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

作　　者：L.A.Stanislavsky I.N.Bubnov A.A.Konovalenko P.L.Tokarsky S.N.Yerin 

机构地区：[1]Institute of Radio Astronomy,Kharkiv,Ukraine [2]V.N.Karazin Kharkiv National University,Kharkiv,Ukraine

出　　处：《Research in Astronomy and Astrophysics》2021年第8期16-22,共7页天文和天体物理学研究（英文版）

基　　金：partially supported by Research Grant (0120U101334);the National Academy of Sciences of Ukraine for this support。

摘　　要：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 ultralong-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.

关 键 词：Sun:corona Sun:radio radiation methods:data analysis telescopes 

分 类 号：P16[天文地球—天文学]