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Observation of the Solar Eclipse on October 25, 2022 on Radio Telescopes of the Institute of Applied Astronomy, Russian Academy of Sciences (First Results).
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- Geomagnetism & Aeronomy, 2023, v. 63, n. 7, p. 1015, doi. 10.1134/S0016793223070125
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Observation of the Solar Eclipse on October 25, 2022 on Radio Telescopes of the Institute of Applied Astronomy, Russian Academy of Sciences (First Results).
- Published in:
- Geomagnetism & Aeronomy, 2023, v. 63, n. 6, p. 1015, doi. 10.1134/S0016793223070125
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- Publication type:
- Article
Observation of the Solar Eclipse on June 10, 2021 on the Water Vapor Radiometer of the Institute of Applied Astronomy, Russian Academy of Sciences.
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- Geomagnetism & Aeronomy, 2022, v. 62, n. 1, p. S96, doi. 10.1134/S0016793222600643
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Features of Radio-Brightness Distribution over the Solar Disk at Millimeter Waves: Models and Observations.
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- Geomagnetism & Aeronomy, 2021, v. 61, n. 8, p. 1150, doi. 10.1134/S001679322108017X
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Increased Microwave Radiation Brightness as a Sign of Flare-Producing Active Regions Based on Observations of NOAA Active Region 12371.
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- Geomagnetism & Aeronomy, 2021, v. 61, n. 1, p. S24, doi. 10.1134/S0016793222010145
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Tilt Angle of the Magnetic-Field Axis of Sunspots from Microwave Observations: Method and Measurement Results.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 881, doi. 10.1134/S0016793220070257
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Profile of the 9.85-GHz Neutral Hydrogen Line Taking into Account the Zeeman Effect (Computations and Solar Observations).
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- Astronomy Reports, 2019, v. 63, n. 3, p. 229, doi. 10.1134/S1063772919030028
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Cyclotron Line in Solar Microwave Radiation by Radio Telescope RATAN-600 Observations of the Solar Active Region NOAA 12182.
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- Geomagnetism & Aeronomy, 2017, v. 57, n. 7, p. 896, doi. 10.1134/S0016793217070167
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The Gelfreikh-Lubyshev effect according to microwave observations of sunspots.
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- Astrophysical Bulletin, 2016, v. 71, n. 2, p. 232, doi. 10.1134/S1990341316020103
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On the recording of an emission with a reduced brightness in the region of a strong sunspot magnetic field.
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- Cosmic Research, 2015, v. 53, n. 1, p. 10, doi. 10.1134/S0010952515010025
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- Article
Reduced Coronal Emission Above Large Isolated Sunspots.
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- Solar Physics, 2015, v. 290, n. 1, p. 21, doi. 10.1007/s11207-014-0634-3
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'Halo' type sources from microwave observations with high angular resolution.
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- Geomagnetism & Aeronomy, 2014, v. 54, n. 8, p. 1053, doi. 10.1134/S0016793214080155
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Anomalous polarization features of the cyclotron radiation source in the NOAA 7123 active region: The structure, dynamics, and reasons of occurrence.
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- Geomagnetism & Aeronomy, 2013, v. 53, n. 7, p. 1000, doi. 10.1134/S0016793213080185
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Ring-shaped cyclotron radiation source on the example of the NOAA 11140 active region according to high angular resolution observations.
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- Geomagnetism & Aeronomy, 2012, v. 52, n. 7, p. 867, doi. 10.1134/S0016793212070079
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Solar 3.04 cm hydrogen line emission revealed in observations of the active region NOAA 10105.
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- Astronomy Reports, 2011, v. 55, n. 9, p. 841, doi. 10.1134/S1063772911080087
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The microwave radiation of the corona above a large single sunspot in right- and left-circular polarization.
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- Astronomy Reports, 2010, v. 54, n. 1, p. 69, doi. 10.1134/S1063772910010087
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The Tanaka-Enome criterion and solar activity in October-November 2003 as observed by the large pulkovo radio telescope.
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- Cosmic Research, 2004, v. 42, n. 6, p. 561, doi. 10.1007/s10604-005-0003-y
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- Article
Magnetic field of solar prominences: The procedure of radio observations.
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- Astronomische Nachrichten, 1996, v. 317, n. 6, p. 417, doi. 10.1002/asna.2113170607
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- Article