H.: Eastward propagation of a plasma convection enhancement following a southward turning of the interplanetary magnetic field, Geophys
ionospheric convection was observed by the European incoherent scatter (EISCAT) radar. For a nine-hour period, simultaneous observations of the interplanetary magnetic field (IMF) were obtained sunward of the Earth's bow shock. During this period, the IMF abruptly turned southward, having previ...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.694.6246 2023-05-15T16:04:30+02:00 H.: Eastward propagation of a plasma convection enhancement following a southward turning of the interplanetary magnetic field, Geophys M. Lockwood A. P. Van Eyken B. J. I. Bromage D. M. Willis The Pennsylvania State University CiteSeerX Archives 1986 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.694.6246 http://www.eiscat.rl.ac.uk/Members/mike/publications/pdfs/1986/21_Lockwoodetal_1986.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.694.6246 http://www.eiscat.rl.ac.uk/Members/mike/publications/pdfs/1986/21_Lockwoodetal_1986.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.eiscat.rl.ac.uk/Members/mike/publications/pdfs/1986/21_Lockwoodetal_1986.pdf text 1986 ftciteseerx 2016-01-08T18:34:34Z ionospheric convection was observed by the European incoherent scatter (EISCAT) radar. For a nine-hour period, simultaneous observations of the interplanetary magnetic field (IMF) were obtained sunward of the Earth's bow shock. During this period, the IMF abruptly turned southward, having previously been predominantly northward for approximately three hours, and a strong enhancement in convection was observed 11 + _ 1 minutes later. Using the very high time resolution of the EISCAT data, it is shown that the convection enhancement propagated eastward, around the af•ternoon magnetic local time sector, at a speed of the order of 1 kmõ 1. These results are interpreted in terms of the effects of an onset of steady IMF-geomagnetic field merging and are the first to show how a new pattern of enhanced convection is established in the high latitude ionosphere. Text EISCAT Unknown |
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Open Polar |
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ftciteseerx |
language |
English |
description |
ionospheric convection was observed by the European incoherent scatter (EISCAT) radar. For a nine-hour period, simultaneous observations of the interplanetary magnetic field (IMF) were obtained sunward of the Earth's bow shock. During this period, the IMF abruptly turned southward, having previously been predominantly northward for approximately three hours, and a strong enhancement in convection was observed 11 + _ 1 minutes later. Using the very high time resolution of the EISCAT data, it is shown that the convection enhancement propagated eastward, around the af•ternoon magnetic local time sector, at a speed of the order of 1 kmõ 1. These results are interpreted in terms of the effects of an onset of steady IMF-geomagnetic field merging and are the first to show how a new pattern of enhanced convection is established in the high latitude ionosphere. |
author2 |
The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
M. Lockwood A. P. Van Eyken B. J. I. Bromage D. M. Willis |
spellingShingle |
M. Lockwood A. P. Van Eyken B. J. I. Bromage D. M. Willis H.: Eastward propagation of a plasma convection enhancement following a southward turning of the interplanetary magnetic field, Geophys |
author_facet |
M. Lockwood A. P. Van Eyken B. J. I. Bromage D. M. Willis |
author_sort |
M. Lockwood |
title |
H.: Eastward propagation of a plasma convection enhancement following a southward turning of the interplanetary magnetic field, Geophys |
title_short |
H.: Eastward propagation of a plasma convection enhancement following a southward turning of the interplanetary magnetic field, Geophys |
title_full |
H.: Eastward propagation of a plasma convection enhancement following a southward turning of the interplanetary magnetic field, Geophys |
title_fullStr |
H.: Eastward propagation of a plasma convection enhancement following a southward turning of the interplanetary magnetic field, Geophys |
title_full_unstemmed |
H.: Eastward propagation of a plasma convection enhancement following a southward turning of the interplanetary magnetic field, Geophys |
title_sort |
h.: eastward propagation of a plasma convection enhancement following a southward turning of the interplanetary magnetic field, geophys |
publishDate |
1986 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.694.6246 http://www.eiscat.rl.ac.uk/Members/mike/publications/pdfs/1986/21_Lockwoodetal_1986.pdf |
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EISCAT |
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EISCAT |
op_source |
http://www.eiscat.rl.ac.uk/Members/mike/publications/pdfs/1986/21_Lockwoodetal_1986.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.694.6246 http://www.eiscat.rl.ac.uk/Members/mike/publications/pdfs/1986/21_Lockwoodetal_1986.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766400082169561088 |