A theoretical interpretation of ion composition measured on board the 'Active' satellite in the European sector during April 10−12, 1990 geomagnetic storm

Ion composition measurements on board the ACTIVE satellite during the recovery phase of a strong geomagnetic storm of 10-12 April 1990 revealed extremely high concentrations (up to 10<sup>3</sup> cm<sup>-3</sup>) of the NO<sup>+</sup>, O<sup>+</sup><...

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Main Authors: J. Smilauer, A. Mikhailov, V. Mikhailov, M. Förster
Format: Article
Language:English
Published: Copernicus Publications
Series:Annales Geophysicae
Online Access:http://www.ann-geophys.net/13/608/1995/angeo-13-608-1995.html
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spelling doaj-b8d6784ce7b74c8385f5598ef28828ce2020-11-25T00:04:45ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-0576136608616A theoretical interpretation of ion composition measured on board the 'Active' satellite in the European sector during April 10&#x2212;12, 1990 geomagnetic stormJ. SmilauerA. MikhailovV. MikhailovM. FörsterIon composition measurements on board the ACTIVE satellite during the recovery phase of a strong geomagnetic storm of 10-12 April 1990 revealed extremely high concentrations (up to 10<sup>3</sup> cm<sup>-3</sup>) of the NO<sup>+</sup>, O<sup>+</sup><sub>2</sub>, N<sup>+</sup><sub>2</sub> molecular ions in the topside F2-region of the European high-latitude zone. Concentrations of O<sup>+</sup>, N<sup>+</sup>, He<sup>+</sup>, H<sup>+</sup> light ions were slightly decreased relative to prestorm quite conditions. Theoretical calculations were used to analyze the observed variations in ion concentration. Increased neutral temperature and [O<sub>2</sub>], [N<sub>2</sub>] are shown to be the main reasons for the observed ion concentration variations. http://www.ann-geophys.net/13/608/1995/angeo-13-608-1995.html
collection DOAJ
language English
format Article
sources DOAJ
author J. Smilauer
A. Mikhailov
V. Mikhailov
M. Förster
spellingShingle J. Smilauer
A. Mikhailov
V. Mikhailov
M. Förster
A theoretical interpretation of ion composition measured on board the 'Active' satellite in the European sector during April 10&#x2212;12, 1990 geomagnetic storm
Annales Geophysicae
author_facet J. Smilauer
A. Mikhailov
V. Mikhailov
M. Förster
author_sort J. Smilauer
title A theoretical interpretation of ion composition measured on board the 'Active' satellite in the European sector during April 10&#x2212;12, 1990 geomagnetic storm
title_short A theoretical interpretation of ion composition measured on board the 'Active' satellite in the European sector during April 10&#x2212;12, 1990 geomagnetic storm
title_full A theoretical interpretation of ion composition measured on board the 'Active' satellite in the European sector during April 10&#x2212;12, 1990 geomagnetic storm
title_fullStr A theoretical interpretation of ion composition measured on board the 'Active' satellite in the European sector during April 10&#x2212;12, 1990 geomagnetic storm
title_full_unstemmed A theoretical interpretation of ion composition measured on board the 'Active' satellite in the European sector during April 10&#x2212;12, 1990 geomagnetic storm
title_sort theoretical interpretation of ion composition measured on board the 'active' satellite in the european sector during april 10&#x2212;12, 1990 geomagnetic storm
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
description Ion composition measurements on board the ACTIVE satellite during the recovery phase of a strong geomagnetic storm of 10-12 April 1990 revealed extremely high concentrations (up to 10<sup>3</sup> cm<sup>-3</sup>) of the NO<sup>+</sup>, O<sup>+</sup><sub>2</sub>, N<sup>+</sup><sub>2</sub> molecular ions in the topside F2-region of the European high-latitude zone. Concentrations of O<sup>+</sup>, N<sup>+</sup>, He<sup>+</sup>, H<sup>+</sup> light ions were slightly decreased relative to prestorm quite conditions. Theoretical calculations were used to analyze the observed variations in ion concentration. Increased neutral temperature and [O<sub>2</sub>], [N<sub>2</sub>] are shown to be the main reasons for the observed ion concentration variations.
url http://www.ann-geophys.net/13/608/1995/angeo-13-608-1995.html
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