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Infrared Radiation in the Thermosphere Near the End of Solar Cycle 24

Observations of thermospheric infrared radiative cooling by carbon dioxide (CO(2)) and nitric oxide (NO) from 2002 to 2018 are presented. The time span covers more than 6,000 days including most of solar cycle (SC) 23 and the entirety of SC 24 to date. Maxima of infrared cooling rate profiles (nW/m(...

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Autores principales: Mlynczak, Martin G., Hunt, Linda A., Marshall, B. Thomas, Russell, James M.
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/PMC6360400/
https://www.ncbi.nlm.nih.gov/pubmed/30774165
http://dx.doi.org/10.1029/2018GL080389
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author Mlynczak, Martin G.
Hunt, Linda A.
Marshall, B. Thomas
Russell, James M.
author_facet Mlynczak, Martin G.
Hunt, Linda A.
Marshall, B. Thomas
Russell, James M.
author_sort Mlynczak, Martin G.
collection PubMed
description Observations of thermospheric infrared radiative cooling by carbon dioxide (CO(2)) and nitric oxide (NO) from 2002 to 2018 are presented. The time span covers more than 6,000 days including most of solar cycle (SC) 23 and the entirety of SC 24 to date. Maxima of infrared cooling rate profiles (nW/m(3)) are smaller during SC 24 than SC 23, indicating a cooler thermosphere. Rates of global infrared power (W) from CO(2) are now at levels observed during the deep solar minimum of 2009. Rates of NO power are still larger than those observed during 2009 and are being maintained at an elevated level by geomagnetic activity. During SC 24 to date, the thermosphere has radiated 70% of the energy of the mean of the past five cycles and would require an additional 1,690 days at current infrared radiation rates to reach that amount.
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spelling pubmed-63604002019-02-14 Infrared Radiation in the Thermosphere Near the End of Solar Cycle 24 Mlynczak, Martin G. Hunt, Linda A. Marshall, B. Thomas Russell, James M. Geophys Res Lett Research Letters Observations of thermospheric infrared radiative cooling by carbon dioxide (CO(2)) and nitric oxide (NO) from 2002 to 2018 are presented. The time span covers more than 6,000 days including most of solar cycle (SC) 23 and the entirety of SC 24 to date. Maxima of infrared cooling rate profiles (nW/m(3)) are smaller during SC 24 than SC 23, indicating a cooler thermosphere. Rates of global infrared power (W) from CO(2) are now at levels observed during the deep solar minimum of 2009. Rates of NO power are still larger than those observed during 2009 and are being maintained at an elevated level by geomagnetic activity. During SC 24 to date, the thermosphere has radiated 70% of the energy of the mean of the past five cycles and would require an additional 1,690 days at current infrared radiation rates to reach that amount. John Wiley and Sons Inc. 2018-11-09 2018-11-16 /pmc/articles/PMC6360400/ /pubmed/30774165 http://dx.doi.org/10.1029/2018GL080389 Text en ©2018. The Authors. This is an open access article under the terms of the http://creativecommons.org/licenses/by-nc-nd/4.0/ License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made.
spellingShingle Research Letters
Mlynczak, Martin G.
Hunt, Linda A.
Marshall, B. Thomas
Russell, James M.
Infrared Radiation in the Thermosphere Near the End of Solar Cycle 24
title Infrared Radiation in the Thermosphere Near the End of Solar Cycle 24
title_full Infrared Radiation in the Thermosphere Near the End of Solar Cycle 24
title_fullStr Infrared Radiation in the Thermosphere Near the End of Solar Cycle 24
title_full_unstemmed Infrared Radiation in the Thermosphere Near the End of Solar Cycle 24
title_short Infrared Radiation in the Thermosphere Near the End of Solar Cycle 24
title_sort infrared radiation in the thermosphere near the end of solar cycle 24
topic Research Letters
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6360400/
https://www.ncbi.nlm.nih.gov/pubmed/30774165
http://dx.doi.org/10.1029/2018GL080389
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