Radio signature of multi-scaling flare loop interactions

Details Radio signature of multi-scaling flare loop interactions Radio signature of multi-scaling flare loop interactions

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..737r&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Sun: Flares, Sun: Radio Radiation, Method: Spectral Analysis

Scientific paper

The solar radio emission at 3 GHz observed during the June 6, 2000 flare, at times when the EIT/SOHO and SXT/Yohkoh images indicate the flare loop interactions, has been analyzed for its complex temporal variability. Using the Fourier Power Spectrum (FPS) and the Global Wavelet Spectrum (GWS) techniques the power spectra of the 3 GHz signal, observed with time resolution of 0.6 s, have been determined: a 1/f1.66±0.16 power law. The presence of a characteristic power-law implies that the fluctuations are stochastically correlated without a dominant characteristic spatio-temporal scale and contain some self-similarity in time.

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