Discrete polar cap aurora observed from Spitsbergen

ABSTRACT Discrete auroral arcs frequently bridge the polar cap connecting the morning and evening sectors of the auroral oval along the line of the transpolar (electron) current. Very high-latitude stations that lie wholly within the oval during the earth's diurnal rotation pass under this brid...

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Published in:Polar Record
Main Authors: Simmons, D.A.R., Henriksen, K.
Format: Article in Journal/Newspaper
Language:English
Published: Cambridge University Press (CUP) 1992
Subjects:
Online Access:http://dx.doi.org/10.1017/s0032247400020659
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0032247400020659
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spelling crcambridgeupr:10.1017/s0032247400020659 2024-03-03T08:48:21+00:00 Discrete polar cap aurora observed from Spitsbergen Simmons, D.A.R. Henriksen, K. 1992 http://dx.doi.org/10.1017/s0032247400020659 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0032247400020659 en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms Polar Record volume 28, issue 166, page 191-204 ISSN 0032-2474 1475-3057 General Earth and Planetary Sciences Ecology Geography, Planning and Development journal-article 1992 crcambridgeupr https://doi.org/10.1017/s0032247400020659 2024-02-08T08:33:42Z ABSTRACT Discrete auroral arcs frequently bridge the polar cap connecting the morning and evening sectors of the auroral oval along the line of the transpolar (electron) current. Very high-latitude stations that lie wholly within the oval during the earth's diurnal rotation pass under this bridge twice a day, giving morning and evening maxima. Stations at slightly lower latitudes on Spitsbergen lie within the oval in the evening but under, or even south of, the oval in the morning. From such stations the evening, but not the morning, maximum is readily observed. This study is primarily concerned with the orientation of discrete polar cap arcs in the evening skies over Spitsbergen. It shows that the geomagnetic alignment of these arcs is latitude-dependent between geomagnetic colatitudes 6 to 20°N. At the highest latitudes within this range, the arcs are in transpolar alignment, whereas at the lowest latitudes within the polar cap, they are oval-aligned. At intermediate latitudes, the arcs are observed in transitional phases between transpolar and ovalalignment. The solar alignment of discrete polar cap arcs is a function of corrected geomagnetic local time. In the early afternoon, solar alignment is poor but this gradually improves throughout the late afternoon until there is excellent alignment at the time of the evening maximum. Recent satellite studies of plasma convection in the polar ionosphere have helped to explain some of the visual characteristics of discrete polar cap aurora observed from Spitsbergen, particularly the irregular alignment of arcs in the region of the Harang discontinuity. Article in Journal/Newspaper Polar Record Spitsbergen Cambridge University Press Polar Record 28 166 191 204
institution Open Polar
collection Cambridge University Press
op_collection_id crcambridgeupr
language English
topic General Earth and Planetary Sciences
Ecology
Geography, Planning and Development
spellingShingle General Earth and Planetary Sciences
Ecology
Geography, Planning and Development
Simmons, D.A.R.
Henriksen, K.
Discrete polar cap aurora observed from Spitsbergen
topic_facet General Earth and Planetary Sciences
Ecology
Geography, Planning and Development
description ABSTRACT Discrete auroral arcs frequently bridge the polar cap connecting the morning and evening sectors of the auroral oval along the line of the transpolar (electron) current. Very high-latitude stations that lie wholly within the oval during the earth's diurnal rotation pass under this bridge twice a day, giving morning and evening maxima. Stations at slightly lower latitudes on Spitsbergen lie within the oval in the evening but under, or even south of, the oval in the morning. From such stations the evening, but not the morning, maximum is readily observed. This study is primarily concerned with the orientation of discrete polar cap arcs in the evening skies over Spitsbergen. It shows that the geomagnetic alignment of these arcs is latitude-dependent between geomagnetic colatitudes 6 to 20°N. At the highest latitudes within this range, the arcs are in transpolar alignment, whereas at the lowest latitudes within the polar cap, they are oval-aligned. At intermediate latitudes, the arcs are observed in transitional phases between transpolar and ovalalignment. The solar alignment of discrete polar cap arcs is a function of corrected geomagnetic local time. In the early afternoon, solar alignment is poor but this gradually improves throughout the late afternoon until there is excellent alignment at the time of the evening maximum. Recent satellite studies of plasma convection in the polar ionosphere have helped to explain some of the visual characteristics of discrete polar cap aurora observed from Spitsbergen, particularly the irregular alignment of arcs in the region of the Harang discontinuity.
format Article in Journal/Newspaper
author Simmons, D.A.R.
Henriksen, K.
author_facet Simmons, D.A.R.
Henriksen, K.
author_sort Simmons, D.A.R.
title Discrete polar cap aurora observed from Spitsbergen
title_short Discrete polar cap aurora observed from Spitsbergen
title_full Discrete polar cap aurora observed from Spitsbergen
title_fullStr Discrete polar cap aurora observed from Spitsbergen
title_full_unstemmed Discrete polar cap aurora observed from Spitsbergen
title_sort discrete polar cap aurora observed from spitsbergen
publisher Cambridge University Press (CUP)
publishDate 1992
url http://dx.doi.org/10.1017/s0032247400020659
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0032247400020659
genre Polar Record
Spitsbergen
genre_facet Polar Record
Spitsbergen
op_source Polar Record
volume 28, issue 166, page 191-204
ISSN 0032-2474 1475-3057
op_rights https://www.cambridge.org/core/terms
op_doi https://doi.org/10.1017/s0032247400020659
container_title Polar Record
container_volume 28
container_issue 166
container_start_page 191
op_container_end_page 204
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