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Noise storms, also called of type I noise storms, are solar emissions in
metric waves that originate in regions of high concentration of the magnetic field,
such as active regions, and often are related to distinct changes in the solar
corona and the release of energy, adjacent of the active region. The active regions
are classified according to the complexity of the spots that make it up. Solar
emission type I in metric waves is associated with active regions, but not directly
to flares. Using data of the NOAA it was found that on days with the presence of
flares have a larger number of storms and also more lasting. However, for days
without the presence of type I flares occurred storms. Associated with storms are
the chains of type I, whose spectral characteristics can be observed with high
spectral and temporal resolution instruments such as the spectrographs of network
e-CALLISTO. This work investigates the observational and physical parameters the
chains of type I associated with the storms of the day 09/08/2011 (with the presence of flares)
and the day 07/05/2011 (without the presence of flares). The results are presented
and discussed. |
