Solar Physics

, Volume 291, Issue 9–10, pp 2941–2950 | Cite as

An Alternative Measure of Solar Activity from Detailed Sunspot Datasets

Sunspot Number Recalibration

Abstract

The sunspot number is analyzed by using detailed sunspot data, including aspects of observability, sunspot sizes, and proper identification of sunspot groups as discrete entities of solar activity. The tests show that in addition to the subjective factors there are also objective causes of the ambiguities in the series of sunspot numbers. To introduce an alternative solar-activity measure, the physical meaning of the sunspot number has to be reconsidered. It contains two components whose numbers are governed by different physical mechanisms and this is one source of the ambiguity. This article suggests an activity index, which is the amount of emerged magnetic flux. The only long-term proxy measure is the detailed sunspot-area dataset with proper calibration to the magnetic flux. The Debrecen sunspot databases provide an appropriate source for the establishment of the suggested activity index.

Keywords

Sunspots: magnetic fields 

Notes

Acknowledgements

This work has been presented at the Sunspot Number Workshop held in Tucson, Arizona, January 2013; thanks are due to Edward W. Cliver for inviting Judit Muraközy and András Ludmány. The research leading to these results has received funding from the European Commission’s Seventh Framework Programme (FP7/2007-2013) under the grant agreement eHeroes (project n° 284461, www.eheroes.eu ).

Disclosure of Potential Conflicts of Interest

The authors declare that they have no conflicts of interest.

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Copyright information

© Springer Science+Business Media Dordrecht 2016

Authors and Affiliations

  1. 1.Heliophysical Observatory, Research Centre for Astronomy and Earth SciencesHungarian Academy of SciencesDebrecenHungary

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