Using Dynamo Theory to predict the sunspot number during Solar Cycle 21

Geophysical Research Letters

Volumn 5, Issue 5, 1978, Pages 411-414

  Schatten, Kenneth H ^a   Scherrer, Philip H ^a   Svalgaard, Leif ^a   Wilcox, John M ^a  

^a NONE

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000359581     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/GL005i005p00411     Document Type: Article

References (20)

1. The topology of the sun's magnetic field and the 22‐year cycle
2. What determines sunspot maximum?
3. Large‐scale solar magnetic fields
4. A magneto‐kinematic model of the solar cycle
5. On the reliability of the Wolf number series for estimating long‐term periodicities
6. Forecast of the maximum Wolf number for the current eleven‐year cycle
7. The origin of solar activity
8. Heliocentric latitude of the dominant polarity of the interplanetary magnetic field
9. Large‐scale properties of the interplanetary magnetic field
10. Polar faculae during the sunspot cycle
11. Measurements of solar magnetic fields
12. Polar faculae during the interval 1906–1975
13. Three‐dimensional structure of the extended solar magnetic field and the sunspot cycle variation in cosmic ray intensity
14. Predicted and observed coronal structure
15. Shape and structure of the corona at the solar eclipse of Oct. 23, 1976