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How Deep Was the Maunder Minimum?

  • Sunspot Number Recalibration
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Abstract

One of the most enigmatic features of the solar history is the Maunder minimum (MM). We analyze reports of solar observers from the group-sunspot-number database. Particular attention is given to short notes that resulted in an underestimation of the sunspot activity. These reports by Derham, Flamsteed, Hevelius, Picard, G.D. Cassini, and Fogel are found to address the absence of sunspots of great significance, which could signify a secular minimum with a majority of small short-lived spots. Up to Schwabe’s discovery of the solar cycle, sunspots were considered as an irregular phenomenon; sunspot observations were not dedicated to the task of sunspot monitoring and counting. Here, we argue that the level of the solar activity in the past is significantly underestimated.

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Notes

  1. Concerning the Crabtree letters, we did not find his letter to Flamsteed, but in the letter to Gascoigne (Derham, 1710), he wrote that Gassendi affirms that sometimes 40 spots at once are seen on the Sun. Because observers of the seventeenth century did not count sunspots as groups, four to five objects per day in 1638 – 1639 can mean umbras or spots, not groups.

  2. We note that each drawing in a frame covers the entire time interval, 12 – 26 July, 9 – 22 August, or 2 – 24 September.

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Acknowledgments

We use data from the Royal Greenwich Observatory, United States Air Force, National Aeronautics and Space Administration (RGO/USAF/NOAA: solarscience.msfc.nasa.gov/greenwch.shtml ), the revised version of Greenwich Photoheliographic Results (GPR) sunspot catalogue provided by the Debrecen Heliophysical Observatory (DHO: fenyi.solarobs.unideb.hu/deb_obs_en.html ), regular solar observations at the Kislovodsk Mountain Astronomical Station GAS GAO ( en.solarstation.ru ), the database by Hoyt and Schatten (1998) provided by the National Geophysical Data Center (NOAA/NGDS: ngdc.noaa.gov/stp/SOLAR ), and the average group number provided by Svalgaard and Schatten (2016).

The reported study was funded by RFBR according to the research projects No. 15-02-06959-a and No. 16-02-00300-a.

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Sunspot Number Recalibration

Guest Editors: F. Clette, E.W. Cliver, L. Lefèvre, J.M. Vaquero, and L. Svalgaard

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Zolotova, N.V., Ponyavin, D.I. How Deep Was the Maunder Minimum?. Sol Phys 291, 2869–2890 (2016). https://doi.org/10.1007/s11207-016-0908-z

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  • DOI: https://doi.org/10.1007/s11207-016-0908-z

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