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Large scale structure of the solar corona in the declining phase of the solar cycle

โœ Scribed by P. Lantos; C. E. Alissandrakis


Publisher
Springer Netherlands
Year
1995
Tongue
English
Weight
262 KB
Volume
72
Category
Article
ISSN
0038-6308

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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: