Enhancement of equatorial OI(1D) emissions at midnight

Abstract A number of recent studies have highlighted observational evidence of midnight brightness of the 630.0 nm nightglow, which is usually related to the midnight temperature maximum (MTM) effect. In this report, MTM-related enhancements of the 630.0 nm airglow around midnight are observed throu...

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Published in:Earth, Planets and Space
Main Authors: Chih-Yu Chiang, Tzu-Fang Chang, Sunny W. Y. Tam
Format: Article in Journal/Newspaper
Language:English
Published: SpringerOpen 2022
Subjects:
G
Online Access:https://doi.org/10.1186/s40623-022-01596-4
https://doaj.org/article/20db9548f6ec4d8db7b941cee6ef386a
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spelling ftdoajarticles:oai:doaj.org/article:20db9548f6ec4d8db7b941cee6ef386a 2023-05-15T18:12:57+02:00 Enhancement of equatorial OI(1D) emissions at midnight Chih-Yu Chiang Tzu-Fang Chang Sunny W. Y. Tam 2022-03-01T00:00:00Z https://doi.org/10.1186/s40623-022-01596-4 https://doaj.org/article/20db9548f6ec4d8db7b941cee6ef386a EN eng SpringerOpen https://doi.org/10.1186/s40623-022-01596-4 https://doaj.org/toc/1880-5981 doi:10.1186/s40623-022-01596-4 1880-5981 https://doaj.org/article/20db9548f6ec4d8db7b941cee6ef386a Earth, Planets and Space, Vol 74, Iss 1, Pp 1-13 (2022) Midnight temperature maximum ISUAL 630.0 nm SAMI-2 Airglow Geography. Anthropology. Recreation G Geodesy QB275-343 Geology QE1-996.5 article 2022 ftdoajarticles https://doi.org/10.1186/s40623-022-01596-4 2022-12-31T14:44:41Z Abstract A number of recent studies have highlighted observational evidence of midnight brightness of the 630.0 nm nightglow, which is usually related to the midnight temperature maximum (MTM) effect. In this report, MTM-related enhancements of the 630.0 nm airglow around midnight are observed through images from the ISUAL/FORMOSAT-2 satellite. The data statistics are classified into three specific types (no-peak, single-peaked, and double-peaked events) and separated into the different seasons. In order to understand the influences of geomagnetic conditions, the statistical analyses are also separated into two regions. One is collected from the region whose geomagnetic equator is north of the geographic equator, and the other is collected from the region whose geomagnetic equator is south of the geographic equator. The results show that the single-peaked brightness often appears between the geographic equator and the geomagnetic equator. The double-peaked brightness appears simultaneously on the two sides of the region sandwiched by the two equators. Coupled with the summer-to-winter neutral wind generated by seasonal effects, one side of brightness could be enhanced or disappear due to the plasma moving along the field line. The no-peak events mainly occur close to May–July, which may be due to the effect of ionospheric annual anomalies. Overall, the statistical results for the occurrence rate show strong seasonal variations with different cycles at different longitudinal regions for all three types of events. Graphical Abstract Article in Journal/Newspaper sami Directory of Open Access Journals: DOAJ Articles Earth, Planets and Space 74 1
institution Open Polar
collection Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
topic Midnight temperature maximum
ISUAL
630.0 nm
SAMI-2
Airglow
Geography. Anthropology. Recreation
G
Geodesy
QB275-343
Geology
QE1-996.5
spellingShingle Midnight temperature maximum
ISUAL
630.0 nm
SAMI-2
Airglow
Geography. Anthropology. Recreation
G
Geodesy
QB275-343
Geology
QE1-996.5
Chih-Yu Chiang
Tzu-Fang Chang
Sunny W. Y. Tam
Enhancement of equatorial OI(1D) emissions at midnight
topic_facet Midnight temperature maximum
ISUAL
630.0 nm
SAMI-2
Airglow
Geography. Anthropology. Recreation
G
Geodesy
QB275-343
Geology
QE1-996.5
description Abstract A number of recent studies have highlighted observational evidence of midnight brightness of the 630.0 nm nightglow, which is usually related to the midnight temperature maximum (MTM) effect. In this report, MTM-related enhancements of the 630.0 nm airglow around midnight are observed through images from the ISUAL/FORMOSAT-2 satellite. The data statistics are classified into three specific types (no-peak, single-peaked, and double-peaked events) and separated into the different seasons. In order to understand the influences of geomagnetic conditions, the statistical analyses are also separated into two regions. One is collected from the region whose geomagnetic equator is north of the geographic equator, and the other is collected from the region whose geomagnetic equator is south of the geographic equator. The results show that the single-peaked brightness often appears between the geographic equator and the geomagnetic equator. The double-peaked brightness appears simultaneously on the two sides of the region sandwiched by the two equators. Coupled with the summer-to-winter neutral wind generated by seasonal effects, one side of brightness could be enhanced or disappear due to the plasma moving along the field line. The no-peak events mainly occur close to May–July, which may be due to the effect of ionospheric annual anomalies. Overall, the statistical results for the occurrence rate show strong seasonal variations with different cycles at different longitudinal regions for all three types of events. Graphical Abstract
format Article in Journal/Newspaper
author Chih-Yu Chiang
Tzu-Fang Chang
Sunny W. Y. Tam
author_facet Chih-Yu Chiang
Tzu-Fang Chang
Sunny W. Y. Tam
author_sort Chih-Yu Chiang
title Enhancement of equatorial OI(1D) emissions at midnight
title_short Enhancement of equatorial OI(1D) emissions at midnight
title_full Enhancement of equatorial OI(1D) emissions at midnight
title_fullStr Enhancement of equatorial OI(1D) emissions at midnight
title_full_unstemmed Enhancement of equatorial OI(1D) emissions at midnight
title_sort enhancement of equatorial oi(1d) emissions at midnight
publisher SpringerOpen
publishDate 2022
url https://doi.org/10.1186/s40623-022-01596-4
https://doaj.org/article/20db9548f6ec4d8db7b941cee6ef386a
genre sami
genre_facet sami
op_source Earth, Planets and Space, Vol 74, Iss 1, Pp 1-13 (2022)
op_relation https://doi.org/10.1186/s40623-022-01596-4
https://doaj.org/toc/1880-5981
doi:10.1186/s40623-022-01596-4
1880-5981
https://doaj.org/article/20db9548f6ec4d8db7b941cee6ef386a
op_doi https://doi.org/10.1186/s40623-022-01596-4
container_title Earth, Planets and Space
container_volume 74
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