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Search for Rotating Radio Transients in the Pushchino Multibeam Survey.
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- Astronomy Letters, 2023, v. 49, n. 10, p. 533, doi. 10.1134/S1063773723090062
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Detection of Two New RRATs at 111 MHz.
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- Astronomy Reports, 2023, v. 67, n. 6, p. 590, doi. 10.1134/S1063772923070077
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Analysis of the Possibilities of Short-Term Prediction of Geomagnetic Perturbations from Observations of Coronal Mass Ejections at the BSA LPI Radio Telescope.
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- Astronomy Reports, 2023, v. 67, n. 6, p. 607, doi. 10.1134/S1063772923060069
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Corotating Disturbances of the Solar Wind in the Monitoring Data of Interplanetary Scintillations: Simulation and Observation.
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- Astronomy Reports, 2023, v. 67, n. 6, p. 618, doi. 10.1134/S1063772923070053
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On the Problems of Detecting Fast Radio Bursts with the LPA LPI.
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- Astronomy Reports, 2023, v. 67, n. 2, p. 163, doi. 10.1134/S106377292302004X
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Search for Pulsars in an Area with Coordinates 3<sup>h</sup> < α < 4<sup>h</sup> and +21° < δ < +42°.
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- Astronomy Reports, 2023, v. 67, n. 2, p. 172, doi. 10.1134/S1063772923020099
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On Correlation of the Interplanetary Scintillation Level and Solar Wind Speed.
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- Astronomy Reports, 2022, v. 66, n. 12, p. 1325, doi. 10.1134/S1063772922110142
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Detection Statistics of Pulse Signals at Declinations from +42° to +52° at the Frequency 111 MHz.
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- Astronomy Reports, 2022, v. 66, n. 4, p. 341, doi. 10.1134/S1063772922040059
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Solar Wind from Maximum to Minimum for Cycle 24 in Interplanetary Scintillation Monitoring Data.
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- Astronomy Reports, 2022, v. 66, n. 1, p. 42, doi. 10.1134/S1063772922010036
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Search for Dispersed Pulses at Declinations from +56° to +87°.
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- Astronomy Reports, 2021, v. 65, n. 12, p. 1246, doi. 10.1134/S1063772921120088
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Geoeffective Disturbances in the Solar Wind near the Solar Activity Minimum according to the Data of a Two-year Series of Observations of Interplanetary Scintillations with the BSA LPI Radio Telescope.
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- Astronomy Reports, 2021, v. 65, n. 11, p. 1150, doi. 10.1134/S1063772921110056
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Search for Periodic Emission from Five Gamma-Ray Pulsars at the Frequency of 111 MHz.
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- Astronomy Reports, 2021, v. 65, n. 9, p. 819, doi. 10.1134/S1063772921100401
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Black Holes and Neutron Stars in an Oscillating Universe.
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- Astrophysical Bulletin, 2021, v. 76, n. 3, p. 229, doi. 10.1134/S199034132103007X
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Comparison of Solar Wind Speed Estimates from Nearly Simultaneous IPS Observations at 327 and 111 MHz.
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- Solar Physics, 2021, v. 296, n. 4, p. 1, doi. 10.1007/s11207-021-01804-6
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Monitoring of Interplanetary Scintillation and Potential of Short-time Space Weather Forecasting.
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- Russian Meteorology & Hydrology, 2021, v. 46, n. 3, p. 150, doi. 10.3103/S106837392103002X
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Detection of Five New Pulsars with the BSA LPI Radio Telescope.
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- Astronomy Reports, 2020, v. 64, n. 6, p. 526, doi. 10.1134/S1063772920060074
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Study of Bright Compact Radio Sources of the Northern Hemisphere at 111 MHz.
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- Astronomy Reports, 2020, v. 64, n. 5, p. 406, doi. 10.1134/S1063772920060062
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Corotating and Propagating Disturbances in the Solar Wind Based on Monitoring of Interplanetary Scintillations at the LPA Radio Telescope of the Lebedev Physical Institute in 2017.
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- Astronomy Reports, 2020, v. 64, n. 1, p. 66, doi. 10.1134/S1063772920010084
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Search for Long-term Variability of Several Flat-Spectrum Sources at 111 MHz.
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- Astronomy Reports, 2019, v. 63, n. 11, p. 920, doi. 10.1134/S1063772919100068
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Single‐Site IPS Power Spectra Analysis for Space Weather Products Using Cross‐Correlation Function Results From EISCAT and MERLIN IPS Data.
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- Space Weather: The International Journal of Research & Applications, 2019, v. 17, n. 7, p. 1114, doi. 10.1029/2018SW002142
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Studies of the Angular Structure of Scintillating Radio Sources at 111 MHz.
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- Astronomy Reports, 2019, v. 63, n. 6, p. 479, doi. 10.1134/S1063772919060064
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Observations of Corotating Streams of the Solar Wind with the Large Phased Array of the Lebedev Physical Institute in 2016.
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- Astronomy Reports, 2019, v. 63, n. 5, p. 409, doi. 10.1134/S1063772919050019
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Global Structure of the Solar Wind in a of Decreasing Solar Activity from Interplanetary-Scintillation Monitoring Data.
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- Astronomy Reports, 2019, v. 63, n. 2, p. 161, doi. 10.1134/S1063772919020021
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Coronal Mass Ejections in September 2017 from Monitoring of Interplanetary Scintillations with the Large Phased Array of the Lebedev Institute of Physics.
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- Astronomy Reports, 2018, v. 62, n. 5, p. 346, doi. 10.1134/S1063772918050025
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Detection of Five New RRATs at 111 MHz.
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- Astronomy Reports, 2018, v. 62, n. 1, p. 63, doi. 10.1134/S1063772918010079
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Search for and detection of pulsars inmonitoring observations at 111 MHz.
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- Astronomy Reports, 2017, v. 61, n. 10, p. 848, doi. 10.1134/S1063772917100109
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Corotating structures in the solar wind from 111-MHz observations of interplanetary scintillations at large elongations.
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- Astronomy Reports, 2017, v. 61, n. 3, p. 233, doi. 10.1134/S1063772917030040
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Monitoring of the turbulent solar wind with the upgraded Large Phased Array of the Lebedev Institute of Physics: First results.
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- Astronomy Reports, 2016, v. 60, n. 12, p. 1067, doi. 10.1134/S1063772916110068
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Interplanetary and ionosphere scintillation produced by ICME 20 December 2015.
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- Space Weather: The International Journal of Research & Applications, 2016, v. 14, n. 9, p. 682, doi. 10.1002/2016SW001455
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Compilation of a complete sample of giant radio sources from a survey at 102.5 MHz.
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- Astronomy Reports, 2016, v. 60, n. 8, p. 718, doi. 10.1134/S1063772916070027
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Interplanetary scintillations of the radio source ensemble at the maximum of cycle 24 of solar activity.
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- Cosmic Research, 2016, v. 54, n. 3, p. 178, doi. 10.1134/S0010952516010032
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Detection of new pulsars at 111 MHz.
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- Astronomy Reports, 2016, v. 60, n. 2, p. 220, doi. 10.1134/S1063772916020128
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Interplanetary Scintiallation (IPS) of the Radio Source 3C48 During Periods of Low and High Solar Activity.
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- Solar Physics, 2015, v. 290, n. 9, p. 2567, doi. 10.1007/s11207-015-0764-2
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Global Structure of the Turbulent Solar Wind during 24 Solar Activity Maxima from IPS Observations with the Multibeam Radio Telescope BSA LPI at 111 MHz.
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- Solar Physics, 2015, v. 290, n. 9, p. 2577, doi. 10.1007/s11207-015-0703-2
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Parameters of the turbulence of the interplanetary plasma derived from scintillation observations of the quasars 3C 48 and 3C 298 at the solar-activity maximum.
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- Astronomy Reports, 2015, v. 59, n. 1, p. 33, doi. 10.1134/S1063772915010035
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Interplanetary-scintillation observations of coronal mass ejections near the maximum of the 24th solar-activity cycle.
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- Astronomy Reports, 2015, v. 59, n. 1, p. 40, doi. 10.1134/S1063772915010047
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The detection of coronal mass ejections in the interplanetary medium using scintillation observations.
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- Astronomy Reports, 2014, v. 58, n. 9, p. 619, doi. 10.1134/S1063772914090030
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Parameters of the turbulence of the interplanetary plasma derived from scintillation observations of the quasar 3C 48 at the solar-activity minimum.
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- Astronomy Reports, 2013, v. 57, n. 8, p. 586, doi. 10.1134/S1063772913070020
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Determining source angular sizes from interplanetary-scintillation observations in the saturated regime.
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- Astronomy Reports, 2013, v. 57, n. 7, p. 509, doi. 10.1134/S1063772913070032
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Results of IPS Observations in the Period Near Solar Activity Minimum.
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- Solar Physics, 2013, v. 285, n. 1/2, p. 141, doi. 10.1007/s11207-012-9952-5
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The radio sources CTA 21 and OF+247: The hot spots of radio galaxies.
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- Astronomy Reports, 2013, v. 57, n. 6, p. 423, doi. 10.1134/S1063772913050016
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Giant radio-galaxy candidates at declinations from 3.5° to 12°.
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- Astronomy Reports, 2013, v. 57, n. 1, p. 1, doi. 10.1134/S1063772913010034
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Interplanetary scintillations of an ensemble of radio sources during the solar activity minimum of cycles 23/24.
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- Cosmic Research, 2013, v. 51, n. 1, p. 23, doi. 10.1134/S0010952513010024
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Physical conditions in the hot spots of the radio galaxy Cygnus A.
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- Astronomy Reports, 2012, v. 56, n. 9, p. 680, doi. 10.1134/S1063772912090016
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The physical conditions in the core of the quasar 3C 273 on parsec scales.
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- Astronomy Reports, 2012, v. 56, n. 7, p. 483, doi. 10.1134/S1063772911100015
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Interplanetary scintillations of strong radio sources in the descending phase near the cycle 23 minimum.
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- Geomagnetism & Aeronomy, 2011, v. 51, n. 6, p. 794, doi. 10.1134/S0016793211060053
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Interplanetary and Ionosphere Scintillation Monitoring of Radio Sources Ensemble at the Solar Activity Minimum.
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- Solar Physics, 2010, v. 265, n. 1/2, p. 277, doi. 10.1007/s11207-010-9565-9
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The magnetic fields and density of relativistic electrons in the nucleus of NGC 1052.
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- Astronomy Reports, 2009, v. 53, n. 11, p. 988, doi. 10.1134/S1063772909110031
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Study of compact radio sources using interplanetary scintillations at 111 MHz. Strong gigahertz-peaked spectrum sources.
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- Astronomy Reports, 2009, v. 53, n. 4, p. 310, doi. 10.1134/S1063772909040039
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Study of compact radio sources using interplanetary scintillations at 111 MHz. Compact symmetric objects.
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- Astronomy Reports, 2009, v. 53, n. 4, p. 319, doi. 10.1134/S1063772909040040
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