What to Do When the F10.7 Goes Out?

Abstract The solar radio flux at 10.7 cm, known as F10.7, is a critical operational space weather index. However, without a clear backup, any interruption to the service can result in substantial errors in model outputs. In this paper we show the impact of one such outage in March 2022 on the models...

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Main Authors: Sean Elvidge, David R. Themens, Matthew K. Brown, Elizabeth Donegan‐Lawley
Format: Article
Language:English
Published: Wiley 2023-04-01
Series:Space Weather
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Online Access:https://doi.org/10.1029/2022SW003392
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author Sean Elvidge
David R. Themens
Matthew K. Brown
Elizabeth Donegan‐Lawley
author_facet Sean Elvidge
David R. Themens
Matthew K. Brown
Elizabeth Donegan‐Lawley
author_sort Sean Elvidge
collection DOAJ
description Abstract The solar radio flux at 10.7 cm, known as F10.7, is a critical operational space weather index. However, without a clear backup, any interruption to the service can result in substantial errors in model outputs. In this paper we show the impact of one such outage in March 2022 on the models TIE‐GCM and NeQuick, and present a number of alternative solutions that could be used for future outages. The analysis is extended to the F10.7 time series since 1951 and the approach resulting in the smallest reconstruction error of F10.7 uses the solar radio flux observations at alternative wavelengths (the best giving a percentage error of 3.1%). Alternatively, use of Sunspot Number, a regular, robust alternative observation, results in a mean percentage error of 8.2% and is also a reliable fallback solution. Additionally, analysis of the error on the use of the conversion between the 12‐month rolling sunspot number (R12) and its conversion to F10.7 is included.
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spelling doaj-art-44c52ba149834cfcad34f34b0b2a73f22025-01-14T16:26:47ZengWileySpace Weather1542-73902023-04-01214n/an/a10.1029/2022SW003392What to Do When the F10.7 Goes Out?Sean Elvidge0David R. Themens1Matthew K. Brown2Elizabeth Donegan‐Lawley3Space Environment and Radio Engineering Group (SERENE) University of Birmingham Birmingham UKSpace Environment and Radio Engineering Group (SERENE) University of Birmingham Birmingham UKSpace Environment and Radio Engineering Group (SERENE) University of Birmingham Birmingham UKSpace Environment and Radio Engineering Group (SERENE) University of Birmingham Birmingham UKAbstract The solar radio flux at 10.7 cm, known as F10.7, is a critical operational space weather index. However, without a clear backup, any interruption to the service can result in substantial errors in model outputs. In this paper we show the impact of one such outage in March 2022 on the models TIE‐GCM and NeQuick, and present a number of alternative solutions that could be used for future outages. The analysis is extended to the F10.7 time series since 1951 and the approach resulting in the smallest reconstruction error of F10.7 uses the solar radio flux observations at alternative wavelengths (the best giving a percentage error of 3.1%). Alternatively, use of Sunspot Number, a regular, robust alternative observation, results in a mean percentage error of 8.2% and is also a reliable fallback solution. Additionally, analysis of the error on the use of the conversion between the 12‐month rolling sunspot number (R12) and its conversion to F10.7 is included.https://doi.org/10.1029/2022SW003392operationsF10.7upper atmosphereionospherethermosphere
spellingShingle Sean Elvidge
David R. Themens
Matthew K. Brown
Elizabeth Donegan‐Lawley
What to Do When the F10.7 Goes Out?
Space Weather
operations
F10.7
upper atmosphere
ionosphere
thermosphere
title What to Do When the F10.7 Goes Out?
title_full What to Do When the F10.7 Goes Out?
title_fullStr What to Do When the F10.7 Goes Out?
title_full_unstemmed What to Do When the F10.7 Goes Out?
title_short What to Do When the F10.7 Goes Out?
title_sort what to do when the f10 7 goes out
topic operations
F10.7
upper atmosphere
ionosphere
thermosphere
url https://doi.org/10.1029/2022SW003392
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