Sodium dayglow: Observation and interpretation of a large diurnal variation

International audience Analysis of the dayglow of the sodium D lines since September 1960 and the twilight glow since 1954 at Haute Provence Observatory shows a large seasonal maximum of 30 kR for the dayglow in June. The ratio of daytime to twilight abundance then is about 7 to 1. The ratio becomes...

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Published in:Journal of Geophysical Research
Main Authors: Blamont, Jacques Emile, Donahue, T.
Other Authors: Service d'aéronomie (SA), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 1964
Subjects:
Online Access:https://hal-insu.archives-ouvertes.fr/insu-03636083
https://hal-insu.archives-ouvertes.fr/insu-03636083/document
https://hal-insu.archives-ouvertes.fr/insu-03636083/file/ark%20_67375_WNG-ZPPD1V8Q-1.pdf
https://doi.org/10.1029/JZ069i019p04093
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spelling ftinsu:oai:HAL:insu-03636083v1 2023-06-18T03:43:21+02:00 Sodium dayglow: Observation and interpretation of a large diurnal variation Blamont, Jacques Emile Donahue, T. Service d'aéronomie (SA) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) 1964-10-01 https://hal-insu.archives-ouvertes.fr/insu-03636083 https://hal-insu.archives-ouvertes.fr/insu-03636083/document https://hal-insu.archives-ouvertes.fr/insu-03636083/file/ark%20_67375_WNG-ZPPD1V8Q-1.pdf https://doi.org/10.1029/JZ069i019p04093 en eng HAL CCSD American Geophysical Union info:eu-repo/semantics/altIdentifier/doi/10.1029/JZ069i019p04093 insu-03636083 https://hal-insu.archives-ouvertes.fr/insu-03636083 https://hal-insu.archives-ouvertes.fr/insu-03636083/document https://hal-insu.archives-ouvertes.fr/insu-03636083/file/ark%20_67375_WNG-ZPPD1V8Q-1.pdf doi:10.1029/JZ069i019p04093 http://hal.archives-ouvertes.fr/licences/copyright/ info:eu-repo/semantics/OpenAccess ISSN: 0148-0227 EISSN: 2156-2202 Journal of Geophysical Research https://hal-insu.archives-ouvertes.fr/insu-03636083 Journal of Geophysical Research, 1964, 69 (19), pp.4093-4127. ⟨10.1029/JZ069i019p04093⟩ Sodium D Lines Dayglow Twilight Glow Diurnal Variation Atmospheric Ozone [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] info:eu-repo/semantics/article Journal articles 1964 ftinsu https://doi.org/10.1029/JZ069i019p04093 2023-06-05T20:43:05Z International audience Analysis of the dayglow of the sodium D lines since September 1960 and the twilight glow since 1954 at Haute Provence Observatory shows a large seasonal maximum of 30 kR for the dayglow in June. The ratio of daytime to twilight abundance then is about 7 to 1. The ratio becomes 2 to 1 in December. Evidence presented for the reality of this effect includes actual line profiles showing an emission peak above Rayleigh-scattered background, observation of the dayglow from a high-altitude airplane, and observation of the dayglow with a rocket-borne photometer. The seasonal maximum is accompanied by a seasonal decrease of 5 km in twilight layer altitude in midsummer. The effect is interpreted as being caused by a diurnal variation in atomic oxygen and ozone enhanced by turbulent diffusion of the sodium and its compounds. Other possible interpretations such as photochemical excitation are rejected. A seasonal variation is also found in the ratio of morning to evening sodium abundance in twilight. The maximum ratio is 1.4 at the equinoxes. At Tromsø, Norway, the dayglow intensity is about 15 kR and shows no seasonal variation. Article in Journal/Newspaper Tromsø Institut national des sciences de l'Univers: HAL-INSU Norway Tromsø Journal of Geophysical Research 69 19 4093 4127
institution Open Polar
collection Institut national des sciences de l'Univers: HAL-INSU
op_collection_id ftinsu
language English
topic Sodium D Lines
Dayglow
Twilight Glow
Diurnal Variation
Atmospheric Ozone
[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
spellingShingle Sodium D Lines
Dayglow
Twilight Glow
Diurnal Variation
Atmospheric Ozone
[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
Blamont, Jacques Emile
Donahue, T.
Sodium dayglow: Observation and interpretation of a large diurnal variation
topic_facet Sodium D Lines
Dayglow
Twilight Glow
Diurnal Variation
Atmospheric Ozone
[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]
description International audience Analysis of the dayglow of the sodium D lines since September 1960 and the twilight glow since 1954 at Haute Provence Observatory shows a large seasonal maximum of 30 kR for the dayglow in June. The ratio of daytime to twilight abundance then is about 7 to 1. The ratio becomes 2 to 1 in December. Evidence presented for the reality of this effect includes actual line profiles showing an emission peak above Rayleigh-scattered background, observation of the dayglow from a high-altitude airplane, and observation of the dayglow with a rocket-borne photometer. The seasonal maximum is accompanied by a seasonal decrease of 5 km in twilight layer altitude in midsummer. The effect is interpreted as being caused by a diurnal variation in atomic oxygen and ozone enhanced by turbulent diffusion of the sodium and its compounds. Other possible interpretations such as photochemical excitation are rejected. A seasonal variation is also found in the ratio of morning to evening sodium abundance in twilight. The maximum ratio is 1.4 at the equinoxes. At Tromsø, Norway, the dayglow intensity is about 15 kR and shows no seasonal variation.
author2 Service d'aéronomie (SA)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
format Article in Journal/Newspaper
author Blamont, Jacques Emile
Donahue, T.
author_facet Blamont, Jacques Emile
Donahue, T.
author_sort Blamont, Jacques Emile
title Sodium dayglow: Observation and interpretation of a large diurnal variation
title_short Sodium dayglow: Observation and interpretation of a large diurnal variation
title_full Sodium dayglow: Observation and interpretation of a large diurnal variation
title_fullStr Sodium dayglow: Observation and interpretation of a large diurnal variation
title_full_unstemmed Sodium dayglow: Observation and interpretation of a large diurnal variation
title_sort sodium dayglow: observation and interpretation of a large diurnal variation
publisher HAL CCSD
publishDate 1964
url https://hal-insu.archives-ouvertes.fr/insu-03636083
https://hal-insu.archives-ouvertes.fr/insu-03636083/document
https://hal-insu.archives-ouvertes.fr/insu-03636083/file/ark%20_67375_WNG-ZPPD1V8Q-1.pdf
https://doi.org/10.1029/JZ069i019p04093
geographic Norway
Tromsø
geographic_facet Norway
Tromsø
genre Tromsø
genre_facet Tromsø
op_source ISSN: 0148-0227
EISSN: 2156-2202
Journal of Geophysical Research
https://hal-insu.archives-ouvertes.fr/insu-03636083
Journal of Geophysical Research, 1964, 69 (19), pp.4093-4127. ⟨10.1029/JZ069i019p04093⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1029/JZ069i019p04093
insu-03636083
https://hal-insu.archives-ouvertes.fr/insu-03636083
https://hal-insu.archives-ouvertes.fr/insu-03636083/document
https://hal-insu.archives-ouvertes.fr/insu-03636083/file/ark%20_67375_WNG-ZPPD1V8Q-1.pdf
doi:10.1029/JZ069i019p04093
op_rights http://hal.archives-ouvertes.fr/licences/copyright/
info:eu-repo/semantics/OpenAccess
op_doi https://doi.org/10.1029/JZ069i019p04093
container_title Journal of Geophysical Research
container_volume 69
container_issue 19
container_start_page 4093
op_container_end_page 4127
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