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Some features of relative sunspot number during the declining phase of solar cycle 19

โœ Scribed by B. N. Bhargava


Publisher
Springer
Year
1968
Tongue
English
Weight
153 KB
Volume
3
Category
Article
ISSN
0038-0938

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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: