Estimating the size and timing of maximum amplitude for cycle 23 from its early cycle behavior

Journal of Geophysical Research: Space Physics

Volumn 103, Issue A8, 1998, Pages 17411-17418

  Wilson, Robert M ^a  

^a NASA MARSHALL SPACE FLIGHT CENTER   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0013192169     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article

References (9)

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3. Hathaway, D. H., R. M. Wilson, and E. J. Reichmann, The shape of the sunspot cycle, Sol. Phys., 151, 177-190, 1994.
4. Howard, R., Solar cycle, solar rotation, and large-scale circulation, in Illustrated Glossary for Solar and Solar-Terrestrial Physics, edited by A. Bruzek and C. J. Durrant, pp. 7-12, D. Reidel, Norwell, Mass., 1977.
5. Joselyn, J, A., J. B. Anderson, H. C. Coffey, K. Harvey, D. Hathaway, G. Heckman, E. Hildner, W. Mende, K. Schatten, R. Thompson, A. W. P. Thomson, and O. R. White, Panel achieves consensus prediction of solar cycle 23, Eos, Trans. AGU, 78, 205, 211-212, 1997.
6. Kane, R. P., A preliminary estimate of the size of the coming solar cycle 23, based on Ohl's precursor method, Geophys. Res. Lett., 24, 1899-1902, 1997.
7. Kopecky, M., Forecast of the maximum of the next 11-year cycle of sunspots no. 23, Bull. Astron. Inst. Czech., 42, 157-158, 1991.
8. Rabin, D., R. M. Wilson, and R. L. Moore, Bimodality of the solar cycle, Geophys. Res. Lett., 13, 352-354, 1986.
9. Waldmeier, M., Neue Eigenschaften der Sonnenfleckenkurve, Astron. Mitt. Zurich, 74(133), 105-130, 1935.