Abstract
The eleven-year sunspot cycles are considered to represent one of the solar activities. The daily observations of the sunspots in the KAAU Solar Observatory (KAAUSO) have been utilised to reduce a period of the present solar cycle, using Fourier technique. The highest peak in the amplitude spectrum was for a frequency of 0.00029 day−1, for which the maximum occurred mid 1990.
References
Al-Milaky, Y.M.: 1993, to be published inJ. of KAAU Science.
Hill, J.R.: 1977,Nature 266, 151.
Ferraz-Mello, S.: 1981,Astronom. J. 86, 619.
Kane, R.P.: 1992,Solar Phys. 140, 171.
McIntosh, P.S.: 1991,Sky & Telescope, January, 21.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Basurah, H.M., Al-Mleaky, Y.M. & Malawi, A.A. The solar activity maximum of cycle no. 22 from KAAU solar observatory. Astrophys Space Sci 215, 131–133 (1994). https://doi.org/10.1007/BF00627465
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00627465