The ionospheric response to perturbation electric fields during the onset phase of geomagnetic storms

The generation and propagation of ionospheric storms are studied by analyzing EISCAT radar, and vertical-sounding and total-electron-content data obtained under different geophysical conditions. Both, case studies as well as the average storm pattern of percentage deviations of different ionospheric...

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Published in:Canadian Journal of Physics
Main Authors: Jakowski, N., Jungstand, A., Schlegel, K., Kohl, H., Rinnert, K.
Format: Article in Journal/Newspaper
Language:English
Published: Canadian Science Publishing 1992
Subjects:
Online Access:http://dx.doi.org/10.1139/p92-093
http://www.nrcresearchpress.com/doi/pdf/10.1139/p92-093
id crcansciencepubl:10.1139/p92-093
record_format openpolar
spelling crcansciencepubl:10.1139/p92-093 2024-03-03T08:44:02+00:00 The ionospheric response to perturbation electric fields during the onset phase of geomagnetic storms Jakowski, N. Jungstand, A. Schlegel, K. Kohl, H. Rinnert, K. 1992 http://dx.doi.org/10.1139/p92-093 http://www.nrcresearchpress.com/doi/pdf/10.1139/p92-093 en eng Canadian Science Publishing http://www.nrcresearchpress.com/page/about/CorporateTextAndDataMining Canadian Journal of Physics volume 70, issue 7, page 575-581 ISSN 0008-4204 1208-6045 General Physics and Astronomy journal-article 1992 crcansciencepubl https://doi.org/10.1139/p92-093 2024-02-07T10:53:31Z The generation and propagation of ionospheric storms are studied by analyzing EISCAT radar, and vertical-sounding and total-electron-content data obtained under different geophysical conditions. Both, case studies as well as the average storm pattern of percentage deviations of different ionospheric parameters from their corresponding reference values such as total electron content, F2-layer critical frequency foF2, F2-layer height hmF2, and slab thickness τ indicate the action of a perturbation electric field during the first few hours during the onset phase of geomagnetic storms. Considering the onset phase of the storm on July 28–29, 1987 evidence has been found that high-latitude electric fields may penetrate to lower latitudes before the ring current has developed. In most cases this process is accompanied by a positive phase in the upper ionosphere and F2-layer ionization. Different mechanisms are assumed to be responsible for the daytime and nighttime behaviour, respectively. The negative phase propagates equatorward with velocities in the order of 70–350 m s −1 following a strong heating of the thermosphere and ionosphere due to the auroral electrojet. Article in Journal/Newspaper EISCAT Canadian Science Publishing Canadian Journal of Physics 70 7 575 581
institution Open Polar
collection Canadian Science Publishing
op_collection_id crcansciencepubl
language English
topic General Physics and Astronomy
spellingShingle General Physics and Astronomy
Jakowski, N.
Jungstand, A.
Schlegel, K.
Kohl, H.
Rinnert, K.
The ionospheric response to perturbation electric fields during the onset phase of geomagnetic storms
topic_facet General Physics and Astronomy
description The generation and propagation of ionospheric storms are studied by analyzing EISCAT radar, and vertical-sounding and total-electron-content data obtained under different geophysical conditions. Both, case studies as well as the average storm pattern of percentage deviations of different ionospheric parameters from their corresponding reference values such as total electron content, F2-layer critical frequency foF2, F2-layer height hmF2, and slab thickness τ indicate the action of a perturbation electric field during the first few hours during the onset phase of geomagnetic storms. Considering the onset phase of the storm on July 28–29, 1987 evidence has been found that high-latitude electric fields may penetrate to lower latitudes before the ring current has developed. In most cases this process is accompanied by a positive phase in the upper ionosphere and F2-layer ionization. Different mechanisms are assumed to be responsible for the daytime and nighttime behaviour, respectively. The negative phase propagates equatorward with velocities in the order of 70–350 m s −1 following a strong heating of the thermosphere and ionosphere due to the auroral electrojet.
format Article in Journal/Newspaper
author Jakowski, N.
Jungstand, A.
Schlegel, K.
Kohl, H.
Rinnert, K.
author_facet Jakowski, N.
Jungstand, A.
Schlegel, K.
Kohl, H.
Rinnert, K.
author_sort Jakowski, N.
title The ionospheric response to perturbation electric fields during the onset phase of geomagnetic storms
title_short The ionospheric response to perturbation electric fields during the onset phase of geomagnetic storms
title_full The ionospheric response to perturbation electric fields during the onset phase of geomagnetic storms
title_fullStr The ionospheric response to perturbation electric fields during the onset phase of geomagnetic storms
title_full_unstemmed The ionospheric response to perturbation electric fields during the onset phase of geomagnetic storms
title_sort ionospheric response to perturbation electric fields during the onset phase of geomagnetic storms
publisher Canadian Science Publishing
publishDate 1992
url http://dx.doi.org/10.1139/p92-093
http://www.nrcresearchpress.com/doi/pdf/10.1139/p92-093
genre EISCAT
genre_facet EISCAT
op_source Canadian Journal of Physics
volume 70, issue 7, page 575-581
ISSN 0008-4204 1208-6045
op_rights http://www.nrcresearchpress.com/page/about/CorporateTextAndDataMining
op_doi https://doi.org/10.1139/p92-093
container_title Canadian Journal of Physics
container_volume 70
container_issue 7
container_start_page 575
op_container_end_page 581
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