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Reduced Coronal Emission Above Large Isolated Sunspots

Solar physics, 2015-01, Vol.290 (1), p.21-35

2015

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Features of the Spectra of Microwave Sources above Sunspots Inferred from Observations with RATAN-600

Astrophysical bulletin, 2024-06, Vol.79 (2), p.304-320

2024

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Increased Microwave Radiation Brightness as a Sign of Flare-Producing Active Regions Based on Observations of NOAA Active Region 12371

Geomagnetism and Aeronomy, 2021-12, Vol.61 (Suppl 1), p.S24-S35

2021

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Observation of the Solar Eclipse on June 10, 2021 on the Water Vapor Radiometer of the Institute of Applied Astronomy, Russian Academy of Sciences

Geomagnetism and Aeronomy, 2022-12, Vol.62 (Suppl 1), p.S96-S102

2022

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“Halo” type sources from microwave observations with high angular resolution

Geomagnetism and Aeronomy, 2014-12, Vol.54 (8), p.1053-1057

2014

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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)

Geomagnetism and Aeronomy, 2023-12, Vol.63 (7), p.1015-1023

2023

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On the recording of an emission with a reduced brightness in the region of a strong sunspot magnetic field

Cosmic research, 2015, Vol.53 (1), p.10-20

2015

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Cyclotron Line in Solar Microwave Radiation by Radio Telescope RATAN-600 Observations of the Solar Active Region NOAA 12182

Geomagnetism and Aeronomy, 2017-12, Vol.57 (7), p.896-901

2017

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The microwave radiation of the corona above a large single sunspot in right- and left-circular polarization

Astronomy reports, 2010, Vol.54 (1), p.69-85

2010

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Solar 3.04 cm hydrogen line emission revealed in observations of the active region NOAA 10105

Astronomy reports, 2011-09, Vol.55 (9), p.841-848

2011

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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

Geomagnetism and Aeronomy, 2013-12, Vol.53 (8), p.1000-1006

2013

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Ring-shaped cyclotron radiation source on the example of the NOAA 11140 active region according to high angular resolution observations

Geomagnetism and Aeronomy, 2012-12, Vol.52 (7), p.867-874

2012

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Tilt Angle of the Magnetic-Field Axis of Sunspots from Microwave Observations: Method and Measurement Results

Geomagnetism and aeronomy, 2020-12, Vol.60 (7), p.881-888

2020

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Studying the solar corona above active regions from microwave observations during solar flares recorded by CORONAS-F satellite

Geomagnetism and Aeronomy, 2006-10, Vol.46 (5), p.547-554

2006

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Profile of the 9.85-GHz Neutral Hydrogen Line Taking into Account the Zeeman Effect (Computations and Solar Observations)

Astronomy reports, 2019-03, Vol.63 (3), p.229-237

2019

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Features of Radio-Brightness Distribution over the Solar Disk at Millimeter Waves: Models and Observations

Geomagnetism and aeronomy, 2021-12, Vol.61 (8), p.1150-1158

2021

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The Tanaka-Enome criterion and solar activity in October?November 2003 as observed by the Large Pulkovo Radio Telescope

Cosmic research, 2004-11, Vol.42 (6), p.561-570

2004

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The Gelfreikh–Lubyshev effect according to microwave observations of sunspots

Astrophysical bulletin, 2016-04, Vol.71 (2), p.232-240

2016

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The Microwave Radiation of the Corona above a Large Single Sunspot in Right- and Left-Circular Polarization

Astronomy reports, 2010, Vol.54 (1), p.69-85

2010

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Solar 3.04 cm Hydrogen Line Emission Revealed in Observations of the Active Region NOAA 10105

Astronomy reports, 2011, Vol.55 (9), p.841-848

2011

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Distribution of the longitudinal component of the magnetic field of prominences from radioastronomical measurements

Radiophysics and quantum electronics, 1996-11, Vol.39 (11-12), p.962-966

1996

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Magnetic field of solar prominences: The procedure of radio observations

Astronomische Nachrichten, 1996, Vol.317 (6), p.417-421

1996

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Microwave study of coronal active regions from the CORONAS-F list of solar flares observed in Gamma- and X- rays

Proceedings of the International Astronomical Union, 2004-06, Vol.2004 (IAUS223), p.223-224

2004

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Sharp Changes in the Ordinary Mode Microwave Emission from a Stable Sunspot: Model Analysis

Latvian journal of physics and technical sciences, 2011-04, Vol.48 (2), p.56

2011

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Reduced Coronal Emission Above Large Isolated Sunspots

Features of the Spectra of Microwave Sources above Sunspots Inferred from Observations with RATAN-600

Increased Microwave Radiation Brightness as a Sign of Flare-Producing Active Regions Based on Observations of NOAA Active Region 12371

Observation of the Solar Eclipse on June 10, 2021 on the Water Vapor Radiometer of the Institute of Applied Astronomy, Russian Academy of Sciences

“Halo” type sources from microwave observations with high angular resolution

Observation of the Solar Eclipse on October 25, 2022 on Radio Telescopes of the Institute of Applied Astronomy, Russian Academy of Sciences (First Results)

On the recording of an emission with a reduced brightness in the region of a strong sunspot magnetic field

Cyclotron Line in Solar Microwave Radiation by Radio Telescope RATAN-600 Observations of the Solar Active Region NOAA 12182

The microwave radiation of the corona above a large single sunspot in right- and left-circular polarization

Solar 3.04 cm hydrogen line emission revealed in observations of the active region NOAA 10105

Anomalous polarization features of the cyclotron radiation source in the NOAA 7123 active region: The structure, dynamics, and reasons of occurrence

Ring-shaped cyclotron radiation source on the example of the NOAA 11140 active region according to high angular resolution observations

Tilt Angle of the Magnetic-Field Axis of Sunspots from Microwave Observations: Method and Measurement Results

Studying the solar corona above active regions from microwave observations during solar flares recorded by CORONAS-F satellite

Profile of the 9.85-GHz Neutral Hydrogen Line Taking into Account the Zeeman Effect (Computations and Solar Observations)

Features of Radio-Brightness Distribution over the Solar Disk at Millimeter Waves: Models and Observations

The Tanaka-Enome criterion and solar activity in October?November 2003 as observed by the Large Pulkovo Radio Telescope

The Gelfreikh–Lubyshev effect according to microwave observations of sunspots

The Microwave Radiation of the Corona above a Large Single Sunspot in Right- and Left-Circular Polarization

Solar 3.04 cm Hydrogen Line Emission Revealed in Observations of the Active Region NOAA 10105

Distribution of the longitudinal component of the magnetic field of prominences from radioastronomical measurements

Magnetic field of solar prominences: The procedure of radio observations

Microwave study of coronal active regions from the CORONAS-F list of solar flares observed in Gamma- and X- rays

Sharp Changes in the Ordinary Mode Microwave Emission from a Stable Sunspot: Model Analysis

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