A New Model of Solar Illumination of Earth’s Atmosphere during Night-Time

In this work, a solar illumination model of the Earth’s atmosphere is developed. The developed model allows us to determine with extreme accuracy how the atmospheric illumination varies during night hours on a global scale. This time-dependent variation in illumination causes a series of sudden chan...

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Main Authors: Roberto Colonna, Valerio Tramutoli
Format: Article
Language:English
Published: MDPI AG 2021-04-01
Series:Earth
Subjects:
Online Access:https://www.mdpi.com/2673-4834/2/2/12
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spelling doaj-a70d64efb80f4af98fd5e9bc0da086b72021-09-09T13:41:46ZengMDPI AGEarth2673-48342021-04-0121219120710.3390/earth2020012A New Model of Solar Illumination of Earth’s Atmosphere during Night-TimeRoberto Colonna0Valerio Tramutoli1School of Engineering, University of Basilicata, 85100 Potenza, ItalySchool of Engineering, University of Basilicata, 85100 Potenza, ItalyIn this work, a solar illumination model of the Earth’s atmosphere is developed. The developed model allows us to determine with extreme accuracy how the atmospheric illumination varies during night hours on a global scale. This time-dependent variation in illumination causes a series of sudden changes in the entire Earth-atmosphere-ionosphere system of considerable interest for various research sectors and applications related to climate change, ionospheric disturbances, navigation and global positioning systems. The use of the proposed solar illumination model to calculate the time-dependent Solar Terminator Height (<i>STH</i>) at the global scale is also presented.Time-dependent <i>STH</i> impact on the measurements of ionospheric Total Electron Content (<i>TEC</i>) is, for the first time, investigated on the basis of 20 years long time series of GPS-based measurements collected at ground. The correlation analysis, performed in the post-sunset hours, allows new insights into the dependence of <i>TEC</i>–<i>STH</i> relation on the different periods (seasons) of observation and solar activity conditions.https://www.mdpi.com/2673-4834/2/2/12Solar Terminator Heightsolar illumination of the atmosphereTotal Electron ContentionosphereGNSSsolar activity
collection DOAJ
language English
format Article
sources DOAJ
author Roberto Colonna
Valerio Tramutoli
spellingShingle Roberto Colonna
Valerio Tramutoli
A New Model of Solar Illumination of Earth’s Atmosphere during Night-Time
Earth
Solar Terminator Height
solar illumination of the atmosphere
Total Electron Content
ionosphere
GNSS
solar activity
author_facet Roberto Colonna
Valerio Tramutoli
author_sort Roberto Colonna
title A New Model of Solar Illumination of Earth’s Atmosphere during Night-Time
title_short A New Model of Solar Illumination of Earth’s Atmosphere during Night-Time
title_full A New Model of Solar Illumination of Earth’s Atmosphere during Night-Time
title_fullStr A New Model of Solar Illumination of Earth’s Atmosphere during Night-Time
title_full_unstemmed A New Model of Solar Illumination of Earth’s Atmosphere during Night-Time
title_sort new model of solar illumination of earth’s atmosphere during night-time
publisher MDPI AG
series Earth
issn 2673-4834
publishDate 2021-04-01
description In this work, a solar illumination model of the Earth’s atmosphere is developed. The developed model allows us to determine with extreme accuracy how the atmospheric illumination varies during night hours on a global scale. This time-dependent variation in illumination causes a series of sudden changes in the entire Earth-atmosphere-ionosphere system of considerable interest for various research sectors and applications related to climate change, ionospheric disturbances, navigation and global positioning systems. The use of the proposed solar illumination model to calculate the time-dependent Solar Terminator Height (<i>STH</i>) at the global scale is also presented.Time-dependent <i>STH</i> impact on the measurements of ionospheric Total Electron Content (<i>TEC</i>) is, for the first time, investigated on the basis of 20 years long time series of GPS-based measurements collected at ground. The correlation analysis, performed in the post-sunset hours, allows new insights into the dependence of <i>TEC</i>–<i>STH</i> relation on the different periods (seasons) of observation and solar activity conditions.
topic Solar Terminator Height
solar illumination of the atmosphere
Total Electron Content
ionosphere
GNSS
solar activity
url https://www.mdpi.com/2673-4834/2/2/12
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