Bayesian Methods for Reconstructing Sunspot Numbers Before and During the Maunder Minimum
The Maunder Minimum (MM) was an extended period of reduced solar activity in terms of yearly sunspot numbers (SSN) during 1610 – 1715. The reality of this “grand minimum” is generally accepted in the scientific community, but the statistics of the SSN record suggest a need for data reconstruction. T...
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Veröffentlicht in: | Solar physics 2017, Vol.292 (1), p.1, Article 23 |
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