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File:SH SunspotNumbers.png

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Summary

Description Numbers of sunspots since 1610.[1][2] Several periodic cycles are evident, most notably the 11 year (131 ± 14 month) cycle. The green line represents continuous monthly averages reported by the Solar Influences Data Center since 1749. The red data points represent sporadic observations since 1610.
  1. Hoyt, D.V.; K.H. Schatten (1998). "Group sunspot numbers: A new solar activity reconstruction. Part 1". Solar Physics 179: 189-219. 
  2. Hoyt, D.V.; K.H. Schatten (1998). "Group sunspot numbers: A new solar activity reconstruction. Part 2". Solar Physics 181: 491-512. 
Source

Wikimedia Commons (wikimedia.org)

Date

2008-08-01

Author

User:Slashme

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Date/TimeThumbnailDimensionsUserComment
current18:29, 22 September 2011Thumbnail for version as of 18:29, 22 September 20111,000 × 606 (55 KB)Imhezok (talk | contribs){{Information |Description= Numbers of sunspots since 1610.<ref name='Hoyt-Schatten_a'> {{cite journal|title=Group sunspot numbers: A new solar activity reconstruction. Part 1|journal=Solar Physics|date=1998|first=D.V.|last=Hoyt|coauthors=K.H. Schatten|vo

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