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The first detection of the solar U+III association with an antenna prototype for the future lunar observatory

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arxiv 2102.02533 v3 pith:WW2MVNEW submitted 2021-02-04 astro-ph.IM astro-ph.SR

Lev Stanislavsky , Igor Bubnov , Alexander Konovalenko , Peter Tokarsky , Serge Yerin This is my paper · ORCID
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keywords antennaobservationsprototypesolaractiveanalysisarraysassociation
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We report about observations of the solar U+III bursts on 5 June of 2020 by means of a new active antenna designed to receive radiation in 4-70 MHz. This instrument can serve as a prototype of the ultra-long-wavelength radiotelescope for observations on the farside of the Moon. Our analysis of experimental data is based on simultaneous records obtained with the antenna arrays GURT and NDA in high frequency and time resolution, e-Callisto network as well as by using the space-based observatories STEREO and WIND. The results from this observational study confirm the model of Reid and Kontar (2017).

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