Charting the solar cycle

Sunspot records reveal that whilst the Sun has an approximately 11 year cycle of activity, no two cycles are of the same duration. Since this activity is a direct driver of space weather at Earth, this presents an operational challenge to quantifying space weather risk. We recently showed that the H...

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Main Author: S. C. Chapman
Format: Article
Language:English
Published: Frontiers Media S.A. 2023-02-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2022.1037096/full
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author S. C. Chapman
S. C. Chapman
author_facet S. C. Chapman
S. C. Chapman
author_sort S. C. Chapman
collection DOAJ
description Sunspot records reveal that whilst the Sun has an approximately 11 year cycle of activity, no two cycles are of the same duration. Since this activity is a direct driver of space weather at Earth, this presents an operational challenge to quantifying space weather risk. We recently showed that the Hilbert transform of the sunspot record can be used to map the variable cycle length onto a regular “clock” where each cycle has the same duration in Hilbert analytic phase. Extreme geomagnetic storms rarely occur within the quiet part of the cycle which is a fixed interval of analytic phase on the clock; there is a clear active-quiet switch-off and quiet-active switch-on of activity. Here we show how the times of the switch-on/off can be determined directly from the sunspot time-series, without requiring a Hilbert transform. We propose a method-charting-that can be used to combine observations, and reports of societal impacts, to improve our understanding of space weather risk.
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spelling doaj.art-a8463c9ba1b04bf5a4538e4fc22405132023-02-09T04:50:01ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2023-02-01910.3389/fspas.2022.10370961037096Charting the solar cycleS. C. Chapman0S. C. Chapman1Centre for Fusion, Space and Astrophysics, University of Warwick, Coventry, United KingdomDepartment of Mathematics and Statistics, University of Tromso, Tromso, NorwaySunspot records reveal that whilst the Sun has an approximately 11 year cycle of activity, no two cycles are of the same duration. Since this activity is a direct driver of space weather at Earth, this presents an operational challenge to quantifying space weather risk. We recently showed that the Hilbert transform of the sunspot record can be used to map the variable cycle length onto a regular “clock” where each cycle has the same duration in Hilbert analytic phase. Extreme geomagnetic storms rarely occur within the quiet part of the cycle which is a fixed interval of analytic phase on the clock; there is a clear active-quiet switch-off and quiet-active switch-on of activity. Here we show how the times of the switch-on/off can be determined directly from the sunspot time-series, without requiring a Hilbert transform. We propose a method-charting-that can be used to combine observations, and reports of societal impacts, to improve our understanding of space weather risk.https://www.frontiersin.org/articles/10.3389/fspas.2022.1037096/fullsolar cyclespace weathergeomagnetic stormsHilbert transformsunspot recordGleissberg cycle
spellingShingle S. C. Chapman
S. C. Chapman
Charting the solar cycle
Frontiers in Astronomy and Space Sciences
solar cycle
space weather
geomagnetic storms
Hilbert transform
sunspot record
Gleissberg cycle
title Charting the solar cycle
title_full Charting the solar cycle
title_fullStr Charting the solar cycle
title_full_unstemmed Charting the solar cycle
title_short Charting the solar cycle
title_sort charting the solar cycle
topic solar cycle
space weather
geomagnetic storms
Hilbert transform
sunspot record
Gleissberg cycle
url https://www.frontiersin.org/articles/10.3389/fspas.2022.1037096/full
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