Number of the records: 1  

Nonlinear analysis of decimetric solar bursts

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    SYSNO ASEP0355597
    Document TypeC - Proceedings Paper (int. conf.)
    R&D Document TypeConference Paper
    TitleNonlinear analysis of decimetric solar bursts
    Author(s) Rosa, R. R. (BR)
    Bolzan, M.J.A. (BR)
    Fernandes, F. C. R. (BR)
    Sawant, H. S. (BR)
    Karlický, Marian (ASU-R) RID, ORCID
    Source TitleSolar and stellar variability: Impact on Earth and planets. - Cambridge : Cambridge University Press, 2010 / Kosovichev A.G. ; Andrei A.H. ; Rozelot J.-P. - ISSN 1743-9213 - ISBN 978-0-521-76492-6
    Pagess. 279-281
    Number of pages3 s.
    ActionSymposium of the International Astronomical Union /264./
    Event date03.08.2009-07.08.2009
    VEvent locationRio de Janeiro
    CountryBR - Brazil
    Event typeWRD
    Languageeng - English
    CountryGB - United Kingdom
    Keywordsturbulence ; radio radiation ; solar-terrestrial relations
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    CEZAV0Z1003909 - ASU-R
    UT WOS000280547700048
    DOI10.1017/S174392130999278X
    AnnotationThe 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.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2011
Number of the records: 1  

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