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| | Great Moments in Solar Physics 2 |
 | | This period is now known as the Maunder minimum, after the solar astronomer E.W. Maunder, who, following the pioneering historical investigations of Gustav Spörer (1822-1895), was most active and steadfast in investigating the dearth of sunspot sightings by astronomers active in the second half of the seventeenth century. |
 | | First, the latitude at which sunspots are most often seen decreases systematically from about 40° to 5° latitude as the sunspot cycle proceeds from one minimum to the next (see diagram below). |
 | | Ribes, J. C., and Nesme-Ribes, E. 1993, The solar sunspot cycle in the Maunder minimum AD1645 to AD1715, Astronomy and Astrophysics, 276, 549-563. |
| www.hao.ucar.edu /public/education/sp/great_moments.2.html (270 words) |
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