Siberian Radioheliograph: first results

Author:

Лесовой Сергей1,Lesovoi Sergey2,Алтынцев Александр1,Altyntsev Alexander2,Кочанов Алексей13,Kochanov Aleksey24,Гречнев Виктор1,Grechnev Victor2,Губин Алексей1,Gubin Aleksey2,Жданов Дмитрий1,Zhdanov Dmitriy2,Иванов Евгений1,Ivanov Evgeniy2,Уралов Аркадий1,Uralov Arkadiy2,Кашапова Лариса13,Kashapova Larisa24,Кузнецов Алексей1,Kuznetsov Aleksey2,Мешалкина Наталия1,Meshalkina Nataliya2,Сыч Роберт1,Sych Robert2

Affiliation:

1. Институт солнечно-земной физики СО РАН

2. Institute of Solar Terrestrial Physics SB RAS

3. Иркутский государственный университет

4. Irkutsk State University

Abstract

Regular observations of active processes in the solar atmosphere have been started using the first stage of the multiwave Siberian Radioheliograph (SRH), a T-shaped 48-antenna array with a 4–8 GHz operating frequency range and a 10 MHz instantaneous receiving band. Antennas are set on the central antenna posts of the Siberian Solar Radio Telescope. The maximum baseline is 107.4 m, and the angular resolution is up to 70ʹʹ. We present examples of observations of the solar disk at different frequencies, “negative” bursts, and solar flares. The sensitivity to compact sources reaches 0.01 solar flux units (≈10^{-4} of the total solar flux) with an accumulation time of 0.3 s. The high sensitivity of the SRH enables monitoring of solar activity and allows one to study active processes from characteristics of their microwave emission, including faint events, which could not be detected previously.

Publisher

Infra-M Academic Publishing House

Subject

Space and Planetary Science,Atmospheric Science,Geophysics

Reference34 articles.

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