Siberian Radioheliograph: First Results
Autor: | Robert Sych, S. V. Lesovoi, A. A. Kochanov, A. V. Gubin, E. F. Ivanov, Victor Grechnev, A. M. Uralov, Aleksey Kuznetsov, N. S. Meshalkina, D. A. Zhdanov, L. K. Kashapova, Alexander T. Altyntsev |
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Rok vydání: | 2017 |
Předmět: |
Atmospheric Science
Radio telescopes Negative bursts 010504 meteorology & atmospheric sciences Astrophysics::High Energy Astrophysical Phenomena Negative bursts FOS: Physical sciences lcsh:Astrophysics 01 natural sciences Radio telescope 0103 physical sciences lcsh:QB460-466 Radio telescopes Astrophysics::Solar and Stellar Astrophysics Radio emission 010303 astronomy & astrophysics Solar and Stellar Astrophysics (astro-ph.SR) 0105 earth and related environmental sciences Physics Solar flare Sun Astronomy Geophysics Astrophysics - Solar and Stellar Astrophysics Space and Planetary Science Solar flares Physics::Space Physics Astrophysics::Earth and Planetary Astrophysics |
Zdroj: | Solar-Terrestrial Physics, Vol 3, Iss 1, Pp 3-18 (2017) |
DOI: | 10.48550/arxiv.1704.07100 |
Popis: | 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 mounted 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 70". 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 ($\approx 10^{-4}$ of the total solar flux) with an accumulation time of about 0.3 s. The high sensitivity of SRH enables monitoring of solar activity and allows studying active processes from characteristics of their microwave emission, including faint events, which could not be detected previously. Comment: 14 pages, 12 figures |
Databáze: | OpenAIRE |
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