Geomagnetic control of polar mesosphere summer echoes

Using observations with the ALOMAR SOUSY radar near Andenes (69.3°N, 16.0°E) from 1994 until 1997 polar mesosphere summer echoes (PMSE) have been investigated in dependence on geomagnetic K indices derived at the Auroral Observatory Tromsø (69.66°N, 18.94°E). During night-time and morning hours a si...

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Published in:Annales Geophysicae
Main Authors: J. Bremer, P. Hoffmann, T. L. Hansen
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2000
Subjects:
Q
Online Access:https://doi.org/10.1007/s00585-000-0202-z
https://doaj.org/article/515384a156d940a38815f9e263ac8023
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spelling ftdoajarticles:oai:doaj.org/article:515384a156d940a38815f9e263ac8023 2023-05-15T13:25:17+02:00 Geomagnetic control of polar mesosphere summer echoes J. Bremer P. Hoffmann T. L. Hansen 2000-02-01T00:00:00Z https://doi.org/10.1007/s00585-000-0202-z https://doaj.org/article/515384a156d940a38815f9e263ac8023 EN eng Copernicus Publications https://www.ann-geophys.net/18/202/2000/angeo-18-202-2000.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576 doi:10.1007/s00585-000-0202-z 0992-7689 1432-0576 https://doaj.org/article/515384a156d940a38815f9e263ac8023 Annales Geophysicae, Vol 18, Pp 202-208 (2000) Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 article 2000 ftdoajarticles https://doi.org/10.1007/s00585-000-0202-z 2022-12-31T14:10:18Z Using observations with the ALOMAR SOUSY radar near Andenes (69.3°N, 16.0°E) from 1994 until 1997 polar mesosphere summer echoes (PMSE) have been investigated in dependence on geomagnetic K indices derived at the Auroral Observatory Tromsø (69.66°N, 18.94°E). During night-time and morning hours a significant correlation between the signal-to-noise ratio (SNR) of the radar results and the geomagnetic K indices could be detected with a maximum correlation near midnight. The correlation becomes markedly smaller in the afternoon and early evening hours with a minimum near 17 UT. This diurnal variation is in reasonable agreement with riometer absorption at Ivalo (68.55°N, 27.28°E) and can be explained by the diurnal variation of ionization due to precipitating high energetic particles. Therefore, a part of the diurnal PMSE variation is caused by this particle precipitation. The variability of the solar EUV variation, however, has no significant influence on the PMSE during the observation period. Keywords: Ionosphere (auroral ionosphere) - Magnetospheric physics (energetic particles, precipitating) - Radio science (remote sensing) Article in Journal/Newspaper Andenes Tromsø Directory of Open Access Journals: DOAJ Articles Tromsø Alomar ENVELOPE(-67.083,-67.083,-68.133,-68.133) Ivalo ENVELOPE(27.543,27.543,68.651,68.651) Annales Geophysicae 18 2 202 208
institution Open Polar
collection Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
topic Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
spellingShingle Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
J. Bremer
P. Hoffmann
T. L. Hansen
Geomagnetic control of polar mesosphere summer echoes
topic_facet Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
description Using observations with the ALOMAR SOUSY radar near Andenes (69.3°N, 16.0°E) from 1994 until 1997 polar mesosphere summer echoes (PMSE) have been investigated in dependence on geomagnetic K indices derived at the Auroral Observatory Tromsø (69.66°N, 18.94°E). During night-time and morning hours a significant correlation between the signal-to-noise ratio (SNR) of the radar results and the geomagnetic K indices could be detected with a maximum correlation near midnight. The correlation becomes markedly smaller in the afternoon and early evening hours with a minimum near 17 UT. This diurnal variation is in reasonable agreement with riometer absorption at Ivalo (68.55°N, 27.28°E) and can be explained by the diurnal variation of ionization due to precipitating high energetic particles. Therefore, a part of the diurnal PMSE variation is caused by this particle precipitation. The variability of the solar EUV variation, however, has no significant influence on the PMSE during the observation period. Keywords: Ionosphere (auroral ionosphere) - Magnetospheric physics (energetic particles, precipitating) - Radio science (remote sensing)
format Article in Journal/Newspaper
author J. Bremer
P. Hoffmann
T. L. Hansen
author_facet J. Bremer
P. Hoffmann
T. L. Hansen
author_sort J. Bremer
title Geomagnetic control of polar mesosphere summer echoes
title_short Geomagnetic control of polar mesosphere summer echoes
title_full Geomagnetic control of polar mesosphere summer echoes
title_fullStr Geomagnetic control of polar mesosphere summer echoes
title_full_unstemmed Geomagnetic control of polar mesosphere summer echoes
title_sort geomagnetic control of polar mesosphere summer echoes
publisher Copernicus Publications
publishDate 2000
url https://doi.org/10.1007/s00585-000-0202-z
https://doaj.org/article/515384a156d940a38815f9e263ac8023
long_lat ENVELOPE(-67.083,-67.083,-68.133,-68.133)
ENVELOPE(27.543,27.543,68.651,68.651)
geographic Tromsø
Alomar
Ivalo
geographic_facet Tromsø
Alomar
Ivalo
genre Andenes
Tromsø
genre_facet Andenes
Tromsø
op_source Annales Geophysicae, Vol 18, Pp 202-208 (2000)
op_relation https://www.ann-geophys.net/18/202/2000/angeo-18-202-2000.pdf
https://doaj.org/toc/0992-7689
https://doaj.org/toc/1432-0576
doi:10.1007/s00585-000-0202-z
0992-7689
1432-0576
https://doaj.org/article/515384a156d940a38815f9e263ac8023
op_doi https://doi.org/10.1007/s00585-000-0202-z
container_title Annales Geophysicae
container_volume 18
container_issue 2
container_start_page 202
op_container_end_page 208
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