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 Observa- tory Tromsù (69.66°N, 18.94°E). During night-time and morning hours a...

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Main Authors: Bremer, J., Hansen, T.L., Hoffmann, P.
Format: Article in Journal/Newspaper
Language:English
Published: European Geophysical Society 2000
Subjects:
Online Access:https://hdl.handle.net/10037/558
id ftunivtroemsoe:oai:munin.uit.no:10037/558
record_format openpolar
spelling ftunivtroemsoe:oai:munin.uit.no:10037/558 2024-06-02T07:55:06+00:00 Geomagnetic control of polar mesosphere summer echoes. Bremer, J. Hansen, T.L. Hoffmann, P. 2000 180462 bytes application/pdf https://hdl.handle.net/10037/558 eng eng European Geophysical Society Annales Geophysicae 18(2000), pp 202-208 1432-0576 (elektronisk) https://hdl.handle.net/10037/558 URN:NBN:no-uit_munin_385 openAccess ionosphere auroral ionosphere Magnetospheric physics energetic particles precipitating radio science remote sensing VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme akustikk optikk: 434 VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437 Journal article Tidsskriftartikkel 2000 ftunivtroemsoe 2024-05-07T08:40:37Z 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 Observa- tory Tromsù (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 maxi- mum correlation near midnight. The correlation be- comes 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 varia- tion, however, has no significant influence on the PMSE during the observation period. Article in Journal/Newspaper Andenes University of Tromsø: Munin Open Research Archive Alomar ENVELOPE(-67.083,-67.083,-68.133,-68.133) Ivalo ENVELOPE(27.543,27.543,68.651,68.651)
institution Open Polar
collection University of Tromsø: Munin Open Research Archive
op_collection_id ftunivtroemsoe
language English
topic ionosphere
auroral ionosphere
Magnetospheric physics
energetic particles
precipitating
radio science
remote sensing
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
spellingShingle ionosphere
auroral ionosphere
Magnetospheric physics
energetic particles
precipitating
radio science
remote sensing
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
Bremer, J.
Hansen, T.L.
Hoffmann, P.
Geomagnetic control of polar mesosphere summer echoes.
topic_facet ionosphere
auroral ionosphere
Magnetospheric physics
energetic particles
precipitating
radio science
remote sensing
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
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 Observa- tory Tromsù (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 maxi- mum correlation near midnight. The correlation be- comes 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 varia- tion, however, has no significant influence on the PMSE during the observation period.
format Article in Journal/Newspaper
author Bremer, J.
Hansen, T.L.
Hoffmann, P.
author_facet Bremer, J.
Hansen, T.L.
Hoffmann, P.
author_sort Bremer, J.
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 European Geophysical Society
publishDate 2000
url https://hdl.handle.net/10037/558
long_lat ENVELOPE(-67.083,-67.083,-68.133,-68.133)
ENVELOPE(27.543,27.543,68.651,68.651)
geographic Alomar
Ivalo
geographic_facet Alomar
Ivalo
genre Andenes
genre_facet Andenes
op_relation Annales Geophysicae 18(2000), pp 202-208
1432-0576 (elektronisk)
https://hdl.handle.net/10037/558
URN:NBN:no-uit_munin_385
op_rights openAccess
_version_ 1800745501192093696