Polar Mesospheric Summer Echo Characteristics in Magnetic Local Time and Height Profiles

We conducted a statistical study of polar mesospheric summer echoes (PMSEs) in relation to magnetic local time (MLT), considering the geomagnetic conditions using the K-index (or K). Additionally, we performed a case study to examine the velocity profile, specifically for high velocities (≥ ~100 m...

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Main Authors: Young-Sook Lee, Ram Singh, Geonhwa Jee, Young-Sil Kwak, Yong Ha Kim
Format: Article
Language:English
Published: The Korean Space Science Society 2023-09-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:https://www.janss.kr/archive/view_article?pid=jass-40-3-101
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author Young-Sook Lee
Ram Singh
Geonhwa Jee
Young-Sil Kwak
Yong Ha Kim
author_facet Young-Sook Lee
Ram Singh
Geonhwa Jee
Young-Sil Kwak
Yong Ha Kim
author_sort Young-Sook Lee
collection DOAJ
description We conducted a statistical study of polar mesospheric summer echoes (PMSEs) in relation to magnetic local time (MLT), considering the geomagnetic conditions using the K-index (or K). Additionally, we performed a case study to examine the velocity profile, specifically for high velocities (≥ ~100 m/s) varying with high temporal resolution at high K-index values. This study utilized the PMSE data obtained from the mesosphere–stratosphere–troposphere radar located in Esrange, Sweden (63.7°N, 21°E). The change in K-index in terms of MLT was high (K ≥ 4) from 23 to 04 MLT, estimated for the time PMSE was present. During the near-midnight period (0–4 MLT), both PMSE occurrence and signal-to-noise ratio (SNR) displayed an asymmetric structure with upper curves for K ≥ 3 and lower curves for K < 3. Furthermore, the occurrence of high velocities peaked at 3–4 MLT for K ≥ 3. From case studies focusing on the 0–3 MLT period, we observed persistent eastward-biased high velocities (≥ 200 m/s) prevailing for ~18 min. These high velocities were accompanied with the systematic motion of profiles at 85–88 km, including large shear formation. Importantly, the rapid variations observed in velocity could not be attributed to neutral wind effects. The present findings suggest a strong substorm influence on PMSE, especially in the midnight and early dawn sectors. The large zonal drift observed in PMSE were potentially energized by local electromagnetic fields or the global convection field induced by the electron precipitation during substorms.
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spelling doaj.art-15be50b3f35548bbbce7e4add1aeac502024-02-03T11:07:58ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092023-09-0140310111110.5140/JASS.2023.40.3.101Polar Mesospheric Summer Echo Characteristics in Magnetic Local Time and Height ProfilesYoung-Sook Lee0https://orcid.org/0000-0002-7746-9718Ram Singh1https://orcid.org/0000-0002-8140-3500Geonhwa Jee2https://orcid.org/0000-0001-7996-0482Young-Sil Kwak3https://orcid.org/0000-0003-3375-8574Yong Ha Kim4https://orcid.org/0000-0003-0200-9423Department of Astronomy and Space Science, Chungnam National University, Daejeon 34134, KoreaDepartment of Astronomy and Space Science, Chungnam National University, Daejeon 34134, KoreaKorea Polar Research Institute, Incheon 21990, KoreaKorea Astronomy and Space Science Institute, Daejeon 34055, KoreaChungnam National University, Daejeon 34134, KoreaWe conducted a statistical study of polar mesospheric summer echoes (PMSEs) in relation to magnetic local time (MLT), considering the geomagnetic conditions using the K-index (or K). Additionally, we performed a case study to examine the velocity profile, specifically for high velocities (≥ ~100 m/s) varying with high temporal resolution at high K-index values. This study utilized the PMSE data obtained from the mesosphere–stratosphere–troposphere radar located in Esrange, Sweden (63.7°N, 21°E). The change in K-index in terms of MLT was high (K ≥ 4) from 23 to 04 MLT, estimated for the time PMSE was present. During the near-midnight period (0–4 MLT), both PMSE occurrence and signal-to-noise ratio (SNR) displayed an asymmetric structure with upper curves for K ≥ 3 and lower curves for K < 3. Furthermore, the occurrence of high velocities peaked at 3–4 MLT for K ≥ 3. From case studies focusing on the 0–3 MLT period, we observed persistent eastward-biased high velocities (≥ 200 m/s) prevailing for ~18 min. These high velocities were accompanied with the systematic motion of profiles at 85–88 km, including large shear formation. Importantly, the rapid variations observed in velocity could not be attributed to neutral wind effects. The present findings suggest a strong substorm influence on PMSE, especially in the midnight and early dawn sectors. The large zonal drift observed in PMSE were potentially energized by local electromagnetic fields or the global convection field induced by the electron precipitation during substorms.https://www.janss.kr/archive/view_article?pid=jass-40-3-101polar mesospheric summer echo (pmse)substormsmagnetic local timezonal drift of polar mesospheric summer echoe (pmse)k-index
spellingShingle Young-Sook Lee
Ram Singh
Geonhwa Jee
Young-Sil Kwak
Yong Ha Kim
Polar Mesospheric Summer Echo Characteristics in Magnetic Local Time and Height Profiles
Journal of Astronomy and Space Sciences
polar mesospheric summer echo (pmse)
substorms
magnetic local time
zonal drift of polar mesospheric summer echoe (pmse)
k-index
title Polar Mesospheric Summer Echo Characteristics in Magnetic Local Time and Height Profiles
title_full Polar Mesospheric Summer Echo Characteristics in Magnetic Local Time and Height Profiles
title_fullStr Polar Mesospheric Summer Echo Characteristics in Magnetic Local Time and Height Profiles
title_full_unstemmed Polar Mesospheric Summer Echo Characteristics in Magnetic Local Time and Height Profiles
title_short Polar Mesospheric Summer Echo Characteristics in Magnetic Local Time and Height Profiles
title_sort polar mesospheric summer echo characteristics in magnetic local time and height profiles
topic polar mesospheric summer echo (pmse)
substorms
magnetic local time
zonal drift of polar mesospheric summer echoe (pmse)
k-index
url https://www.janss.kr/archive/view_article?pid=jass-40-3-101
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