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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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 |
work_keys_str_mv |
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