Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997arep...41..845y&link_type=abstract
Astronomy Reports, Volume 41, Issue 6, November 1997, pp.845-856
Astronomy and Astrophysics
Astronomy
Scientific paper
Observed sequences of type III solar radio bursts are analyzed taking into account the fact that resonant and self-sustained mechanisms for modulating the radio emission are characterized by different distributions of the pauses between bursts. Modulation of the flux of accelerated electrons during a flare proves to be a stochastic process obeying Poisson statistics (noise), and is not the result of oscillations of any resonant or periodic self-excited systems. Therefore, the observed properties of type III bursts do not confirm the existence of current layers with oscillatory dynamics during flares or the appearance of resonant magnetohydrodynamic oscillations in active regions.
No associations
LandOfFree
On mechanisms for modulating the radio emission of solar flares does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with On mechanisms for modulating the radio emission of solar flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On mechanisms for modulating the radio emission of solar flares will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1686654