Auroral E-region electron density gradients measured

In the theory of E -region plasma instabilities, the ambient electric field and electron density gradient are both included in the same dispersion relation as the key parameters that provide the energy for the generation and growth of electrostatic plasma waves. While there exist numerous measuremen...

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Published in:Annales Geophysicae
Main Authors: Haldoupis, C., Schlegel, K., Hussey, G.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.1007/s00585-000-1172-x
https://angeo.copernicus.org/articles/18/1172/2000/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo34588 2023-05-15T16:04:45+02:00 Auroral E-region electron density gradients measured Haldoupis, C. Schlegel, K. Hussey, G. 2018-09-27 application/pdf https://doi.org/10.1007/s00585-000-1172-x https://angeo.copernicus.org/articles/18/1172/2000/ eng eng doi:10.1007/s00585-000-1172-x https://angeo.copernicus.org/articles/18/1172/2000/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.1007/s00585-000-1172-x 2020-07-20T16:27:57Z In the theory of E -region plasma instabilities, the ambient electric field and electron density gradient are both included in the same dispersion relation as the key parameters that provide the energy for the generation and growth of electrostatic plasma waves. While there exist numerous measurements of ionospheric electric fields, there are very few measurements and limited knowledge about the ambient electron density gradients, ∇ N e , in the E -region plasma. In this work, we took advantage of the EISCAT CP1 data base and studied statistically the vertical electron density gradient length, L z = N e /(d N e /d z ), at auroral E -region heights during both eastward and westward electrojet conditions and different ambient electric field levels. Overall, the prevailing electron density gradients, with L z ranging from 4 to 7 km, are found to be located below 100 km, but to move steadily up in altitude as the electric field level increases. The steepest density gradients, with L z possibly less than 3 km, occur near 110 km mostly in the eastward electrojet during times of strong electric fields. The results and their implications are examined and discussed in the frame of the linear gradient drift instability theory. Finally, it would be interesting to test the implications of the present results with a vertical radar interferometer. Key words: Ionosphere (auroral ionosphere; ionospheric irregularities; plasma waves and instabilities) Text EISCAT Copernicus Publications: E-Journals Annales Geophysicae 18 9 1172 1181
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description In the theory of E -region plasma instabilities, the ambient electric field and electron density gradient are both included in the same dispersion relation as the key parameters that provide the energy for the generation and growth of electrostatic plasma waves. While there exist numerous measurements of ionospheric electric fields, there are very few measurements and limited knowledge about the ambient electron density gradients, ∇ N e , in the E -region plasma. In this work, we took advantage of the EISCAT CP1 data base and studied statistically the vertical electron density gradient length, L z = N e /(d N e /d z ), at auroral E -region heights during both eastward and westward electrojet conditions and different ambient electric field levels. Overall, the prevailing electron density gradients, with L z ranging from 4 to 7 km, are found to be located below 100 km, but to move steadily up in altitude as the electric field level increases. The steepest density gradients, with L z possibly less than 3 km, occur near 110 km mostly in the eastward electrojet during times of strong electric fields. The results and their implications are examined and discussed in the frame of the linear gradient drift instability theory. Finally, it would be interesting to test the implications of the present results with a vertical radar interferometer. Key words: Ionosphere (auroral ionosphere; ionospheric irregularities; plasma waves and instabilities)
format Text
author Haldoupis, C.
Schlegel, K.
Hussey, G.
spellingShingle Haldoupis, C.
Schlegel, K.
Hussey, G.
Auroral E-region electron density gradients measured
author_facet Haldoupis, C.
Schlegel, K.
Hussey, G.
author_sort Haldoupis, C.
title Auroral E-region electron density gradients measured
title_short Auroral E-region electron density gradients measured
title_full Auroral E-region electron density gradients measured
title_fullStr Auroral E-region electron density gradients measured
title_full_unstemmed Auroral E-region electron density gradients measured
title_sort auroral e-region electron density gradients measured
publishDate 2018
url https://doi.org/10.1007/s00585-000-1172-x
https://angeo.copernicus.org/articles/18/1172/2000/
genre EISCAT
genre_facet EISCAT
op_source eISSN: 1432-0576
op_relation doi:10.1007/s00585-000-1172-x
https://angeo.copernicus.org/articles/18/1172/2000/
op_doi https://doi.org/10.1007/s00585-000-1172-x
container_title Annales Geophysicae
container_volume 18
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container_start_page 1172
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