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Expansion and Compression of a Flare Loop System during the Flare on January 15, 2022 According to Ultraviolet and Microwave Data.
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- Geomagnetism & Aeronomy, 2023, v. 63, n. 7, p. 1054, doi. 10.1134/S0016793223070162
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Expansion and Compression of a Flare Loop System during the Flare on January 15, 2022 According to Ultraviolet and Microwave Data.
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- Geomagnetism & Aeronomy, 2023, v. 63, n. 6, p. 1054, doi. 10.1134/S0016793223070162
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- Article
Analysis of the Properties of SEP Events and Their Solar Sources Taking Into Account of the Magneto-Morphological Classification of Active Regions.
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- Geomagnetism & Aeronomy, 2021, v. 61, n. 7, p. 1022, doi. 10.1134/S0016793221070082
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Relation between the active region magnetic field and solar flares.
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- Geomagnetism & Aeronomy, 2013, v. 53, n. 6, p. 690, doi. 10.1134/S001679321306011X
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Effect of a self-induced electric field on the electron beam kinetics and resulting hard X-ray and microwave emissions in flares.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 8, p. 1029, doi. 10.1134/S0016793211080329
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An Extreme Solar Event of 20 January 2005: Properties of the Flare and the Origin of Energetic Particles.
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- Solar Physics, 2008, v. 252, n. 1, p. 149, doi. 10.1007/s11207-008-9245-1
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Microwave Type III-Like Bursts as Possible Signatures of Magnetic Reconnection.
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- Solar Physics, 2007, v. 242, n. 1/2, p. 111, doi. 10.1007/s11207-007-0207-9
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On the wave mode of subsecond pulses in the cm-range.
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- Solar Physics, 2004, v. 221, n. 1, p. 85, doi. 10.1023/B:SOLA.0000033356.96547.65
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- Article
Mysteries of the 17 May 2012 Solar Event Responsible for GLE71. I. CME Development and the Role of Disturbances Excited by Eruptions.
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- Solar Physics, 2024, v. 299, n. 9, p. 1, doi. 10.1007/s11207-024-02373-0
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Relationships Between the Spectra of Near-Earth Proton Enhancements, Hard X-Ray Bursts, and CME Speeds.
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- Solar Physics, 2022, v. 297, n. 5, p. 1, doi. 10.1007/s11207-022-01986-7
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Twin Null-Point-Associated Major Eruptive Three-Ribbon Flares with Unusual Microwave Spectra.
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- Solar Physics, 2020, v. 295, n. 9, p. N.PAG, doi. 10.1007/s11207-020-01702-3
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- Article
Sources of Quasi-periodic Pulses in the Flare of 18 August 2012.
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- Solar Physics, 2016, v. 291, n. 2, p. 445, doi. 10.1007/s11207-016-0846-9
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Relations Between Microwave Bursts and Near-Earth High-Energy Proton Enhancements and Their Origin.
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- Solar Physics, 2015, v. 290, n. 10, p. 2827, doi. 10.1007/s11207-015-0797-6
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- Article
Study of Flare Energy Release Using Events with Numerous Type III-like Bursts in Microwaves.
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- Solar Physics, 2012, v. 280, n. 2, p. 537, doi. 10.1007/s11207-012-0065-y
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Detection of Acceleration Processes During the Initial Phase of the 12 June 2010 Flare.
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- Solar Physics, 2012, v. 280, n. 2, p. 525, doi. 10.1007/s11207-012-0080-z
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Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. I. Reconciliation of 'EIT Waves', Type II Radio Bursts, and Leading Edges of CMEs.
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- Solar Physics, 2011, v. 273, n. 2, p. 433, doi. 10.1007/s11207-011-9780-z
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Radioheliograph Observations of Microwave Bursts with Zebra Structures.
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- Solar Physics, 2011, v. 273, n. 1, p. 163, doi. 10.1007/s11207-011-9856-9
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- Article
High-Energy Emission from a Solar Flare in Hard X-rays and Microwaves.
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- Solar Physics, 2009, v. 260, n. 1, p. 135, doi. 10.1007/s11207-009-9437-3
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Temporal and spatial association between microwaves and type III bursts in the upper corona.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 671, p. 1, doi. 10.1051/0004-6361/202244599
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Dynamics of magnetic fields of active regions in pre-flare states and during solar flares.
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- Astronomy Reports, 2015, v. 59, n. 8, p. 795, doi. 10.1134/S1063772915080065
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Simulation of the current sheet in a flare-active region and comparison to radio data.
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- Solar System Research, 2007, v. 41, n. 4, p. 322, doi. 10.1134/S0038094607040053
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On the correlation between spectra of solar microwave bursts and proton fluxes near the Earth.
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- Astronomy Reports, 2009, v. 53, n. 11, p. 1059, doi. 10.1134/S1063772909110110
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