A 3,000-Year Record of Solar Activity Reference
Usoskin, I.G., Hulot, G., Gallet, Y., Roth, R., Licht, A., Joos, F., Kovaltsov, G.A., Thebault, E. and Khokhlov, A. 2014. Evidence for distinct modes of solar activity. Astronomy and Astrophysics 562: L10, doi: 10.1051/0004-6361/201423391.
What was done
According to Usoskin et al. (2014), the Sun "shows strong variability in its magnetic activity, from Grand minima to Grand maxima, but the nature of the variability is not fully understood, mostly because of the insufficient length of the directly observed solar activity records and of uncertainties related to long-term reconstructions." Now, however, in an attempt to overcome such uncertainties, in a Letter to the Editor published in the journal Astronomy and Astrophysics, Usoskin et al. "present the first fully adjustment-free physical reconstruction of solar activity" covering the past 3,000 years, which record allowed them "to study different modes of solar activity at an unprecedented level of detail."
What was learned
As illustrated in the figure below, the authors report there is "remarkable agreement" among the overlapping years of their reconstruction (solid black line) and the number of sunspots recorded from direct observations since 1610 (red line). Their reconstruction of solar activity also displays several "distinct features," including several "well-defined Grand minima of solar activity, ca. 770 BC, 350 BC, 680 AD, 1050 AD, 1310 AD, 1470 AD, and 1680 AD," as well as "the modern Grand maximum (which occurred during solar cycles 19-23, i.e., 1950-2009)," which they describe as "a rare or even unique event, in both magnitude and duration, in the past three millennia."
http://www.co2science.org/articles/V17/N32/C1.php
