Regular variations of 3 GHz radio flux and current-loop coalescence model of solar flares.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F03%3A01030068" target="_blank" >RIV/67985815:_____/03:01030068 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Regular variations of 3 GHz radio flux and current-loop coalescence model of solar flares.
Original language description
The 3 GHz radio flux records of two solar flares (April 7, 1997 and March 29, 2001) with regular variations are presented. The authors interpret the observed phenomena using the current loop coalescence model of solar flares.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2003
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Solar variability as an input to the Earth's environment.
ISBN
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ISSN
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e-ISSN
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Number of pages
4
Pages from-to
499-502
Publisher name
ESA Publication division
Place of publication
Noordwijk
Event location
Tatranská Lomnica [SK]
Event date
Jun 23, 2003
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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