Aeronomy, a 20th Century emergent science: the role of solar Lyman series

Aeronomy is, by definition, a multidisciplinary science which can be used to study the terrestrial atmosphere, as well as any planetary atmosphere and even the interplanetary space. It was officially recognized in 1954 by the International Union of Geodesy and Geophysics. The major objective...

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Main Author: G. Kockarts
Format: Article
Language:English
Published: Copernicus Publications 2002-05-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/20/585/2002/angeo-20-585-2002.pdf
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author G. Kockarts
G. Kockarts
author_facet G. Kockarts
G. Kockarts
author_sort G. Kockarts
collection DOAJ
description Aeronomy is, by definition, a multidisciplinary science which can be used to study the terrestrial atmosphere, as well as any planetary atmosphere and even the interplanetary space. It was officially recognized in 1954 by the International Union of Geodesy and Geophysics. The major objective of the present paper is to show how aeronomy developed since its infancy. The subject is so large that a guide-line has been chosen to see how aeronomy affects our atmospheric knowledge. This guideline is the solar Lyman alpha radiation which has different effects in the solar system. After a short description of the origins of aeronomy the first observations of this line are summarized since the beginning of the space age. Then the consequences of these observations are analyzed for the physics and chemistry of the neutral terrestrial atmosphere. New chemical processes had to be introduced, as well as new transport phenomena. Solar Lyman alpha also influences the structure of the Earth’s ionosphere, particularly the D-region. In the terrestrial exosphere, solar Lyman alpha scattered resonantly by atomic hydrogen is at present the only way to estimate this constituent in an almost collisionless medium. Since planetary atmospheres also contain atomic hydrogen, the Lyman alpha line has been used to deduce the abundance of this constituent. The same is true for the interplanetary space where Lyman alpha observations can be a good tool to determine the concentration. The last section of the paper presents a question which is intended to stimulate further research in aeronomy.<br><br><b>Key words. </b>Atmospheric composition and structure (middle atmosphere – composition and chemistry; thermosphere – composition and chemistry) – history of geophysics (atmospheric sciences)
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spelling doaj.art-5a30e619f6b946d3899d1f191ad3c5d42022-12-21T18:28:11ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762002-05-012058559810.5194/angeo-20-585-2002Aeronomy, a 20th Century emergent science: the role of solar Lyman seriesG. Kockarts0G. Kockarts1Correspondence to: G. Kockarts (gaston.kockarts@oma.be)Institut d’Aéronomie spatiale de Belgique, 3 avenue Circulaire, B-1180 Brussels, BelgiumAeronomy is, by definition, a multidisciplinary science which can be used to study the terrestrial atmosphere, as well as any planetary atmosphere and even the interplanetary space. It was officially recognized in 1954 by the International Union of Geodesy and Geophysics. The major objective of the present paper is to show how aeronomy developed since its infancy. The subject is so large that a guide-line has been chosen to see how aeronomy affects our atmospheric knowledge. This guideline is the solar Lyman alpha radiation which has different effects in the solar system. After a short description of the origins of aeronomy the first observations of this line are summarized since the beginning of the space age. Then the consequences of these observations are analyzed for the physics and chemistry of the neutral terrestrial atmosphere. New chemical processes had to be introduced, as well as new transport phenomena. Solar Lyman alpha also influences the structure of the Earth’s ionosphere, particularly the D-region. In the terrestrial exosphere, solar Lyman alpha scattered resonantly by atomic hydrogen is at present the only way to estimate this constituent in an almost collisionless medium. Since planetary atmospheres also contain atomic hydrogen, the Lyman alpha line has been used to deduce the abundance of this constituent. The same is true for the interplanetary space where Lyman alpha observations can be a good tool to determine the concentration. The last section of the paper presents a question which is intended to stimulate further research in aeronomy.<br><br><b>Key words. </b>Atmospheric composition and structure (middle atmosphere – composition and chemistry; thermosphere – composition and chemistry) – history of geophysics (atmospheric sciences)https://www.ann-geophys.net/20/585/2002/angeo-20-585-2002.pdf
spellingShingle G. Kockarts
G. Kockarts
Aeronomy, a 20th Century emergent science: the role of solar Lyman series
Annales Geophysicae
title Aeronomy, a 20th Century emergent science: the role of solar Lyman series
title_full Aeronomy, a 20th Century emergent science: the role of solar Lyman series
title_fullStr Aeronomy, a 20th Century emergent science: the role of solar Lyman series
title_full_unstemmed Aeronomy, a 20th Century emergent science: the role of solar Lyman series
title_short Aeronomy, a 20th Century emergent science: the role of solar Lyman series
title_sort aeronomy a 20th century emergent science the role of solar lyman series
url https://www.ann-geophys.net/20/585/2002/angeo-20-585-2002.pdf
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