Nonlinear analysis of decimetric solar bursts

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00355597" target="_blank" >RIV/67985815:_____/10:00355597 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Nonlinear analysis of decimetric solar bursts
Original language description
The solar radio emissions in the decimetric frequency range (above 1 GHz) are very rich in temporal and spectral fine structures due to nonlinear processes occurring in the magnetic structures on the corresponding active regions. In this paper we characterize the singularity spectrum, f (a), for solar bursts observed at 1.6, 2.0 and 3 CHz. We interpret our findings as evidence of inhornogeneous plasma turbulence driving the underlying plasma emission process and discuss the nonlinear multifractal approach into the context of geoeffective solar active regions.
Czech name
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Czech description
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Publication year
2010
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Solar and stellar variability: Impact on Earth and planets
ISBN
978-0-521-76492-6
ISSN
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e-ISSN
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Number of pages
3
Pages from-to
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Publisher name
Cambridge University Press
Place of publication
Cambridge
Event location
Rio de Janeiro
Event date
Aug 3, 2009
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000280547700048

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