Panel achieves consensus prediction of solar cycle 23

Eos

Volumn 78, Issue 20, 1997, Pages 205-212

  Joselyn, Jo Ann ^a   Anderson, Jeffrey B ^b   Coffey, Helen ^b   Harvey, Karen ^b   Hathaway, David ^b   Heckman, Gary ^b   Hildner, Ernie ^b   Mende, Werner ^b   Schatten, Kenneth ^b   Thompson, Richard ^b   Thomson, A W P ^b   White, Oran R ^b  

^a NOAA EARTH SYSTEM RESEARCH LABORATORY   (United States)

^b NONE

Author keywords

[No Author keywords available]

Indexed keywords

EID: 8344280853     PISSN: 00963941     EISSN: None     Source Type: Journal    
DOI: 10.1029/97eo00136     Document Type: Article

References (8)

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4. Mayaud, P. N., Derivation, Meaning, and Use of Geomagnetic Indices, Geophys. Monogr. Ser., vol. 22, pp. 82-84, AGU, Washington, D.C., 1980.
5. Menvielle, M., and A. Berthelier, The K-derived planetary indices: Description and availability, Rev. Geophys., 29, 415-432, 1991.
6. Schatten, K. H., and W. D. Pesnell, An early solar dynamo prediction: Cycle 23 - Cycle 22, Geophys. Res. Lett., 20, 2275-2278, 1993.
7. Thompson , R. J., A technique for predicting the amplitude of the solar cycle, Solar Phys., 148, 383-388, 1993.
8. Wilson, R. M., Predicting the maximum amplitude for the sunspot cycle from the rate of rise in sunspot number, Solar Phys., 117, 179-186, 1988.