Simulations of the gross solar magnetic field during sunspot cycle 21

Solar Physics

Volumn 106, Issue 2, 1986, Pages 251-268

  Sheeley Jr , Neil R ^a   Devore, C Richard ^a   Shampine, Lauree R ^a  

^a NAVAL RESEARCH LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0007224769     PISSN: 00380938     EISSN: 1573093X     Source Type: Journal    
DOI: 10.1007/BF00158496     Document Type: Article

References (27)

1. Stellar Activity Cycles
2. Twenty-seven day recurrences in terrestrial-magnetic and solar activity, 1923–1933
3. Variability of the solar flux in the far ultraviolet 1175–2100 Å
4. Temporal characteristics of the solar UV flux and He I line at 1083 nm
5. Large-scale patterns formed by solar active regions during the ascending phase of cycle 21
6. Rotation of the sun measured from Mount Wilson white-light images
7. Observations of Solar Magnetic Fields in Plage Regions.
8. Transport of Magnetic Fields on the Sun.
9. The Sun's Rotation Derived from Sunspots 1934-1944 and Additional Results
10. The influence of differential rotation on the equatorial component of the sun's magnetic dipole field
11. The sun as a star - Three-component analysis of chromospheric variability in the calcium K line
12. Magnetic rotation of the solar photosphere
13. Solar luminosity variation. III - Calcium K variation from solar minimum to maximum in cycle 21
14. Chromospheric variations in main-sequence stars