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Recalibration of the Sunspot-Number: Status Report

2023/03/01 by F. Clette, Laure Lefèvre, L. Lefèvre +31 · 1 voice · 8 citations
Earth and Planetary Sciences · Physics and Astronomy · #Geophysics and Gravity Measurements #Ionosphere and magnetosphere dynamics #Solar and Space Plasma Dynamics

paper · pdf · doi:10.1007/s11207-023-02136-3

openalex publication_date 2023/03/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Abstract We report progress on the ongoing recalibration of the Wolf sunspot number ( SN <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>S</mml:mi><mml:mi>N</mml:mi></mml:msub></mml:math> ) and group-sunspot number ( GN <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>G</mml:mi><mml:mi>N</mml:mi></mml:msub></mml:math> ) following the release of version 2.0 of SN <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>S</mml:mi><mml:mi>N</mml:mi></mml:msub></mml:math> in 2015. This report constitutes both an update of the efforts reported in the 2016 Topical Issue of Solar Physics and a summary of work by the International Space Science Institute (ISSI) International Team formed in 2017 to develop optimal SN <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>S</mml:mi><mml:mi>N</mml:mi></mml:msub></mml:math> and GN <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>G</mml:mi><mml:mi>N</mml:mi></mml:msub></mml:math> reconstruction methods while continuing to expand the historical sunspot-number database. Significant progress has been made on the database side while more work is needed to bring the various proposed SN <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>S</mml:mi><mml:mi>N</mml:mi></mml:msub></mml:math> and (primarily) GN <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>G</mml:mi><mml:mi>N</mml:mi></mml:msub></mml:math> reconstruction methods closer to maturity, after which the new reconstructions (or combinations thereof) can be compared with (a) “benchmark” expectations for any normalization scheme (e.g., a general increase in observer normalization factors going back in time), and (b) independent proxy data series such as F10.7 and the daily range of variations of Earth’s undisturbed magnetic field. New versions of the underlying databases for SN <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>S</mml:mi><mml:mi>N</mml:mi></mml:msub></mml:math> and GN <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>G</mml:mi><mml:mi>N</mml:mi></mml:msub></mml:math> will shortly become available for years through 2022 and we anticipate the release of the next versions of these two time series in 2024.

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