Longitudinal Structure in the Altitude of the Sporadic E Observed by COSMIC in Low-Latitudes

The longitudinal structure in the altitude of the Sporadic E (Es) was investigated for the first time based on the S4 index provided by the Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) in low latitudes. The longitudinal structure is identified as a symmetrically l...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Zhendi Liu, Qingfeng Li, Hanxian Fang, Ze Gao
Formato: article
Lenguaje:EN
Publicado: MDPI AG 2021
Materias:
Q
Acceso en línea:https://doaj.org/article/4c2c3c9fb808436c9ac9f727d18b71ad
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
id oai:doaj.org-article:4c2c3c9fb808436c9ac9f727d18b71ad
record_format dspace
spelling oai:doaj.org-article:4c2c3c9fb808436c9ac9f727d18b71ad2021-11-25T18:55:41ZLongitudinal Structure in the Altitude of the Sporadic E Observed by COSMIC in Low-Latitudes10.3390/rs132247142072-4292https://doaj.org/article/4c2c3c9fb808436c9ac9f727d18b71ad2021-11-01T00:00:00Zhttps://www.mdpi.com/2072-4292/13/22/4714https://doaj.org/toc/2072-4292The longitudinal structure in the altitude of the Sporadic E (Es) was investigated for the first time based on the S4 index provided by the Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) in low latitudes. The longitudinal structure is identified as a symmetrically located wavenumber-4 (WN4) pattern within 30°S–30°N. The WN4 occurs primarily during the daytime at the June solstice and equinoxes, with the largest amplitude at the September equinox and the smallest one at the March equinox. It moves eastward with a speed of ~90°/day. The strongest WN4 appears within 10–20°N and 5–15°S in the Northern and Southern hemispheres, respectively. At the June solstice and the September equinox, the WN4 is stronger in the Northern hemisphere than in the Southern hemisphere, while the situation is reversed at the March equinox. The altitude distribution of the convergence null in the diurnal eastward non-migrating tide with zonal wavenumber-3 (DE3) for the zonal wind is similar to that of the WN4. This and other similar features, such as the seasonal variation, eastward speed, and the symmetrical locations, support the dominant role of the DE3 tide for the formation of the WN4 structure.Zhendi LiuQingfeng LiHanxian FangZe GaoMDPI AGarticlesporadic Elongitudinal structurewind shearnon-migrating tidewavenumber-4 (WN4)ScienceQENRemote Sensing, Vol 13, Iss 4714, p 4714 (2021)
institution DOAJ
collection DOAJ
language EN
topic sporadic E
longitudinal structure
wind shear
non-migrating tide
wavenumber-4 (WN4)
Science
Q
spellingShingle sporadic E
longitudinal structure
wind shear
non-migrating tide
wavenumber-4 (WN4)
Science
Q
Zhendi Liu
Qingfeng Li
Hanxian Fang
Ze Gao
Longitudinal Structure in the Altitude of the Sporadic E Observed by COSMIC in Low-Latitudes
description The longitudinal structure in the altitude of the Sporadic E (Es) was investigated for the first time based on the S4 index provided by the Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) in low latitudes. The longitudinal structure is identified as a symmetrically located wavenumber-4 (WN4) pattern within 30°S–30°N. The WN4 occurs primarily during the daytime at the June solstice and equinoxes, with the largest amplitude at the September equinox and the smallest one at the March equinox. It moves eastward with a speed of ~90°/day. The strongest WN4 appears within 10–20°N and 5–15°S in the Northern and Southern hemispheres, respectively. At the June solstice and the September equinox, the WN4 is stronger in the Northern hemisphere than in the Southern hemisphere, while the situation is reversed at the March equinox. The altitude distribution of the convergence null in the diurnal eastward non-migrating tide with zonal wavenumber-3 (DE3) for the zonal wind is similar to that of the WN4. This and other similar features, such as the seasonal variation, eastward speed, and the symmetrical locations, support the dominant role of the DE3 tide for the formation of the WN4 structure.
format article
author Zhendi Liu
Qingfeng Li
Hanxian Fang
Ze Gao
author_facet Zhendi Liu
Qingfeng Li
Hanxian Fang
Ze Gao
author_sort Zhendi Liu
title Longitudinal Structure in the Altitude of the Sporadic E Observed by COSMIC in Low-Latitudes
title_short Longitudinal Structure in the Altitude of the Sporadic E Observed by COSMIC in Low-Latitudes
title_full Longitudinal Structure in the Altitude of the Sporadic E Observed by COSMIC in Low-Latitudes
title_fullStr Longitudinal Structure in the Altitude of the Sporadic E Observed by COSMIC in Low-Latitudes
title_full_unstemmed Longitudinal Structure in the Altitude of the Sporadic E Observed by COSMIC in Low-Latitudes
title_sort longitudinal structure in the altitude of the sporadic e observed by cosmic in low-latitudes
publisher MDPI AG
publishDate 2021
url https://doaj.org/article/4c2c3c9fb808436c9ac9f727d18b71ad
work_keys_str_mv AT zhendiliu longitudinalstructureinthealtitudeofthesporadiceobservedbycosmicinlowlatitudes
AT qingfengli longitudinalstructureinthealtitudeofthesporadiceobservedbycosmicinlowlatitudes
AT hanxianfang longitudinalstructureinthealtitudeofthesporadiceobservedbycosmicinlowlatitudes
AT zegao longitudinalstructureinthealtitudeofthesporadiceobservedbycosmicinlowlatitudes
_version_ 1718410522147160064