author_facet Goodwin, L.
St.‐Maurice, J.‐P.
Richards, P.
Nicolls, M.
Hairston, M.
Goodwin, L.
St.‐Maurice, J.‐P.
Richards, P.
Nicolls, M.
Hairston, M.
author Goodwin, L.
St.‐Maurice, J.‐P.
Richards, P.
Nicolls, M.
Hairston, M.
spellingShingle Goodwin, L.
St.‐Maurice, J.‐P.
Richards, P.
Nicolls, M.
Hairston, M.
Geophysical Research Letters
F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
General Earth and Planetary Sciences
Geophysics
author_sort goodwin, l.
spelling Goodwin, L. St.‐Maurice, J.‐P. Richards, P. Nicolls, M. Hairston, M. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1002/2013gl058442 <jats:p>Using Poker Flat Incoherent Scatter Radar data from the International Polar Year, we observed unexpected short‐lived enhancements of a few 100 K in the <jats:italic>F</jats:italic> region ion temperature, or “<jats:italic>T</jats:italic><jats:sub><jats:italic>i</jats:italic></jats:sub> spikes”, in conjunction with sharp <jats:italic>F</jats:italic> region plasma density drops near the dusk plasmapause. The geomagnetic conditions were moderately to weakly disturbed and the dusk spikes were often the largest <jats:italic>T</jats:italic><jats:sub><jats:italic>i</jats:italic></jats:sub> values recorded within the day. Taking various other observations into consideration, we conclude that the radar observed ion frictional heating events driven by large ion‐neutral relative drifts caused by temporary intensifications in the convection pattern. The heating rate was enhanced through an increase in the size of the convection pattern, causing the neutrals just poleward of the dusk plasmapause to be moving antisunward while ions were moving sunward.</jats:p> F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern Geophysical Research Letters
doi_str_mv 10.1002/2013gl058442
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imprint_str_mv American Geophysical Union (AGU), 2014
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recordtype ai
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series Geophysical Research Letters
source_id 49
title F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_unstemmed F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_full F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_fullStr F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_full_unstemmed F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_short F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_sort f region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
topic General Earth and Planetary Sciences
Geophysics
url http://dx.doi.org/10.1002/2013gl058442
publishDate 2014
physical 300-307
description <jats:p>Using Poker Flat Incoherent Scatter Radar data from the International Polar Year, we observed unexpected short‐lived enhancements of a few 100 K in the <jats:italic>F</jats:italic> region ion temperature, or “<jats:italic>T</jats:italic><jats:sub><jats:italic>i</jats:italic></jats:sub> spikes”, in conjunction with sharp <jats:italic>F</jats:italic> region plasma density drops near the dusk plasmapause. The geomagnetic conditions were moderately to weakly disturbed and the dusk spikes were often the largest <jats:italic>T</jats:italic><jats:sub><jats:italic>i</jats:italic></jats:sub> values recorded within the day. Taking various other observations into consideration, we conclude that the radar observed ion frictional heating events driven by large ion‐neutral relative drifts caused by temporary intensifications in the convection pattern. The heating rate was enhanced through an increase in the size of the convection pattern, causing the neutrals just poleward of the dusk plasmapause to be moving antisunward while ions were moving sunward.</jats:p>
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author Goodwin, L., St.‐Maurice, J.‐P., Richards, P., Nicolls, M., Hairston, M.
author_facet Goodwin, L., St.‐Maurice, J.‐P., Richards, P., Nicolls, M., Hairston, M., Goodwin, L., St.‐Maurice, J.‐P., Richards, P., Nicolls, M., Hairston, M.
author_sort goodwin, l.
container_issue 2
container_start_page 300
container_title Geophysical Research Letters
container_volume 41
description <jats:p>Using Poker Flat Incoherent Scatter Radar data from the International Polar Year, we observed unexpected short‐lived enhancements of a few 100 K in the <jats:italic>F</jats:italic> region ion temperature, or “<jats:italic>T</jats:italic><jats:sub><jats:italic>i</jats:italic></jats:sub> spikes”, in conjunction with sharp <jats:italic>F</jats:italic> region plasma density drops near the dusk plasmapause. The geomagnetic conditions were moderately to weakly disturbed and the dusk spikes were often the largest <jats:italic>T</jats:italic><jats:sub><jats:italic>i</jats:italic></jats:sub> values recorded within the day. Taking various other observations into consideration, we conclude that the radar observed ion frictional heating events driven by large ion‐neutral relative drifts caused by temporary intensifications in the convection pattern. The heating rate was enhanced through an increase in the size of the convection pattern, causing the neutrals just poleward of the dusk plasmapause to be moving antisunward while ions were moving sunward.</jats:p>
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imprint American Geophysical Union (AGU), 2014
imprint_str_mv American Geophysical Union (AGU), 2014
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spelling Goodwin, L. St.‐Maurice, J.‐P. Richards, P. Nicolls, M. Hairston, M. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1002/2013gl058442 <jats:p>Using Poker Flat Incoherent Scatter Radar data from the International Polar Year, we observed unexpected short‐lived enhancements of a few 100 K in the <jats:italic>F</jats:italic> region ion temperature, or “<jats:italic>T</jats:italic><jats:sub><jats:italic>i</jats:italic></jats:sub> spikes”, in conjunction with sharp <jats:italic>F</jats:italic> region plasma density drops near the dusk plasmapause. The geomagnetic conditions were moderately to weakly disturbed and the dusk spikes were often the largest <jats:italic>T</jats:italic><jats:sub><jats:italic>i</jats:italic></jats:sub> values recorded within the day. Taking various other observations into consideration, we conclude that the radar observed ion frictional heating events driven by large ion‐neutral relative drifts caused by temporary intensifications in the convection pattern. The heating rate was enhanced through an increase in the size of the convection pattern, causing the neutrals just poleward of the dusk plasmapause to be moving antisunward while ions were moving sunward.</jats:p> F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern Geophysical Research Letters
spellingShingle Goodwin, L., St.‐Maurice, J.‐P., Richards, P., Nicolls, M., Hairston, M., Geophysical Research Letters, F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern, General Earth and Planetary Sciences, Geophysics
title F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_full F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_fullStr F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_full_unstemmed F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_short F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_sort f region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
title_unstemmed F region dusk ion temperature spikes at the equatorward edge of the high‐latitude convection pattern
topic General Earth and Planetary Sciences, Geophysics
url http://dx.doi.org/10.1002/2013gl058442