Optical tomography of the aurora and EISCAT

Tomographic reconstruction of the three-dimensional auroral arc emission is used to obtain vertical and horizontal distributions of the optical auroral emission. Under the given experimental conditions with a very limited angular range and a small number of observers, algebraic reconstruction method...

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Published in:Annales Geophysicae
Main Authors: Frey, H. U., Frey, S., Lanchester, B. S., Kosch, M.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.1007/s00585-998-1332-y
https://angeo.copernicus.org/articles/16/1332/1998/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo34229 2023-05-15T16:04:24+02:00 Optical tomography of the aurora and EISCAT Frey, H. U. Frey, S. Lanchester, B. S. Kosch, M. 2018-09-27 application/pdf https://doi.org/10.1007/s00585-998-1332-y https://angeo.copernicus.org/articles/16/1332/1998/ eng eng doi:10.1007/s00585-998-1332-y https://angeo.copernicus.org/articles/16/1332/1998/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.1007/s00585-998-1332-y 2020-07-20T16:28:05Z Tomographic reconstruction of the three-dimensional auroral arc emission is used to obtain vertical and horizontal distributions of the optical auroral emission. Under the given experimental conditions with a very limited angular range and a small number of observers, algebraic reconstruction methods generally yield better results than transform techniques. Different algebraic reconstruction methods are tested with an auroral arc model and the best results are obtained with an iterative least-square method adapted from emission-computed tomography. The observation geometry used during a campaign in Norway in 1995 is tested with the arc model and root-mean-square errors, to be expected under the given geometrical conditions, are calculated. Although optimum geometry was not used, root-mean-square errors of less than 2% for the images and of the order of 30% for the distribution could be obtained. The method is applied to images from real observations. The correspondence of original pictures and projections of the reconstructed volume is discussed, and emission profiles along magnetic field lines through the three-dimensionally reconstructed arc are calibrated into electron density profiles with additional EISCAT measurements. Including a background profile and the temporal changes of the electron density due to recombination, good agreement can be obtained between measured profiles and the time-sequence of calculated profiles. These profiles are used to estimate the conductivity distribution in the vicinity of the EISCAT site. While the radar can only probe the ionosphere along the radar beam, the three-dimensional tomography enables conductivity estimates in a large area around the radar site. Key words. Tomography · Aurora · EISCAT · Ionosphere · Conductivity Text EISCAT Copernicus Publications: E-Journals Norway Annales Geophysicae 16 10 1332 1342
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Tomographic reconstruction of the three-dimensional auroral arc emission is used to obtain vertical and horizontal distributions of the optical auroral emission. Under the given experimental conditions with a very limited angular range and a small number of observers, algebraic reconstruction methods generally yield better results than transform techniques. Different algebraic reconstruction methods are tested with an auroral arc model and the best results are obtained with an iterative least-square method adapted from emission-computed tomography. The observation geometry used during a campaign in Norway in 1995 is tested with the arc model and root-mean-square errors, to be expected under the given geometrical conditions, are calculated. Although optimum geometry was not used, root-mean-square errors of less than 2% for the images and of the order of 30% for the distribution could be obtained. The method is applied to images from real observations. The correspondence of original pictures and projections of the reconstructed volume is discussed, and emission profiles along magnetic field lines through the three-dimensionally reconstructed arc are calibrated into electron density profiles with additional EISCAT measurements. Including a background profile and the temporal changes of the electron density due to recombination, good agreement can be obtained between measured profiles and the time-sequence of calculated profiles. These profiles are used to estimate the conductivity distribution in the vicinity of the EISCAT site. While the radar can only probe the ionosphere along the radar beam, the three-dimensional tomography enables conductivity estimates in a large area around the radar site. Key words. Tomography · Aurora · EISCAT · Ionosphere · Conductivity
format Text
author Frey, H. U.
Frey, S.
Lanchester, B. S.
Kosch, M.
spellingShingle Frey, H. U.
Frey, S.
Lanchester, B. S.
Kosch, M.
Optical tomography of the aurora and EISCAT
author_facet Frey, H. U.
Frey, S.
Lanchester, B. S.
Kosch, M.
author_sort Frey, H. U.
title Optical tomography of the aurora and EISCAT
title_short Optical tomography of the aurora and EISCAT
title_full Optical tomography of the aurora and EISCAT
title_fullStr Optical tomography of the aurora and EISCAT
title_full_unstemmed Optical tomography of the aurora and EISCAT
title_sort optical tomography of the aurora and eiscat
publishDate 2018
url https://doi.org/10.1007/s00585-998-1332-y
https://angeo.copernicus.org/articles/16/1332/1998/
geographic Norway
geographic_facet Norway
genre EISCAT
genre_facet EISCAT
op_source eISSN: 1432-0576
op_relation doi:10.1007/s00585-998-1332-y
https://angeo.copernicus.org/articles/16/1332/1998/
op_doi https://doi.org/10.1007/s00585-998-1332-y
container_title Annales Geophysicae
container_volume 16
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