Observing, modeling and predicting the effects of solar radio bursts on radio communications

Details Observing, modeling and predicting the effects of solar radio bursts on radio communications Observing, modeling and predicting the effects of solar radio bursts on radio communications

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1043..277m&link_type=abstract

EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP Conference Proceedings, Volume 1043, pp. 277-283 (2008).

Statistics

Applications

2

Radiative Processes, Solar Radiation, Artificial Earth Satellites, Corona, Flares, Magnetohydrodynamics And Plasmas, Chromosphere

Scientific paper

The Sun is a source of broadband radio noise, which can reach significantly high levels during outbursts associated with the time evolution of the activity cycle. The statistics point out that the maximum occurrence frequency and intensity of solar radio bursts (SRBs) are observed in the proximity of the activity maximum, but relevant phenomena can occur also in the raising and declining phases of the cycle. Both theoretical estimations based on extensive statistical analyses carried out in recent years and direct observations performed in the past solar activity cycle indicate that solar radio bursts can interfere wireless communications as well as Global Navigation Satellite Systems (GNSS). In this work, we briefly review the theoretical basis and the experimental evidences to date and we show the effectiveness of fast multichannel solar radiopolarimeters, like the Trieste Solar Radio System, in monitoring and predicting solar radio noise increase in the framework of Space Weather applications.

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