Solar radio emission as a disturbance of aeronautical radionavigation
C. Marqu\'e, K.-L. Klein, C. Monstein, H. Opgenoorth, A. Pulkkinen, S., Buchert, S. Krucker, R. Van Hoof, P. Thulesen

TL;DR
This study links a strong solar radio burst around 1 GHz to disturbances in aeronautical radar and GPS signals, highlighting the need for real-time monitoring to mitigate space weather impacts.
Contribution
It identifies a specific solar radio burst as the cause of radar disturbances and emphasizes the importance of continuous Sun radio flux monitoring for space weather prediction.
Findings
Solar radio burst coincides with radar disturbances.
Radio burst is due to coherent emission processes.
Monitoring instruments can help identify and mitigate disturbances.
Abstract
On November 4th 2015 secondary air traffic control radar was strongly disturbed in Sweden and some other European countries. The disturbances occurred when the radar antennas were pointing at the Sun. In this paper, we show that the disturbances coincided with the time of peaks of an exceptionally strong ( Solar Flux Units) solar radio burst in a relatively narrow frequency range around 1~GHz. This indicates that this radio burst is the most probable space weather candidate for explaining the radar disturbances. The dynamic radio spectrum shows that the high flux densities are not due to synchrotron emission of energetic electrons, but to coherent emission processes, which produce a large variety of rapidly varying short bursts (such as pulsations, fiber bursts, and zebra patterns). The radio burst occurs outside the impulsive phase of the associated flare, about 30 minutes…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Astro and Planetary Science
