Are variations in PMSE intensity affected by energetic particle precipitation?
The correlation between variations in Polar Mesosphere Summer Echoes (PMSE) and variations in energetic particle precipitation is examined. PMSE were observed by the Esrange VHF MST Radar (ESRAD) at 67°53' N, 21°06' E. The 30 MHz riometer in Abisko (68°24' N, 18°54' E) registered...
Published in: | Annales Geophysicae |
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Main Authors: | , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
Copernicus Publications
2002
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Subjects: | |
Online Access: | https://doi.org/10.5194/angeo-20-539-2002 https://doaj.org/article/e8b028b1f1324d60aa156701fc073e8a |
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author | V. Barabash S. Kirkwood P. B. Chilson |
author_facet | V. Barabash S. Kirkwood P. B. Chilson |
author_sort | V. Barabash |
collection | Directory of Open Access Journals: DOAJ Articles |
container_issue | 4 |
container_start_page | 539 |
container_title | Annales Geophysicae |
container_volume | 20 |
description | The correlation between variations in Polar Mesosphere Summer Echoes (PMSE) and variations in energetic particle precipitation is examined. PMSE were observed by the Esrange VHF MST Radar (ESRAD) at 67°53' N, 21°06' E. The 30 MHz riometer in Abisko (68°24' N, 18°54' E) registered radio wave absorption caused by ionization changes in response to energetic particle precipitation. The relationship between the linear PMSE intensity and the square of absorption has been estimated using the Pearson linear correlation and the Spearman rank correlation. The mean diurnal variation of the square of absorption and the linear PMSE intensity are highly correlated. However, their day-to-day variations show significant correlation only during the late evening hours. The correlation in late evening does not exceed 0.6. This indicates that varying ionization cannot be considered as a primary source of varying PMSE, and the high correlation found when mean diurnal variations are compared is likely a by-product of daily variations caused by other factors. Key words. Ionosphere (particle precipitation) Magnetospheric physics (energetic particles, precipitating) Meteorology and atmospheric dynamics (precipitation) |
format | Article in Journal/Newspaper |
genre | Abisko |
genre_facet | Abisko |
geographic | Abisko Esrange |
geographic_facet | Abisko Esrange |
id | ftdoajarticles:oai:doaj.org/article:e8b028b1f1324d60aa156701fc073e8a |
institution | Open Polar |
language | English |
long_lat | ENVELOPE(18.829,18.829,68.349,68.349) ENVELOPE(21.117,21.117,67.883,67.883) |
op_collection_id | ftdoajarticles |
op_container_end_page | 545 |
op_doi | https://doi.org/10.5194/angeo-20-539-2002 |
op_relation | https://www.ann-geophys.net/20/539/2002/angeo-20-539-2002.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576 doi:10.5194/angeo-20-539-2002 0992-7689 1432-0576 https://doaj.org/article/e8b028b1f1324d60aa156701fc073e8a |
op_source | Annales Geophysicae, Vol 20, Pp 539-545 (2002) |
publishDate | 2002 |
publisher | Copernicus Publications |
record_format | openpolar |
spelling | ftdoajarticles:oai:doaj.org/article:e8b028b1f1324d60aa156701fc073e8a 2025-01-16T18:31:54+00:00 Are variations in PMSE intensity affected by energetic particle precipitation? V. Barabash S. Kirkwood P. B. Chilson 2002-04-01T00:00:00Z https://doi.org/10.5194/angeo-20-539-2002 https://doaj.org/article/e8b028b1f1324d60aa156701fc073e8a EN eng Copernicus Publications https://www.ann-geophys.net/20/539/2002/angeo-20-539-2002.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576 doi:10.5194/angeo-20-539-2002 0992-7689 1432-0576 https://doaj.org/article/e8b028b1f1324d60aa156701fc073e8a Annales Geophysicae, Vol 20, Pp 539-545 (2002) Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 article 2002 ftdoajarticles https://doi.org/10.5194/angeo-20-539-2002 2022-12-31T01:21:56Z The correlation between variations in Polar Mesosphere Summer Echoes (PMSE) and variations in energetic particle precipitation is examined. PMSE were observed by the Esrange VHF MST Radar (ESRAD) at 67°53' N, 21°06' E. The 30 MHz riometer in Abisko (68°24' N, 18°54' E) registered radio wave absorption caused by ionization changes in response to energetic particle precipitation. The relationship between the linear PMSE intensity and the square of absorption has been estimated using the Pearson linear correlation and the Spearman rank correlation. The mean diurnal variation of the square of absorption and the linear PMSE intensity are highly correlated. However, their day-to-day variations show significant correlation only during the late evening hours. The correlation in late evening does not exceed 0.6. This indicates that varying ionization cannot be considered as a primary source of varying PMSE, and the high correlation found when mean diurnal variations are compared is likely a by-product of daily variations caused by other factors. Key words. Ionosphere (particle precipitation) Magnetospheric physics (energetic particles, precipitating) Meteorology and atmospheric dynamics (precipitation) Article in Journal/Newspaper Abisko Directory of Open Access Journals: DOAJ Articles Abisko ENVELOPE(18.829,18.829,68.349,68.349) Esrange ENVELOPE(21.117,21.117,67.883,67.883) Annales Geophysicae 20 4 539 545 |
spellingShingle | Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 V. Barabash S. Kirkwood P. B. Chilson Are variations in PMSE intensity affected by energetic particle precipitation? |
title | Are variations in PMSE intensity affected by energetic particle precipitation? |
title_full | Are variations in PMSE intensity affected by energetic particle precipitation? |
title_fullStr | Are variations in PMSE intensity affected by energetic particle precipitation? |
title_full_unstemmed | Are variations in PMSE intensity affected by energetic particle precipitation? |
title_short | Are variations in PMSE intensity affected by energetic particle precipitation? |
title_sort | are variations in pmse intensity affected by energetic particle precipitation? |
topic | Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 |
topic_facet | Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 |
url | https://doi.org/10.5194/angeo-20-539-2002 https://doaj.org/article/e8b028b1f1324d60aa156701fc073e8a |