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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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 |