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| Description |
Sunspot Numbers.svg
English: 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.
- ↑ Hoyt, D.V.; K.H. Schatten (1998). "Group sunspot numbers: A new solar activity reconstruction. Part 1". Solar Physics 179: 189-219. Retrieved on 2008-07-31.
- ↑ Hoyt, D.V.; K.H. Schatten (1998). "Group sunspot numbers: A new solar activity reconstruction. Part 2". Solar Physics 181: 491-512. Retrieved on 2008-07-31.
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| Date |
1 August 2008(2008-08-01)
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| Source |
Self-made using gnuplot.
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| Author |
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Permission
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Image:Sunspot Numbers.png |
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Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.
www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue
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| Date/Time | Thumbnail | Dimensions | User | Comment |
| current | 21:02, 1 August 2008 |  | 660 × 400 (294 KB) | Slashme | |
| 20:46, 1 August 2008 |  | 660 × 400 (299 KB) | Slashme | |
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