Cosmic radio noise absorption events associated with equatorward drifting arcs during a substorm growth phase
Cosmic radio noise absorption (CNA) events associated with equatorward drifting arcs during a substorm growth phase are studied by using simultaneous optical auroral, IRIS imaging riometer and EISCAT incoherent scatter radar measurements. The CNA is generally attributed to energetic particle precipi...
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ftdoajarticles:oai:doaj.org/article:a15260aeb5b54cb5990cf57122d454ba 2023-05-15T16:04:46+02:00 Cosmic radio noise absorption events associated with equatorward drifting arcs during a substorm growth phase J. R. T. Jussila A. T. Aikio S. Shalimov S. R. Marple 2004-04-01T00:00:00Z https://doi.org/10.5194/angeo-22-1675-2004 https://doaj.org/article/a15260aeb5b54cb5990cf57122d454ba EN eng Copernicus Publications https://www.ann-geophys.net/22/1675/2004/angeo-22-1675-2004.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576 doi:10.5194/angeo-22-1675-2004 0992-7689 1432-0576 https://doaj.org/article/a15260aeb5b54cb5990cf57122d454ba Annales Geophysicae, Vol 22, Pp 1675-1686 (2004) Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 article 2004 ftdoajarticles https://doi.org/10.5194/angeo-22-1675-2004 2022-12-31T00:36:44Z Cosmic radio noise absorption (CNA) events associated with equatorward drifting arcs during a substorm growth phase are studied by using simultaneous optical auroral, IRIS imaging riometer and EISCAT incoherent scatter radar measurements. The CNA is generally attributed to energetic particle precipitation in the D-region. However, it has been argued that plasma irregularities or enhanced electron temperature ( T e ) in the E-region could also produce CNA. Both of the latter mechanisms are related to intense electric fields in the ionosphere. We present two events which occur during a substorm growth phase in the evening MLT sector. In both of the events, an auroral arc is drifting equatorward, together with a region of CNA (auroral absorption bay) located on the equatorward side and outside of the arc. Both of the events are associated with enhanced D-region electron density on the equatorward side of the auroral arc, but in the second event, a region of intense electric field and enhanced electron temperature in the E-region is also located on the equatorward side of the arc. We show that in the studied events neither plasma instabilities nor enhanced T e play a significant role in producing the measured CNA, but the CNA in the vicinity of the equatorward drifting arcs is produced by D-region energetic electron precipitation. Key words. Ionosphere (auroral ionosphere; particle precipitation; electric fields and currents) Article in Journal/Newspaper EISCAT Directory of Open Access Journals: DOAJ Articles Annales Geophysicae 22 5 1675 1686 |
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Open Polar |
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Directory of Open Access Journals: DOAJ Articles |
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English |
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Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 |
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Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 J. R. T. Jussila A. T. Aikio S. Shalimov S. R. Marple Cosmic radio noise absorption events associated with equatorward drifting arcs during a substorm growth phase |
topic_facet |
Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 |
description |
Cosmic radio noise absorption (CNA) events associated with equatorward drifting arcs during a substorm growth phase are studied by using simultaneous optical auroral, IRIS imaging riometer and EISCAT incoherent scatter radar measurements. The CNA is generally attributed to energetic particle precipitation in the D-region. However, it has been argued that plasma irregularities or enhanced electron temperature ( T e ) in the E-region could also produce CNA. Both of the latter mechanisms are related to intense electric fields in the ionosphere. We present two events which occur during a substorm growth phase in the evening MLT sector. In both of the events, an auroral arc is drifting equatorward, together with a region of CNA (auroral absorption bay) located on the equatorward side and outside of the arc. Both of the events are associated with enhanced D-region electron density on the equatorward side of the auroral arc, but in the second event, a region of intense electric field and enhanced electron temperature in the E-region is also located on the equatorward side of the arc. We show that in the studied events neither plasma instabilities nor enhanced T e play a significant role in producing the measured CNA, but the CNA in the vicinity of the equatorward drifting arcs is produced by D-region energetic electron precipitation. Key words. Ionosphere (auroral ionosphere; particle precipitation; electric fields and currents) |
format |
Article in Journal/Newspaper |
author |
J. R. T. Jussila A. T. Aikio S. Shalimov S. R. Marple |
author_facet |
J. R. T. Jussila A. T. Aikio S. Shalimov S. R. Marple |
author_sort |
J. R. T. Jussila |
title |
Cosmic radio noise absorption events associated with equatorward drifting arcs during a substorm growth phase |
title_short |
Cosmic radio noise absorption events associated with equatorward drifting arcs during a substorm growth phase |
title_full |
Cosmic radio noise absorption events associated with equatorward drifting arcs during a substorm growth phase |
title_fullStr |
Cosmic radio noise absorption events associated with equatorward drifting arcs during a substorm growth phase |
title_full_unstemmed |
Cosmic radio noise absorption events associated with equatorward drifting arcs during a substorm growth phase |
title_sort |
cosmic radio noise absorption events associated with equatorward drifting arcs during a substorm growth phase |
publisher |
Copernicus Publications |
publishDate |
2004 |
url |
https://doi.org/10.5194/angeo-22-1675-2004 https://doaj.org/article/a15260aeb5b54cb5990cf57122d454ba |
genre |
EISCAT |
genre_facet |
EISCAT |
op_source |
Annales Geophysicae, Vol 22, Pp 1675-1686 (2004) |
op_relation |
https://www.ann-geophys.net/22/1675/2004/angeo-22-1675-2004.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576 doi:10.5194/angeo-22-1675-2004 0992-7689 1432-0576 https://doaj.org/article/a15260aeb5b54cb5990cf57122d454ba |
op_doi |
https://doi.org/10.5194/angeo-22-1675-2004 |
container_title |
Annales Geophysicae |
container_volume |
22 |
container_issue |
5 |
container_start_page |
1675 |
op_container_end_page |
1686 |
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1766400400103047168 |