Date of upload:
19.10.2015
Co-author:
Francisco C. R. Fernandes
Abstract:
We report the analysis of the observational parameters of the two Radio Noise Storms (RNS): one day in the occurrence of the solar flares in X-rays and one day without the presence of the flare. The spectral information about the chains of type I in the events obtained of the network e-CALLISTO (Compact Astronomical Low-cost Low-frequency Instrument for Spectroscopy and Transportable Observatory) revealed in 07/05/2011 (day without flare) bandwidth in the range 5.7 {-}{-} 91 MHz, the duration varied from 7 {-}{-} 361 seconds, and the frequency drift-rate was in the range -5.2 {-}{-} +2.5 MHzs$^{-1}$. Day whit flare (01/08/2011) presented bandwidth in the range 4.7 {-}{-} 60 MHz, duration between 6 and 214 seconds and frequency drift-rate varied from -6 to +1.8 MHzs$^{-1}$.
