Cargando…

Realistic Worst Case for a Severe Space Weather Event Driven by a Fast Solar Wind Stream

Satellite charging is one of the most important risks for satellites on orbit. Satellite charging can lead to an electrostatic discharge resulting in component damage, phantom commands, and loss of service and in exceptional cases total satellite loss. Here we construct a realistic worst case for a...

Descripción completa

Detalles Bibliográficos
Autores principales: Horne, Richard B., Phillips, Mark W., Glauert, Sarah A., Meredith, Nigel P., Hands, Alex D. P., Ryden, Keith A., Li, Wen
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2018
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6473668/
https://www.ncbi.nlm.nih.gov/pubmed/31031572
http://dx.doi.org/10.1029/2018SW001948
_version_ 1783412482010775552
author Horne, Richard B.
Phillips, Mark W.
Glauert, Sarah A.
Meredith, Nigel P.
Hands, Alex D. P.
Ryden, Keith A.
Li, Wen
author_facet Horne, Richard B.
Phillips, Mark W.
Glauert, Sarah A.
Meredith, Nigel P.
Hands, Alex D. P.
Ryden, Keith A.
Li, Wen
author_sort Horne, Richard B.
collection PubMed
description Satellite charging is one of the most important risks for satellites on orbit. Satellite charging can lead to an electrostatic discharge resulting in component damage, phantom commands, and loss of service and in exceptional cases total satellite loss. Here we construct a realistic worst case for a fast solar wind stream event lasting 5 days or more and use a physical model to calculate the maximum electron flux greater than 2 MeV for geostationary orbit. We find that the flux tends toward a value of 10(6) cm(−2)·s(−1)·sr(−1) after 5 days and remains high for another 5 days. The resulting flux is comparable to a 1 in 150‐year event found from an independent statistical analysis of electron data. Approximately 2.5 mm of Al shielding would be required to reduce the internal charging current to below the National Aeronautics and Space Administration‐recommended guidelines, much more than is currently used. Thus, we would expect many satellites to report electrostatic discharge anomalies during such an event with a strong likelihood of service outage and total satellite loss. We conclude that satellites at geostationary orbit are more likely to be at risk from fast solar wind stream event than a Carrington‐type storm.
format Online
Article
Text
id pubmed-6473668
institution National Center for Biotechnology Information
language English
publishDate 2018
publisher John Wiley and Sons Inc.
record_format MEDLINE/PubMed
spelling pubmed-64736682019-04-24 Realistic Worst Case for a Severe Space Weather Event Driven by a Fast Solar Wind Stream Horne, Richard B. Phillips, Mark W. Glauert, Sarah A. Meredith, Nigel P. Hands, Alex D. P. Ryden, Keith A. Li, Wen Space Weather Research Articles Satellite charging is one of the most important risks for satellites on orbit. Satellite charging can lead to an electrostatic discharge resulting in component damage, phantom commands, and loss of service and in exceptional cases total satellite loss. Here we construct a realistic worst case for a fast solar wind stream event lasting 5 days or more and use a physical model to calculate the maximum electron flux greater than 2 MeV for geostationary orbit. We find that the flux tends toward a value of 10(6) cm(−2)·s(−1)·sr(−1) after 5 days and remains high for another 5 days. The resulting flux is comparable to a 1 in 150‐year event found from an independent statistical analysis of electron data. Approximately 2.5 mm of Al shielding would be required to reduce the internal charging current to below the National Aeronautics and Space Administration‐recommended guidelines, much more than is currently used. Thus, we would expect many satellites to report electrostatic discharge anomalies during such an event with a strong likelihood of service outage and total satellite loss. We conclude that satellites at geostationary orbit are more likely to be at risk from fast solar wind stream event than a Carrington‐type storm. John Wiley and Sons Inc. 2018-09-03 2018-09 /pmc/articles/PMC6473668/ /pubmed/31031572 http://dx.doi.org/10.1029/2018SW001948 Text en ©2018. The Authors. This is an open access article under the terms of the http://creativecommons.org/licenses/by/4.0/ License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
spellingShingle Research Articles
Horne, Richard B.
Phillips, Mark W.
Glauert, Sarah A.
Meredith, Nigel P.
Hands, Alex D. P.
Ryden, Keith A.
Li, Wen
Realistic Worst Case for a Severe Space Weather Event Driven by a Fast Solar Wind Stream
title Realistic Worst Case for a Severe Space Weather Event Driven by a Fast Solar Wind Stream
title_full Realistic Worst Case for a Severe Space Weather Event Driven by a Fast Solar Wind Stream
title_fullStr Realistic Worst Case for a Severe Space Weather Event Driven by a Fast Solar Wind Stream
title_full_unstemmed Realistic Worst Case for a Severe Space Weather Event Driven by a Fast Solar Wind Stream
title_short Realistic Worst Case for a Severe Space Weather Event Driven by a Fast Solar Wind Stream
title_sort realistic worst case for a severe space weather event driven by a fast solar wind stream
topic Research Articles
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6473668/
https://www.ncbi.nlm.nih.gov/pubmed/31031572
http://dx.doi.org/10.1029/2018SW001948
work_keys_str_mv AT hornerichardb realisticworstcaseforaseverespaceweathereventdrivenbyafastsolarwindstream
AT phillipsmarkw realisticworstcaseforaseverespaceweathereventdrivenbyafastsolarwindstream
AT glauertsaraha realisticworstcaseforaseverespaceweathereventdrivenbyafastsolarwindstream
AT meredithnigelp realisticworstcaseforaseverespaceweathereventdrivenbyafastsolarwindstream
AT handsalexdp realisticworstcaseforaseverespaceweathereventdrivenbyafastsolarwindstream
AT rydenkeitha realisticworstcaseforaseverespaceweathereventdrivenbyafastsolarwindstream
AT liwen realisticworstcaseforaseverespaceweathereventdrivenbyafastsolarwindstream