
Yayımlanma Tarihi | 1 Ocak 1956 |
Gönderilme Tarihi | 1 Ocak 1956 |
Yayımlandığı Sayı | Yıl 1956 Cilt: 08 |
Communications Faculty of Sciences University of Ankara Series A1 Mathematics and Statistics.
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