The response of the ionosphere to faint and bright solar flares as deduced from global GPS network data

Results derived from analysing the ionosphere response to faint and bright solar flares are presented. The analysis used technology of a global detection of ionospheric effects from solar flares as developed by the authors, on the basis of phase measurements of the Total Electron Content (TEC) in th...

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Main Authors: L. A. Leonovich, V. V. Grechnev, A. T. Altynsev, E. L. Afraimovich
Format: Article
Language:English
Published: Istituto Nazionale di Geofisica e Vulcanologia (INGV) 2002-06-01
Series:Annals of Geophysics
Subjects:
Online Access:http://www.annalsofgeophysics.eu/index.php/annals/article/view/3480
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spelling doaj-948a4fced2e44607aece7d51f5cf856b2020-11-24T23:35:23ZengIstituto Nazionale di Geofisica e Vulcanologia (INGV)Annals of Geophysics1593-52132037-416X2002-06-0145110.4401/ag-3480The response of the ionosphere to faint and bright solar flares as deduced from global GPS network dataL. A. LeonovichV. V. GrechnevA. T. AltynsevE. L. AfraimovichResults derived from analysing the ionosphere response to faint and bright solar flares are presented. The analysis used technology of a global detection of ionospheric effects from solar flares as developed by the authors, on the basis of phase measurements of the Total Electron Content (TEC) in the ionosphere using an international GPS network. The essence of the method is that use is made of appropriate filtering and a coherent processing of variations in the TEC which is determined from GPS data, simultaneously for the entire set of visible GPS satellites at all stations used in the analysis. This technique is useful for identifying the ionospheric response to faint solar flares (of X-ray class C) when the variation amplitude of the TEC response to separate line-on-sight to GPS satellite is comparable to the level of background fluctuations. The dependence of the TEC variation response amplitude on the bright flares location on the Sun is investigatedhttp://www.annalsofgeophysics.eu/index.php/annals/article/view/3480ionopshereTotal Electron Content
collection DOAJ
language English
format Article
sources DOAJ
author L. A. Leonovich
V. V. Grechnev
A. T. Altynsev
E. L. Afraimovich
spellingShingle L. A. Leonovich
V. V. Grechnev
A. T. Altynsev
E. L. Afraimovich
The response of the ionosphere to faint and bright solar flares as deduced from global GPS network data
Annals of Geophysics
ionopshere
Total Electron Content
author_facet L. A. Leonovich
V. V. Grechnev
A. T. Altynsev
E. L. Afraimovich
author_sort L. A. Leonovich
title The response of the ionosphere to faint and bright solar flares as deduced from global GPS network data
title_short The response of the ionosphere to faint and bright solar flares as deduced from global GPS network data
title_full The response of the ionosphere to faint and bright solar flares as deduced from global GPS network data
title_fullStr The response of the ionosphere to faint and bright solar flares as deduced from global GPS network data
title_full_unstemmed The response of the ionosphere to faint and bright solar flares as deduced from global GPS network data
title_sort response of the ionosphere to faint and bright solar flares as deduced from global gps network data
publisher Istituto Nazionale di Geofisica e Vulcanologia (INGV)
series Annals of Geophysics
issn 1593-5213
2037-416X
publishDate 2002-06-01
description Results derived from analysing the ionosphere response to faint and bright solar flares are presented. The analysis used technology of a global detection of ionospheric effects from solar flares as developed by the authors, on the basis of phase measurements of the Total Electron Content (TEC) in the ionosphere using an international GPS network. The essence of the method is that use is made of appropriate filtering and a coherent processing of variations in the TEC which is determined from GPS data, simultaneously for the entire set of visible GPS satellites at all stations used in the analysis. This technique is useful for identifying the ionospheric response to faint solar flares (of X-ray class C) when the variation amplitude of the TEC response to separate line-on-sight to GPS satellite is comparable to the level of background fluctuations. The dependence of the TEC variation response amplitude on the bright flares location on the Sun is investigated
topic ionopshere
Total Electron Content
url http://www.annalsofgeophysics.eu/index.php/annals/article/view/3480
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