Ionospheric response to magnetic disturbances under low solar activity conditions and STORM model corrections for the disturbed periods

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F13%3A00431026" target="_blank" >RIV/68378289:_____/13:00431026 - isvavai.cz</a>

Result on the web

<a href="http://www.uwm.edu.pl/kaig/iri_workshop_2013/media/pdf/Buresova.pdf" target="_blank" >http://www.uwm.edu.pl/kaig/iri_workshop_2013/media/pdf/Buresova.pdf</a>

DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Ionospheric response to magnetic disturbances under low solar activity conditions and STORM model corrections for the disturbed periods

Original language description

The presented results show that the effects on the middle latitude ionosphere of weak-to-moderate CIR-related magnetic storms, which mostly occur during the declining phase of the solar cycle, could be comparable with the effects of strong magnetic storms. In general, both positive and negative deviations of foF2 and hmF2 from their 27-days running means have been observed independent on season and location. Positive effects on foF2 prevail and are more significant. The IRI STORM model gives no corrections of foF2 for analysed events.

Czech name

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Czech description

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Type

A - Audiovisual production

CEP classification

DG - Atmospheric sciences, meteorology

OECD FORD branch

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Project

<a href="/en/project/GAP209%2F11%2F1908" target="_blank" >GAP209/11/1908: Ionospheric response to magnetic storm-induced disturbances:recovery phase</a><br>

Continuities

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year

2013

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

ISBN

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Place of publication

Olsztyn

Publisher/client name

University of Olsztyn

Version

1.

Carrier ID

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