Deriving the normalised ion-neutral collision frequency from EISCAT observations

Common programme observations by the EISCAT UHF radar revealed an extended interval, post geomagnetic local noon on 03 April 1992, during which the F-region ion velocity orthogonal to the geomagnetic field was significantly enhanced, to values exceeding 2 km s –1 corresponding to a perpendicular ele...

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Published in:Annales Geophysicae
Main Authors: Davies, J. A., Lester, M., Robinson, T. R.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.1007/s00585-997-1557-1
https://angeo.copernicus.org/articles/15/1557/1997/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo34290 2023-05-15T16:04:34+02:00 Deriving the normalised ion-neutral collision frequency from EISCAT observations Davies, J. A. Lester, M. Robinson, T. R. 2018-09-27 application/pdf https://doi.org/10.1007/s00585-997-1557-1 https://angeo.copernicus.org/articles/15/1557/1997/ eng eng doi:10.1007/s00585-997-1557-1 https://angeo.copernicus.org/articles/15/1557/1997/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.1007/s00585-997-1557-1 2020-07-20T16:28:07Z Common programme observations by the EISCAT UHF radar revealed an extended interval, post geomagnetic local noon on 03 April 1992, during which the F-region ion velocity orthogonal to the geomagnetic field was significantly enhanced, to values exceeding 2 km s –1 corresponding to a perpendicular electric field of some 100 mV m –1 . Observations from this interval are used to illustrate a method by which estimates of the E-region ion-neutral collision frequency may be derived in the presence of enhanced electric field. From both the rotation of the ion velocity vector and the reduction in the ion velocity magnitude relative to that in the F-region, independent estimates of the normalised ion-neutral collision frequency are made at the UHF E-region tristatic altitudes; the derived values are, in general, lower than model predictions. Although initial calculations assume a stationary neutral atmosphere, first-order estimates of the E-region neutral wind are subsequently employed to calculate revised estimates of the normalised ion-neutral collision frequency; these neutral winds are derived by attributing the difference between predicted and observed enhancements in field-parallel ion temperature to thermospheric motion. The inclusion of neutral winds, which are themselves not inconsiderable, appears to have only a limited effect on the normalised collision frequencies derived. Text EISCAT Copernicus Publications: E-Journals Annales Geophysicae 15 12 1557 1569
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Common programme observations by the EISCAT UHF radar revealed an extended interval, post geomagnetic local noon on 03 April 1992, during which the F-region ion velocity orthogonal to the geomagnetic field was significantly enhanced, to values exceeding 2 km s –1 corresponding to a perpendicular electric field of some 100 mV m –1 . Observations from this interval are used to illustrate a method by which estimates of the E-region ion-neutral collision frequency may be derived in the presence of enhanced electric field. From both the rotation of the ion velocity vector and the reduction in the ion velocity magnitude relative to that in the F-region, independent estimates of the normalised ion-neutral collision frequency are made at the UHF E-region tristatic altitudes; the derived values are, in general, lower than model predictions. Although initial calculations assume a stationary neutral atmosphere, first-order estimates of the E-region neutral wind are subsequently employed to calculate revised estimates of the normalised ion-neutral collision frequency; these neutral winds are derived by attributing the difference between predicted and observed enhancements in field-parallel ion temperature to thermospheric motion. The inclusion of neutral winds, which are themselves not inconsiderable, appears to have only a limited effect on the normalised collision frequencies derived.
format Text
author Davies, J. A.
Lester, M.
Robinson, T. R.
spellingShingle Davies, J. A.
Lester, M.
Robinson, T. R.
Deriving the normalised ion-neutral collision frequency from EISCAT observations
author_facet Davies, J. A.
Lester, M.
Robinson, T. R.
author_sort Davies, J. A.
title Deriving the normalised ion-neutral collision frequency from EISCAT observations
title_short Deriving the normalised ion-neutral collision frequency from EISCAT observations
title_full Deriving the normalised ion-neutral collision frequency from EISCAT observations
title_fullStr Deriving the normalised ion-neutral collision frequency from EISCAT observations
title_full_unstemmed Deriving the normalised ion-neutral collision frequency from EISCAT observations
title_sort deriving the normalised ion-neutral collision frequency from eiscat observations
publishDate 2018
url https://doi.org/10.1007/s00585-997-1557-1
https://angeo.copernicus.org/articles/15/1557/1997/
genre EISCAT
genre_facet EISCAT
op_source eISSN: 1432-0576
op_relation doi:10.1007/s00585-997-1557-1
https://angeo.copernicus.org/articles/15/1557/1997/
op_doi https://doi.org/10.1007/s00585-997-1557-1
container_title Annales Geophysicae
container_volume 15
container_issue 12
container_start_page 1557
op_container_end_page 1569
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