The first detection of the solar U+III association with an antenna prototype for the future lunar observatory. (arXiv:2102.02533v2 [astro-ph.IM] UPDATED)

The first detection of the solar U+III association with an antenna prototype for the future lunar observatory. (arXiv:2102.02533v2 [astro-ph.IM] UPDATED)
<a href="http://arxiv.org/find/astro-ph/1/au:+Stanislavsky_L/0/1/0/all/0/1">Lev Stanislavsky</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bubnov_I/0/1/0/all/0/1">Igor Bubnov</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Konovalenko_A/0/1/0/all/0/1">Alexander Konovalenko</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tokarsky_P/0/1/0/all/0/1">Peter Tokarsky</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yerin_S/0/1/0/all/0/1">Serge Yerin</a>

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).

http://arxiv.org/icons/sfx.gif