Winter nighttime ion temperatures and energetic electrons from OGO 6 plasma measurements
In the reported investigation, ion temperature and suprathermal electron flux data were acquired with the retarding potential analyzer on board the OGO 6 satellite when it was in solar eclipse. Attention is given to measurements in the 400- to 800-km height interval between midnight and predawn in t...
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ftnasantrs:oai:casi.ntrs.nasa.gov:19810050980 2023-05-15T17:32:12+02:00 Winter nighttime ion temperatures and energetic electrons from OGO 6 plasma measurements Sanatani, S. Breig, E. L. Unclassified, Unlimited, Publicly available May 1, 1981 http://ntrs.nasa.gov/search.jsp?R=19810050980 unknown http://ntrs.nasa.gov/search.jsp?R=19810050980 Accession ID: 81A35384 Copyright Other Sources 46 Journal of Geophysical Research; 86; May 1 1981 ftnasantrs 2012-02-15T14:40:47Z In the reported investigation, ion temperature and suprathermal electron flux data were acquired with the retarding potential analyzer on board the OGO 6 satellite when it was in solar eclipse. Attention is given to measurements in the 400- to 800-km height interval between midnight and predawn in the northern winter nonpolar ionosphere. Statistical analysis of data recorded during a 1 month time span permits a decoupling of horizontal and altitude effects. A distinct longitudinal variation is observed for ion temperature above 500 km, with a significant relative enhancement over the western North Atlantic. Altitude distributions of ion temperature are compatible with Millstone Hill profiles within the common region of this enhancement. Large fluxes of energetic electrons are observed and extend to much lower geomagnetic latitudes in the same longitude sector. Other/Unknown Material North Atlantic NASA Technical Reports Server (NTRS) |
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46 Sanatani, S. Breig, E. L. Winter nighttime ion temperatures and energetic electrons from OGO 6 plasma measurements |
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46 |
description |
In the reported investigation, ion temperature and suprathermal electron flux data were acquired with the retarding potential analyzer on board the OGO 6 satellite when it was in solar eclipse. Attention is given to measurements in the 400- to 800-km height interval between midnight and predawn in the northern winter nonpolar ionosphere. Statistical analysis of data recorded during a 1 month time span permits a decoupling of horizontal and altitude effects. A distinct longitudinal variation is observed for ion temperature above 500 km, with a significant relative enhancement over the western North Atlantic. Altitude distributions of ion temperature are compatible with Millstone Hill profiles within the common region of this enhancement. Large fluxes of energetic electrons are observed and extend to much lower geomagnetic latitudes in the same longitude sector. |
format |
Other/Unknown Material |
author |
Sanatani, S. Breig, E. L. |
author_facet |
Sanatani, S. Breig, E. L. |
author_sort |
Sanatani, S. |
title |
Winter nighttime ion temperatures and energetic electrons from OGO 6 plasma measurements |
title_short |
Winter nighttime ion temperatures and energetic electrons from OGO 6 plasma measurements |
title_full |
Winter nighttime ion temperatures and energetic electrons from OGO 6 plasma measurements |
title_fullStr |
Winter nighttime ion temperatures and energetic electrons from OGO 6 plasma measurements |
title_full_unstemmed |
Winter nighttime ion temperatures and energetic electrons from OGO 6 plasma measurements |
title_sort |
winter nighttime ion temperatures and energetic electrons from ogo 6 plasma measurements |
publishDate |
1981 |
url |
http://ntrs.nasa.gov/search.jsp?R=19810050980 |
op_coverage |
Unclassified, Unlimited, Publicly available |
genre |
North Atlantic |
genre_facet |
North Atlantic |
op_source |
Other Sources |
op_relation |
http://ntrs.nasa.gov/search.jsp?R=19810050980 Accession ID: 81A35384 |
op_rights |
Copyright |
_version_ |
1766130188710576128 |