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: H. U. Frey, S. Frey, B. S. Lanchester, M. Kosch
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 1998
Subjects:
Q
Online Access:https://doi.org/10.1007/s00585-998-1332-y
https://doaj.org/article/94d10f8245fb477ca3308f53154b32c6
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spelling ftdoajarticles:oai:doaj.org/article:94d10f8245fb477ca3308f53154b32c6 2023-05-15T16:04:25+02:00 Optical tomography of the aurora and EISCAT H. U. Frey S. Frey B. S. Lanchester M. Kosch 1998-10-01T00:00:00Z https://doi.org/10.1007/s00585-998-1332-y https://doaj.org/article/94d10f8245fb477ca3308f53154b32c6 EN eng Copernicus Publications https://www.ann-geophys.net/16/1332/1998/angeo-16-1332-1998.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576 doi:10.1007/s00585-998-1332-y 0992-7689 1432-0576 https://doaj.org/article/94d10f8245fb477ca3308f53154b32c6 Annales Geophysicae, Vol 16, Pp 1332-1342 (1998) Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 article 1998 ftdoajarticles https://doi.org/10.1007/s00585-998-1332-y 2022-12-31T04:45:22Z 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 Article in Journal/Newspaper EISCAT Directory of Open Access Journals: DOAJ Articles Norway Annales Geophysicae 16 10 1332 1342
institution Open Polar
collection Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
topic Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
spellingShingle Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
H. U. Frey
S. Frey
B. S. Lanchester
M. Kosch
Optical tomography of the aurora and EISCAT
topic_facet Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
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 Article in Journal/Newspaper
author H. U. Frey
S. Frey
B. S. Lanchester
M. Kosch
author_facet H. U. Frey
S. Frey
B. S. Lanchester
M. Kosch
author_sort H. U. Frey
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
publisher Copernicus Publications
publishDate 1998
url https://doi.org/10.1007/s00585-998-1332-y
https://doaj.org/article/94d10f8245fb477ca3308f53154b32c6
geographic Norway
geographic_facet Norway
genre EISCAT
genre_facet EISCAT
op_source Annales Geophysicae, Vol 16, Pp 1332-1342 (1998)
op_relation https://www.ann-geophys.net/16/1332/1998/angeo-16-1332-1998.pdf
https://doaj.org/toc/0992-7689
https://doaj.org/toc/1432-0576
doi:10.1007/s00585-998-1332-y
0992-7689
1432-0576
https://doaj.org/article/94d10f8245fb477ca3308f53154b32c6
op_doi https://doi.org/10.1007/s00585-998-1332-y
container_title Annales Geophysicae
container_volume 16
container_issue 10
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