Photoionization and Photodissociation Rates across a Solar Cycle

Unattenuated photoionization and photodissociation rate coefficients are calculated using solar spectral irradiance measurements across a continuous solar cycle spanning 2004–2014. These rates are organized by corresponding daily F _10.7 P indices, where F _10.7 P $=\,\frac{1}{2}({F}_{10.7}+{F}_{10....

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Main Authors: Luke Moore, Russell Mapaye
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Planetary Science Journal
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Online Access:https://doi.org/10.3847/PSJ/add6a2
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author Luke Moore
Russell Mapaye
author_facet Luke Moore
Russell Mapaye
author_sort Luke Moore
collection DOAJ
description Unattenuated photoionization and photodissociation rate coefficients are calculated using solar spectral irradiance measurements across a continuous solar cycle spanning 2004–2014. These rates are organized by corresponding daily F _10.7 P indices, where F _10.7 P $=\,\frac{1}{2}({F}_{10.7}+{F}_{10.7}A)$ , F _10.7 is a common historical proxy for solar ultraviolet and soft X-ray activity, and F _10.7 A is its 81 day running average. Power-law relationships are established between F _10.7 P and photo rate coefficients for 48 reactions across 12 of the most common species in solar system upper atmospheres and cometary comae: H, H _2 , OH, H _2 O, O, O _2 , C, CO, CO _2 , N _2 , N, and CH _4 . The resulting coefficients are broadly consistent with previous estimates and provide a practical, efficient means of estimating photoionization and photodissociation rates for a range of planetary and cometary applications.
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spelling doaj-art-2a2e4f1c79ad409fa5d4aade7b1dc3482025-08-20T03:45:15ZengIOP PublishingThe Planetary Science Journal2632-33382025-01-016613110.3847/PSJ/add6a2Photoionization and Photodissociation Rates across a Solar CycleLuke Moore0https://orcid.org/0000-0003-4481-9862Russell Mapaye1https://orcid.org/0009-0000-9453-1299Department of Astronomy, Boston University , Boston, MA, USA; Center for Space Physics, Boston University , Boston, MA, USADepartment of Astronomy, Boston University , Boston, MA, USAUnattenuated photoionization and photodissociation rate coefficients are calculated using solar spectral irradiance measurements across a continuous solar cycle spanning 2004–2014. These rates are organized by corresponding daily F _10.7 P indices, where F _10.7 P $=\,\frac{1}{2}({F}_{10.7}+{F}_{10.7}A)$ , F _10.7 is a common historical proxy for solar ultraviolet and soft X-ray activity, and F _10.7 A is its 81 day running average. Power-law relationships are established between F _10.7 P and photo rate coefficients for 48 reactions across 12 of the most common species in solar system upper atmospheres and cometary comae: H, H _2 , OH, H _2 O, O, O _2 , C, CO, CO _2 , N _2 , N, and CH _4 . The resulting coefficients are broadly consistent with previous estimates and provide a practical, efficient means of estimating photoionization and photodissociation rates for a range of planetary and cometary applications.https://doi.org/10.3847/PSJ/add6a2Planetary atmospheresUpper atmosphereComaePhotoionizationPhotodissociation reactionsSolar spectral irradiance
spellingShingle Luke Moore
Russell Mapaye
Photoionization and Photodissociation Rates across a Solar Cycle
The Planetary Science Journal
Planetary atmospheres
Upper atmosphere
Comae
Photoionization
Photodissociation reactions
Solar spectral irradiance
title Photoionization and Photodissociation Rates across a Solar Cycle
title_full Photoionization and Photodissociation Rates across a Solar Cycle
title_fullStr Photoionization and Photodissociation Rates across a Solar Cycle
title_full_unstemmed Photoionization and Photodissociation Rates across a Solar Cycle
title_short Photoionization and Photodissociation Rates across a Solar Cycle
title_sort photoionization and photodissociation rates across a solar cycle
topic Planetary atmospheres
Upper atmosphere
Comae
Photoionization
Photodissociation reactions
Solar spectral irradiance
url https://doi.org/10.3847/PSJ/add6a2
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