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

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

We report about observations of solar U+III bursts on 2020 June 5 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 radio telescope for observations on the farside of the Moon. Our analysis of experimenta...

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Veröffentlicht in:Research in astronomy and astrophysics 2021-10, Vol.21 (8), p.187-22
Hauptverfasser: Stanislavsky, L. A., Bubnov, I. N., Konovalenko, A. A., Tokarsky, P. L., Yerin, S. N.
Format: Artikel
Sprache:eng
Schlagworte:
Antenna arrays
Antenna design
Antennas
Callisto
methods: data analysis
Moon
Observatories
Prototypes
Radiation
Radio telescopes
Sun: corona
Sun: radio radiation
telescopes
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Beschreibung
Zusammenfassung:We report about observations of solar U+III bursts on 2020 June 5 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 radio telescope 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.
ISSN:1674-4527
DOI:10.1088/1674-4527/21/8/187