Please use this identifier to cite or link to this item:
http://hdl.handle.net/2122/913
DC Field | Value | Language |
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dc.contributor.authorall | Tsagouri, I.; Ionospheric Group, Institute for Space Applications and Remote Sensing, National Observatory of Athens, Palaia Penteli, Greece | en |
dc.contributor.authorall | Belehaki, A.; Ionospheric Group, Institute for Space Applications and Remote Sensing, National Observatory of Athens, Palaia Penteli, Greece | en |
dc.contributor.authorall | Cander, L. R.; Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K. | en |
dc.date.accessioned | 2006-02-22T14:17:52Z | en |
dc.date.available | 2006-02-22T14:17:52Z | en |
dc.date.issued | 2005 | en |
dc.identifier.uri | http://hdl.handle.net/2122/913 | en |
dc.description.abstract | For the reliable performance of technologically advanced radio communications systems under geomagnetically disturbed conditions, the forecast and modelling of the ionospheric response during storms is a high priority. The ionospheric storm forecasting models that are currently in operation have shown a high degree of reliability during quiet conditions, but they have proved inadequate during storm events. To improve their prediction accuracy, we have to take advantage of the deeper understanding in ionospheric storm dynamics that is currently available, indicating a correlation between the Interplanetary Magnetic Field (IMF) disturbances and the qualitative signature of ionospheric storm disturbances at middle latitude stations. In this paper we analyse observations of the foF2 critical frequency parameter from one mid-latitude European ionospheric station (Chilton) in conjunction with observations of IMF parameters (total magnitude, Bt and Bz-IMF component) from the ACE spacecraft mission for eight storm events. The determination of the time delay in the ionospheric response to the interplanetary medium disturbances leads to significant results concerning the forecast of the ionospheric storms onset and their development during the first 24 h. In this way the real-time ACE observations of the solar wind parameters may be used in the development of a real-time dynamic ionospheric storm model with adequate accuracy. | en |
dc.format.extent | 1630058 bytes | en |
dc.format.mimetype | application/pdf | en |
dc.language.iso | English | en |
dc.publisher.name | INGV | en |
dc.relation.ispartof | Annals of Geophysics | en |
dc.relation.ispartofseries | 3/48 (2005) | en |
dc.subject | inospheric forecasting | en |
dc.subject | ionospheric modelling | en |
dc.subject | ionospheric storms | en |
dc.title | A dynamic system to forecast ionospheric storm disturbances based on solar wind conditions | en |
dc.type | article | en |
dc.description.status | Published | en |
dc.type.QualityControl | Peer-reviewed | en |
dc.subject.INGV | 01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniques | en |
dc.description.journalType | JCR Journal | en |
dc.description.fulltext | open | en |
dc.contributor.author | Tsagouri, I. | en |
dc.contributor.author | Belehaki, A. | en |
dc.contributor.author | Cander, L. R. | en |
dc.contributor.department | Ionospheric Group, Institute for Space Applications and Remote Sensing, National Observatory of Athens, Palaia Penteli, Greece | en |
dc.contributor.department | Ionospheric Group, Institute for Space Applications and Remote Sensing, National Observatory of Athens, Palaia Penteli, Greece | en |
dc.contributor.department | Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K. | en |
item.openairetype | article | - |
item.cerifentitytype | Publications | - |
item.languageiso639-1 | en | - |
item.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | National Observatory of Athens, Institute for Space Applications and Remote Sensing, Palaia Penteli 15236, Greece | - |
crisitem.author.dept | Institute for Space Applications and Remote Sensing, National Observatory of Athens, Palaia Penteli, Greece" | - |
crisitem.author.dept | Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, U.K. | - |
crisitem.author.orcid | 0000-0002-9270-5387 | - |
crisitem.author.orcid | 0000-0002-7263-5043 | - |
crisitem.classification.parent | 01. Atmosphere | - |
Appears in Collections: | Annals of Geophysics |
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File | Description | Size | Format | |
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05Tsagouri.pdf | 1.59 MB | Adobe PDF | View/Open |
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