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Prediction of the Amplitude of Sunspot Cycle 23

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Abstract

A few prediction methods have been developed using the ‘precursor’ techniques and are found to be successful. On the basis of geomagnetic activity aa indices during the descending phase of the preceding cycle, we have established an expression which predicts the maximum annual mean sunspot number in cycle 23 to be 166.2. This indicates that cycle 23 would be a highly active and historic cycle. The average geomagnetic activity aa index during the ascending phase of cycle 23 would be about 24.9, comparable to 22.2 and 24.8 in cycles 21 and 22, respectively. This further indicates that during the ascending phase of cycle 23 energetic two-ribbon flares will be produced so as to give rise to strong proton events.

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References

  • Boteler, D. H. and Banks, T: 1990, in R. J. Thompson et al.(eds), Proceedings Solar-Terrestrial Prediction Workshop, Leura, Australia, Vol. 2, p. 25.

    Google Scholar 

  • Brown, G. M.: 1984, in P. A. Simon, G. R. Heckman, and M. A. Shea (eds), Proceedings of the Meudon Solar Terrestrial Predictions Workshop, NOAA, Boulder, Vol. 1, p. 1.

    Google Scholar 

  • Feynman, J.: 1982, J. Geophys. Res. 1987, 6153.

    Google Scholar 

  • Jain, R.: 1987, Monthly Notices Roy. Astron. Soc. 223(4), 877.

    Google Scholar 

  • Jain, R.: 1997, Bull. Astron. Soc. India, submitted.

  • Joselyn, J. A., Anderson, J., Coffey, H., Harvey, K., Hathway, D., Heckman, G., Hildner, E., Mende, W., Schatten, K., Thompson, R., Thompson, A. W. P., and White, O. R.: 1996, ‘Solar Cycle 23 Project: Summary of Panel Findings’, private communication.

  • Kane, R. P.: 1978, Nature 274, 139.

    Google Scholar 

  • Kopecký, M.: 1991, Bull. Astron. Inst. Czech. 42, 157.

    Google Scholar 

  • Kunches, J.: 1993, in J. Hruška et al.(eds), Proceedings of the Ottawa Solar Terrestrial Predictions Workshop, NOAA, Boulder, Vol. 2, p. 198.

    Google Scholar 

  • Legrand, J. P. and Simon, P. A.: 1991, Solar Phys. 131, 187.

    Google Scholar 

  • Mayaud, P. N.: 1973, IAGA Bull. 33.

  • Rangrajan, G. K.: 1977, Proceedings Indian Acad. Sci. (Earth Planetary Sci.) 85, 71.

    Google Scholar 

  • Report UAG-95: 1987, Sunspot Number 1610-1985, World Data Center-A for STP.

  • Rodger, A. S, Hruška, J., Joselyn, J. A., and Marubashi, K.: 1990, in R. J. Thompson et al.(eds), Proceedings Solar-Terrestrial Prediction Workshop, Leura, Australia, Vol. 1, p. 7.

    Google Scholar 

  • Sargent, H. H.: 1978, Trans. Veh. Technol. 28, 490.

    Google Scholar 

  • Schatten, K., Myers, D. J., and Sofia, S.: 1996, Geophys. Res. Letters 23(6), 605.

    Google Scholar 

  • Silverman, S. M.: 1986, J. Geophys. Res. 91, 10157.

    Google Scholar 

  • Simon, P. A. and Legrand, J. P: 1992, Solar Phys. 141, 391.

    Google Scholar 

  • Solar-Geophysical Data Reports: Part I, No. 614.

  • Solar-Geophysical Data Reports: Part II, No. 603.

  • Thompson, R. J.: 1993, Solar Phys. 148, 383.

    Google Scholar 

  • Wilson, P. R.: 1990, in R. J. Thompson et al.(eds.), Proceedings of the Leura Solar Terrestrial

  • Predictions Workshop, NOAA, Boulder, Vol. 1, p. 257.

  • Wilson, R. M.: 1992, Solar Phys. 140, 181.

    Google Scholar 

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Jain, R. Prediction of the Amplitude of Sunspot Cycle 23. Solar Physics 176, 431–437 (1997). https://doi.org/10.1023/A:1004973827442

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