32 citations · 40 across the 4 of their papers we have counts for
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Spectral Characteristics of Large-Scale Radio Emission Areas in Coronal Holes
D. V. Prosovetsky, I. Yu. Grigoryeva, A. A. Kochanov
The spectra of the coronal hole radio emission in solar cycles 23 and 24 have been studied based on RATAN-600 data in the 4-16.5 GHz range at frequencies of 5.7 and 17 GHz and 327…
Imaging of the solar atmosphere by the Siberian Solar Radio Telescope at 5.7 GHz with an enhanced dynamic range
Alexey Kochanov, Sergey Anfinogentov, Dmitry Prosovetsky +2
The Siberian Solar Radio Telescope (SSRT) is a solar-dedicated directly-imaging interferometer observing the Sun at 5.7 GHz. The SSRT operates in the two-dimensional mode since 199…
The connection of solar wind parameters with microwave and UV emission of coronal hole atmosphere
D. Prosovetsky, I. Myagkova
This paper presents results of comparison between observations of coronal holes in the UV (SOHO EIT) and microwave emission (17, 5.7 GHz, 327 and 150.9 MHz, NoRH, SSRT and Nancy ra…
Induced MHD oscillations of fine loop structures located in coronal hole
S. Anfinogentov, R. Sych, D. Prosovetsky
Many phenomena seen in solar atmosphere are connected with underphotospheric processes. MHD oscillation and other dynamical processes observed in quit sun objects are, for example,…