An investigation of polar substorms observed at Halley Bay, Antarctica ...

Ground observations of magnetic and ionospheric substorms are reviewed, and the processes involved are explained. Then magnetic and absorption results from an auroral zone station, Halley Bay, are examined. Positive H bays occur in the evening sector between 16.00 and 22.00 local time while negative...

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Main Author: Boteler, David H.
Format: Text
Language:English
Published: University of British Columbia 2010
Subjects:
Online Access:https://dx.doi.org/10.14288/1.0053464
https://doi.library.ubc.ca/10.14288/1.0053464
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spelling ftdatacite:10.14288/1.0053464 2024-04-28T07:55:53+00:00 An investigation of polar substorms observed at Halley Bay, Antarctica ... Boteler, David H. 2010 https://dx.doi.org/10.14288/1.0053464 https://doi.library.ubc.ca/10.14288/1.0053464 en eng University of British Columbia article-journal Text ScholarlyArticle 2010 ftdatacite https://doi.org/10.14288/1.0053464 2024-04-02T09:36:37Z Ground observations of magnetic and ionospheric substorms are reviewed, and the processes involved are explained. Then magnetic and absorption results from an auroral zone station, Halley Bay, are examined. Positive H bays occur in the evening sector between 16.00 and 22.00 local time while negative H bays occur on the nightside between 22.00 and 06.00 local time. Clockwise and counterclockwise rotating Pi2 pulsations respectively have similar times of occurrence, as do westward and eastward moving radio aurora. Short-period absorption occurs coincident with magnetic bays while longer-period absorption occurs on the dayside (04.00 to 20.00 local time). This information is used to determine the disturbance pattern in local time seen at auroral zone stations. A simple model is presented to illustrate the processes responsible for the effects observed in the 3 different local-time zones. On the nightside there is direct injection of particles from the tail, into the ionosphere, accompanied by short-circuiting ... Text Antarc* Antarctica DataCite Metadata Store (German National Library of Science and Technology)
institution Open Polar
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description Ground observations of magnetic and ionospheric substorms are reviewed, and the processes involved are explained. Then magnetic and absorption results from an auroral zone station, Halley Bay, are examined. Positive H bays occur in the evening sector between 16.00 and 22.00 local time while negative H bays occur on the nightside between 22.00 and 06.00 local time. Clockwise and counterclockwise rotating Pi2 pulsations respectively have similar times of occurrence, as do westward and eastward moving radio aurora. Short-period absorption occurs coincident with magnetic bays while longer-period absorption occurs on the dayside (04.00 to 20.00 local time). This information is used to determine the disturbance pattern in local time seen at auroral zone stations. A simple model is presented to illustrate the processes responsible for the effects observed in the 3 different local-time zones. On the nightside there is direct injection of particles from the tail, into the ionosphere, accompanied by short-circuiting ...
format Text
author Boteler, David H.
spellingShingle Boteler, David H.
An investigation of polar substorms observed at Halley Bay, Antarctica ...
author_facet Boteler, David H.
author_sort Boteler, David H.
title An investigation of polar substorms observed at Halley Bay, Antarctica ...
title_short An investigation of polar substorms observed at Halley Bay, Antarctica ...
title_full An investigation of polar substorms observed at Halley Bay, Antarctica ...
title_fullStr An investigation of polar substorms observed at Halley Bay, Antarctica ...
title_full_unstemmed An investigation of polar substorms observed at Halley Bay, Antarctica ...
title_sort investigation of polar substorms observed at halley bay, antarctica ...
publisher University of British Columbia
publishDate 2010
url https://dx.doi.org/10.14288/1.0053464
https://doi.library.ubc.ca/10.14288/1.0053464
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Antarctica
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Antarctica
op_doi https://doi.org/10.14288/1.0053464
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