The method proposed by Hathaway et al. [SoPh 151 (1994) 177] was employed to predict the magnitude of sunspot activities in the declining phase of solar Cycle 23, based on the monthly averages of sunspot number and the smoothed monthly averages of sunspot number, respectively. Our results show that:
โฆ LIBER โฆ
Prediction of the height of solar cycle 23
โ Scribed by V. Letfus
- Publisher
- Springer
- Year
- 1994
- Tongue
- English
- Weight
- 332 KB
- Volume
- 149
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Prediction of sunspot numbers in the dec
โ
Lasheng Zhan; Haijuan Zhao; Hongfei Liang
๐
Article
๐
2003
๐
Elsevier Science
๐
English
โ 129 KB
A prediction of solar activities in the
โ
Jia-long Wang
๐
Article
๐
1993
๐
Elsevier Science
๐
English
โ 52 KB
Some comments on the problem of solar cy
โ
V. N. Obridko
๐
Article
๐
1995
๐
Springer
๐
English
โ 635 KB
Prediction of wave height based on half-
โ
Michel K. Ochi; Michael A. Eckhoff
๐
Article
๐
1984
๐
Elsevier Science
๐
English
โ 533 KB
A technique for predicting the amplitude
โ
R. J. Thompson
๐
Article
๐
1993
๐
Springer
๐
English
โ 292 KB
Latitude and solar-cycle dependence of t
โ
W. Graf; R. N. Bracewell
๐
Article
๐
1973
๐
Springer
๐
English
โ 602 KB
The apparent height of radio sources above the photosphere was determined for the period of 1968-1971, by a method which makes use of the displacement in latitude of the centroid of the radio emission relative to the associated optical feature. The apparent height fell progressively in time by amou