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IRI topside correction

The topside segment of the International Reference Ionosphere (IRI) electron density model (and also of the Bent model) is based on the limited amount of topside data available at the time (approx 40,000 Alouette 1 profiles). Being established from such a small database it is therefore not surprisin...

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Autor principal: Bilitza, D
Lenguaje:eng
Publicado: 2002
Materias:
Acceso en línea:http://cds.cern.ch/record/746996
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author Bilitza, D
author_facet Bilitza, D
author_sort Bilitza, D
collection CERN
description The topside segment of the International Reference Ionosphere (IRI) electron density model (and also of the Bent model) is based on the limited amount of topside data available at the time (approx 40,000 Alouette 1 profiles). Being established from such a small database it is therefore not surprising that these models have well-known shortcomings, for example, at high solar activities. Meanwhile a large data base of close to 200,000 topside profiles from Alouette 1, 2, and ISIS 1, 2 has become available online. A program of automated scaling and inversion of a large volume of digitized ionograms adds continuously to this data pool. We have used the currently available ISIS/Alouette topside profiles to evaluate the IRI topside model and to investigate ways of improving the model. The IRI model performs generally well at middle latitudes and shows discrepancies at low and high latitudes and these discrepancies are largest during high solar activity. In the upper topside IRI consistently overestimates the measurements. Based on averages of the data-model ratios we have established correction factors for the IRI model. These factors vary with altitude, modified dip latitude, and local time.
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institution Organización Europea para la Investigación Nuclear
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publishDate 2002
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spelling cern-7469962019-09-30T06:29:59Zhttp://cds.cern.ch/record/746996engBilitza, DIRI topside correctionGeneral Theoretical PhysicsThe topside segment of the International Reference Ionosphere (IRI) electron density model (and also of the Bent model) is based on the limited amount of topside data available at the time (approx 40,000 Alouette 1 profiles). Being established from such a small database it is therefore not surprising that these models have well-known shortcomings, for example, at high solar activities. Meanwhile a large data base of close to 200,000 topside profiles from Alouette 1, 2, and ISIS 1, 2 has become available online. A program of automated scaling and inversion of a large volume of digitized ionograms adds continuously to this data pool. We have used the currently available ISIS/Alouette topside profiles to evaluate the IRI topside model and to investigate ways of improving the model. The IRI model performs generally well at middle latitudes and shows discrepancies at low and high latitudes and these discrepancies are largest during high solar activity. In the upper topside IRI consistently overestimates the measurements. Based on averages of the data-model ratios we have established correction factors for the IRI model. These factors vary with altitude, modified dip latitude, and local time.IC-IR-2003-3INT-0002144oai:cds.cern.ch:7469962002
spellingShingle General Theoretical Physics
Bilitza, D
IRI topside correction
title IRI topside correction
title_full IRI topside correction
title_fullStr IRI topside correction
title_full_unstemmed IRI topside correction
title_short IRI topside correction
title_sort iri topside correction
topic General Theoretical Physics
url http://cds.cern.ch/record/746996
work_keys_str_mv AT bilitzad iritopsidecorrection