Публикации
Публикации по данным Горной Астрономической Станции
2025
• Study of the Red Coronal Line with Altitude from Out-of-Eclipse Observations during Solar Cycle 24. Cosmic Research, vol. 63, pp. 47--55, 2025. DOI: 10.1134/S0010952524601440
• Temporal and Structural Properties of Sunspot Small Short-living Group and Large Long-living Group Populations. The Astrophysical Journal, vol. 987, no. 2, pp. 136, 2025. DOI: 10.3847/1538-4357/ade13a
• Machine learning methods in solar physics. Physics Uspekhi, vol. 68, pp. 374--392, 2025. DOI: 10.3367/UFNe.2025.02.039872
• SOHO/MDI and SDO/HMI sunspot area measurement and analysis. RAS Techniques and Instruments, vol. 4, pp. rzaf024, 2025. DOI: 10.1093/rasti/rzaf024
2024
• Interactive multi-instrumental database of solar activity observations. pp. 944--948, 2024. DOI: 10.26119/VAK2024.180
• Formation of Near-Surface Magnetic Fields of the Sun. Geomagnetism and Aeronomy, vol. 64, pp. 1176--1181, 2024. DOI: 10.1134/S0016793224700269
• Modeling the Solar Wind Speed Based on Various Parameters of the Coronal Magnetic Field. Geomagnetism and Aeronomy, vol. 63, pp. 1298--1307, 2024. DOI: 10.1134/S0016793223080042
• Recovery of a Large-Scale Magnetic Field Using the Stokes I-Profile Approximation Method. Geomagnetism and Aeronomy, vol. 63, pp. 1180--1184, 2024. DOI: 10.1134/S0016793223080248
• Sunspot Magnetic Field Measurements at MWO and CrAO: Radio Emission F10.7 during the Declining and Minimum Phase of Solar Cycle 24. Geomagnetism and Aeronomy, vol. 63, pp. 1144--1148, 2024. DOI: 10.1134/S0016793223080029
• Differential Rotation of Individual Sunspots and Pores. The Astrophysical Journal, vol. 977, no. 1, pp. 110, 2024. DOI: 10.3847/1538-4357/ad90a0
• Pre-impulsive and Impulsive Phases of the Sub-Terahertz Flare of March 28, 2022. Geomagnetism and Aeronomy, vol. 63, pp. 1218--1223, 2024. DOI: 10.1134/S0016793223080157
• WAVELET PREVIEW FOR NON-LINEAR DYNAMICS OF SOLAR FACULAE. Voyage Journal of Scientific Research and Exploration, vol. 1, no. 2, pp. 14--27, 2024. DOI: 10.58622/cqnxsz04
• Solar Wind and Space Weather. Eruptions on the Sun, pp. 361--387, 2024. DOI: 10.1007/978-3-031-58177-9_12
• Evaluation of Sunspot Areas Derived by Automated Sunspot-Detection Methods. Solar Physics, vol. 299, no. 11, pp. 156, 2024. DOI: 10.1007/s11207-024-02402-y
2023
• Solar Filament Eruptions in Hα Doppler Velocity. The Astrophysical Journal, vol. 950, no. 2, pp. 100, 2023. DOI: 10.3847/1538-4357/acd113
• Güneş'teki Aktif Bölgelerin Öbeklenme Eğilimi. Turkish Journal of Astronomy and Astrophysics, vol. 4, pp. 166--168, 2023. DOI: 10.55064/tjaa.1200117
• Near-Surface Azimuthal Magnetic Fields and Their Role in Solar Activity Cycles. Solar Physics, vol. 298, pp. 147, 2023. DOI: 10.1007/s11207-023-02239-x
• Unsupervised learning of active-region nesting on the Sun. pp. EGU--850, 2023. DOI: 10.5194/egusphere-egu23-850
• Study of the Green Coronal Line with Altitude from Out-of-Eclipse Observations during Solar Cycle 24. Cosmic Research, vol. 61, pp. 133--141, 2023. DOI: 10.1134/S0010952522700162
• A Prototype of a Background Solar Wind Forecasting Service Based on MHD Modeling and WSA Boundary Conditions. Cosmic Research, vol. 61, no. 6, pp. 457--463, 2023. DOI: 10.1134/S0010952523700508
• Modeling the Magnetic Field of the Inner Corona in a Radially Expanding Solar Wind. Physics, vol. 5, no. 1, pp. 161--167, 2023. DOI: 10.3390/physics5010012
• Extreme Values of Sunspot Activity on a Long Time Scale. Astronomy Letters, vol. 49, no. 7, pp. 421--429, 2023. DOI: 10.1134/S1063773723070034
2022
• Magnetograph Saturation and the Open Flux Problem. The Astrophysical Journal, vol. 926, pp. 113, 2022. DOI: 10.3847/1538-4357/ac4491
• Coronal Field Geometry and Solar Wind Speed. Universe, vol. 8, pp. 646, 2022. DOI: 10.3390/universe8120646
• Observations of Chromospheric Flows of Matter in Active Regions of the Sun. Geomagnetism and Aeronomy, vol. 62, pp. 862--868, 2022. DOI: 10.1134/S0016793222070064
• Analysis of the Area in Groups of Sunspots of Different Classes. Geomagnetism and Aeronomy, vol. 62, pp. 839--844, 2022. DOI: 10.1134/S0016793222070179
• The Shape of Sunspots and Solar Activity Cycles. Solar Physics, vol. 297, no. 8, pp. 110, 2022. DOI: 10.1007/s11207-022-02045-x
• Revisiting Christoph Scheiner’s Sunspot Records: A New Perspective on Solar Activity of the Early Telescopic Era. The Astrophysical Journal, vol. 927, no. 2, pp. 193, 2022. DOI: 10.3847/1538-4357/ac52ee
• Parametrization of Sunspot Groups Based on Machine-Learning Approach. Solar Physics, vol. 297, no. 2, pp. 19, 2022. DOI: 10.1007/s11207-022-01955-0
• Dark Dots on the Photosphere and Their Counting in the Sunspot Index. Solar Physics, vol. 297, no. 6, pp. 67, 2022. DOI: 10.1007/s11207-022-02002-8
• Изучение Эффекта Вильсона По Данным Анализа Усредненных Форм Солнечных Пятен. pp. 267--270, 2022. DOI: 10.31725/0552-5829-2022-267-270
• Reconstructing solar magnetic fields from historical observations - IX. The photospheric magnetic field from 1915 to 1985. Astronomy Astrophysics, vol. 667, pp. A168, 2022. DOI: 10.1051/0004-6361/202244372
• Variations in Daily Maximum Areas and Longitudinal Widths of Solar Coronal Holes in 2017–2020. Universe, vol. 8, no. 3, pp. 158, 2022. DOI: 10.3390/universe8030158
2021
• Restoration of the Profile of Chromospheric Lines in Quiet and Active Areas of the Sun. Geomagnetism and Aeronomy, vol. 61, pp. 1075--1082, 2021. DOI: 10.1134/S0016793221070033
• Processing of Observations of the Partial Solar Eclipse on June 21, 2020, in the 3.2- and 4.9-cm Wavelength Regions at the Mountain Astronomical Station of the Central Astronomical Observatory. Geomagnetism and Aeronomy, vol. 61, pp. 905--909, 2021. DOI: 10.1134/S001679322106013X
• "Generative" Indices of Sunspot Solar Activity: 145-Year Composite Series. Solar Physics, vol. 296, pp. 32, 2021. DOI: 10.1007/s11207-021-01772-x
• Average annual total sunspot area in the last 410 yr: the most probable values and limits of their uncertainties. Monthly Notices of the Royal Astronomical Society, vol. 505, pp. 1206--1212, 2021. DOI: 10.1093/mnras/stab1328
• On the size distribution of spots within sunspot groups. Astronomy and Astrophysics, vol. 652, pp. A9, 2021. DOI: 10.1051/0004-6361/202140621
• Bi-lognormal Distribution of Sunspot Group Areas. The Astrophysical Journal, vol. 906, pp. 27, 2021. DOI: 10.3847/1538-4357/abc82d
• Strong evidence of low levels of solar activity during the Maunder Minimum. Monthly Notices of the Royal Astronomical Society, vol. 504, no. 4, pp. 5199--5204, 2021. DOI: 10.1093/mnras/stab1155
• Long-term evolution of coronal holes on the Sun and occurrence frequencies of magnetic storms with gradual commencements. Journal of Physics: Conference Series, vol. 2103, no. 1, pp. 012038, 2021. DOI: 10.1088/1742-6596/2103/1/012038
• Long-term studies of photospheric magnetic fields on the Sun. Journal of Space Weather and Space Climate, vol. 11, pp. 4, 2021. DOI: 10.1051/swsc/2020069
• Comparative Analysis of Fractal Properties of Solar Faculae. International Journal of Economic and Environmental Geology (IJEEG), vol. 12, no. 2, pp. 50--59, 2021.
• Deciphering Solar Magnetic Activity: 140 Years of the ‘Extended Solar Cycle’ – Mapping the Hale Cycle. Solar Physics, vol. 296, no. 12, pp. 189, 2021. DOI: 10.1007/s11207-021-01938-7
• The Effect of Missing Groups in the Calculation of the Solar Irradiance Deficit. Solar Physics, vol. 296, no. 10, pp. 149, 2021. DOI: 10.1007/s11207-021-01893-3
• Is the F10.7cm - Sunspot Number relation linear and stable?. Journal of Space Weather and Space Climate, vol. 11, pp. 2, 2021. DOI: 10.1051/swsc/2020071
2020
• Sunspot area catalog revisited: Daily cross-calibrated areas since 1874. Astronomy and Astrophysics, vol. 640, pp. A78, 2020. DOI: 10.1051/0004-6361/202037547
• Comparative Analysis of Terrestrial and Satellite Observations of Photospheric Magnetic Field in an Appendix to Simulation of Parameters of Coronal Holes and Solar Wind. Geomagnetism and Aeronomy, Volume 60, Issue 7, pp. 872-875, vol. 60, no. 7, pp. 872, 2020. DOI: 10.1134/S0016793220070051
• VizieR Online Data Catalog: Plage area composite series (Chatzistergos+, 2020). VizieR Online Data Catalog, vol. 363, pp. J/A+A/639/A88, 2020. DOI: 10.26093/cds/vizier.36390088
• VizieR Online Data Catalog: Sunspot area catalogue revisited (1874-2019) (Mandal+, 2020). VizieR Online Data Catalog, vol. 364, pp. J/A+A/640/A78, 2020. DOI: 10.26093/cds/vizier.36400078
• Drift of Polar Prominences in Solar Cycles 13-24. Geomagnetism and Aeronomy, vol. 59, pp. 1022--1028, 2020. DOI: 10.1134/S001679321908022X
• Continuous 60-Year Observations of the Spectral Solar Corona at the Mountain Astronomical Station of Pulkovo Observatory. Geomagnetism and Aeronomy, vol. 59, pp. 864--869, 2020. DOI: 10.1134/S0016793219070168
• Comparative Analysis of the Catalog of Individual Sunspots Based on Data from Kislovodsk Mountain Astronomical Station. Geomagnetism and Aeronomy, vol. 59, pp. 793--798, 2020. DOI: 10.1134/S0016793219070235
• Simulation of Coronal Mass Ejection Propagation Based on Data from Ground-Based Patrol Observations. Geomagnetism and Aeronomy, vol. 59, pp. 843--845, 2020. DOI: 10.1134/S0016793219070247
• Solar cycle prediction. Living Reviews in Solar Physics, vol. 17, pp. 2, 2020. DOI: 10.1007/s41116-020-0022-z
• Machine-learning Approach to Identification of Coronal Holes in Solar Disk Images and Synoptic Maps. The Astrophysical Journal, vol. 903, no. 2, pp. 115, 2020. DOI: 10.3847/1538-4357/abb94d
• A New Comprehensive Data Set of Solar Filaments of 100 yr Interval. I.. The Astrophysical Journal Supplement Series, vol. 249, no. 1, pp. 11, 2020. DOI: 10.3847/1538-4365/ab92a5
• Observation of the Radio Radiation Flux of the Sun and Flares at a Wavelength of 5 cm. Geomagnetism and Aeronomy, vol. 60, no. 8, pp. 1087--1092, 2020. DOI: 10.1134/S0016793220080241
• Переменная звезда Солнце и его магнитное поле. Земля И Вселенная, no. 4, pp. 45--58, 2020. DOI: 10.7868/S0044394820040052
• Prediction of Solar Flares and Background Fluxes of X-Ray Radiation According to Synoptic Ground-Based Observations Using Machine-Learning Models. Cosmic Research, vol. 58, no. 6, pp. 444--449, 2020. DOI: 10.1134/S0010952520060106
• Analysis of full-disc Ca II K spectroheliograms - III. Plage area composite series covering 1892–2019. Astronomy Astrophysics, vol. 639, pp. A88, 2020. DOI: 10.1051/0004-6361/202037746
• Analysis of full-disc Ca II K spectroheliograms. III. Plage area composite series covering 1892-2019. Astronomy and Astrophysics, vol. 639, pp. A88, 2020. DOI: 10.1051/0004-6361/202037746
2019
• The Characteristic Sizes of the Sunspots and Pores in Solar Cycle 24. Solar Physics, vol. 294, pp. 45, 2019. DOI: 10.1007/s11207-019-1439-1
• Global daily variation of polarized centimeter radio emission of local solar sources and structures of the corresponding groups of spots on the photosphere. Astronomical and Astrophysical Transactions, vol. 31, pp. 243--250, 2019.
• Forecast of solar flares from observations in the microwave range at the Kislovodsk station. Astronomical and Astrophysical Transactions, vol. 31, pp. 103--108, 2019.
• Long-Term Sequences of Solar Observations in the Radio Band at the Mountain Astronomical Station for 60 Years. Geomagnetism and Aeronomy, vol. 59, no. 8, pp. 1139--1145, 2019. DOI: 10.1134/S001679321908019X
• Polar Activity of the Sun and Latitudinal Activity Drifts in Cycles 15–24. Geomagnetism and Aeronomy, vol. 59, no. 8, pp. 1016--1021, 2019. DOI: 10.1134/S0016793219080218
• Refinement of the Gnevyshev-Waldmeier Rule Based on a 140-Year Series of Observations. Astronomy Letters, vol. 45, no. 6, pp. 396--401, 2019. DOI: 10.1134/S1063773719060045
2018
• Stable Sunspot Area Level of Debrecen Photoheliographic Data and Multivariate Correction Factor of SOON Data. Solar Physics, vol. 293, pp. 142, 2018. DOI: 10.1007/s11207-018-1360-z
• The Forecast of Space Weather According to Ground-Based Observatories. vol. 335, pp. 362--364, 2018. DOI: 10.1017/S174392131700881X
• Chromospheric and Coronal Radio Sources from Observations of the Partial Solar Eclipse of March 20, 2015, at the Mountain Astronomical Station of the Central Astronomical Observatory. Geomagnetism and Aeronomy, vol. 58, pp. 464--468, 2018. DOI: 10.1134/S0016793218040163
• Stable sunspot area level of Debrecen Photoheliographic Data and multivariate correction factor of SOON data. pp. 16347, 2018.
• Migration of polar prominences in 13-24 cycles of activity. vol. 340, pp. 189--190, 2018. DOI: 10.1017/S1743921318001102
• Reconstruction of Centennial Series of Solar Activity. Geomagnetism and Aeronomy, vol. 58, no. 8, pp. 1021--1028, 2018. DOI: 10.1134/S0016793218080182
• Reconstruction of solar activity according to the data of centenary observations. Proceedings of the International Astronomical Union, vol. 13, no. S340, pp. 137--140, 2018. DOI: 10.1017/S1743921318001473
• The Gnevyshev-Ohl Rule and Two Sunspot Group Populations. Geomagnetism and Aeronomy, vol. 58, no. 8, pp. 1103--1107, 2018. DOI: 10.1134/S0016793218080121
• Evolution of structures with an open magnetic flux over a hundred years. Proceedings of the International Astronomical Union, vol. 13, no. S340, pp. 141--144, 2018. DOI: 10.1017/S1743921318001862
• Создание атласа солнечной активности. Известия Крымской астрофизической обсерватории, vol. 114, no. 1, pp. 118--122, 2018.
• Sunspot Positions and Areas from Observations by Pierre Gassendi. Solar Physics, vol. 293, no. 11, pp. 150, 2018. DOI: 10.1007/s11207-018-1372-8
• (PDF) A METHOD TO FORECAST SOLAR FLARES USING THE KISLOVODSK’S SOLAR PATROL OPTICAL TELESCOPE (SPOT). ResearchGate, 2018. DOI: 10.31725/0552-5829-2018-303-306
• Some Features of the Two Sunspot Group Populations’ Properties. Geomagnetism and Aeronomy, vol. 58, no. 8, pp. 1170--1174, 2018. DOI: 10.1134/S001679321808025X
• Statistics of “Cold” Early Impulsive Solar Flares in X-Ray and Microwave Domains. The Astrophysical Journal, vol. 856, no. 2, pp. 111, 2018. DOI: 10.3847/1538-4357/aab271
2017
• The Waldmeier Effect for Two Sunspot Populations. Geomagnetism and Aeronomy, vol. 57, pp. 1092--1100, 2017. DOI: 10.1134/S0016793217080199
• Space Weather Parameters: Modeling and Prediction from the Data of Groundbased Observations of Solar Activity. Geomagnetism and Aeronomy, vol. 57, pp. 854--858, 2017. DOI: 10.1134/S0016793217070210
• Prominence Characteristics in 16th Activity Cycle. Geomagnetism and Aeronomy, vol. 57, pp. 829--834, 2017. DOI: 10.1134/S0016793217070234
• Results of Spectral Corona Observations in Solar Activity Cycles 17–24. Geomagnetism and Aeronomy, vol. 57, pp. 798--802, 2017. DOI: 10.1134/S0016793217070039
• Long-term variations in sunspot magnetic field-area relation. Astronomische Nachrichten, vol. 338, pp. 26--34, 2017. DOI: 10.1002/asna.201613035
• Reconstruction of a Hundred Years Series of Solar Filaments from Daily Observational Data. Geomagnetism and Aeronomy, vol. 57, no. 7, pp. 825--828, 2017. DOI: 10.1134/S0016793217070222
• Possibilities and problems of Solar magnetic field observations for space weather forecast. Solar-Terrestrial Physics, vol. 3, pp. 26--39, 2017. DOI: 10.12737/article_58f96ef99d4cd9.20657784
• Reconstruction of the Filament Properties, Based on Centenarian Daily Observations of the Sun in Hα Line. Proceedings of the International Astronomical Union, vol. 13, no. S335, pp. 187--190, 2017. DOI: 10.1017/S1743921317008195
• Coronal Holes as Tracers of the Sun’s Global Magnetic Field in Cycles 21–23 of Solar Activity. Geomagnetism and Aeronomy, vol. 57, no. 7, pp. 803--813, 2017. DOI: 10.1134/S0016793217070040
• Versions of Time Series for Classical Solar Indices and an Adequate Description of Solar Activity. Geomagnetism and Aeronomy, vol. 57, no. 7, pp. 783--787, 2017. DOI: 10.1134/S0016793217070131
• Features of Microwave Radiation and Magnetographic Characteristics of Solar Active Region NOAA 12242 Before the X1.8 Flare on December 20, 2014. Geomagnetism and Aeronomy, vol. 57, no. 8, pp. 978--987, 2017. DOI: 10.1134/S0016793217080023
• Construction of a century solar chromosphere data set for solar activity related research. Solar-Terrestrial Physics, vol. 3, pp. 5--8, 2017. DOI: 10.12737/stp-3220171
2016
• Observations of long-period oscillations of the solar active regions in the visible and UV spectral intervals. Geomagnetism and Aeronomy, vol. 56, pp. 872--879, 2016. DOI: 10.1134/S001679321607015X
• Two populations of sunspots and secular variations of their characteristics. Astronomy Letters, vol. 42, pp. 703--712, 2016. DOI: 10.1134/S1063773716090048
• The area and absolute magnetic flux of sunspots over the past 400 years. Astronomy Reports, vol. 60, pp. 831--838, 2016. DOI: 10.1134/S1063772916090055
• Tilt Angles of Solar Filaments over the Period of 1919 - 2014. Solar Physics, vol. 291, pp. 1115--1127, 2016. DOI: 10.1007/s11207-016-0880-7
• On the origin of 140 GHz emission from the 4 July 2012 solar flare. Advances in Space Research, vol. 57, pp. 1449--1455, 2016. DOI: 10.1016/j.asr.2015.12.037
• Is it Possible to Use the Green Coronal Line Instead of X rays to Cancel an Effect of the Coronal Emissivity Deficit in Estimation of the Prominence Total Mass from Decrease of the EUV-corona Intensities?. vol. 504, pp. 89, 2016.
• Forecast of solar wind parameters according to STOP magnetograph observations. Geomagnetism and Aeronomy, vol. 56, pp. 1095--1103, 2016. DOI: 10.1134/S0016793216080223
• Solar Physics Research in the Russian Subcontinent - Current Status and Future. 2016. DOI: 10.48550/ARXIV.1606.01331
• Construction of the light curves for solar flares in the Hα line. Geomagnetism and Aeronomy, vol. 56, no. 5, pp. 513--523, 2016. DOI: 10.1134/S0016793216050029
• Coronal holes in the long-term modulation of cosmic rays. Geomagnetism and Aeronomy, vol. 56, no. 3, pp. 257--263, 2016. DOI: 10.1134/S0016793216030063
• On-line Tools for Solar Data Compiled at the Debrecen Observatory and Their Extensions with the Greenwich Sunspot Data. Solar Physics, vol. 291, no. 9, pp. 3081--3102, 2016. DOI: 10.1007/s11207-016-0930-1
2015
• Study of some characteristics of large-scale solar magnetic fields during the global field polarity reversal according to observations at the telescope-magnetograph Kislovodsk Observatory. Geomagnetism and Aeronomy, vol. 55, pp. 969--975, 2015. DOI: 10.1134/S0016793215070257
• Synoptic and fast events on the sun according to observations at the center and wings of the Ca II K line at the Kislovodsk Mountain station patrol telescope. Geomagnetism and Aeronomy, vol. 55, pp. 961--968, 2015. DOI: 10.1134/S0016793215070245
• SMALL-SCALE AND GLOBAL DYNAMOS AND THE AREA AND FLUX DISTRIBUTIONS OF ACTIVE REGIONS, SUNSPOT GROUPS, AND SUNSPOTS: A MULTI-DATABASE STUDY. The Astrophysical Journal, vol. 800, no. 1, pp. 48, 2015. DOI: 10.1088/0004-637X/800/1/48
• Orientation of the linear polarization plane of H-alpha emission in prominences. 2015. DOI: 10.48550/arXiv.1502.04637
• THE MINIMUM OF SOLAR CYCLE 23: AS DEEP AS IT COULD BE?. The Astrophysical Journal, vol. 804, no. 1, pp. 68, 2015. DOI: 10.1088/0004-637X/804/1/68
• Solar Cycle Characteristics and Their Relationship with Dynamo Theory. Journal of Physics: Conference Series, vol. 661, no. 1, pp. 012009, 2015. DOI: 10.1088/1742-6596/661/1/012009
• The heliospheric sheet configuration according to the coronal ray synoptic maps in solar activity cycles 23 and 24. Geomagnetism and Aeronomy, vol. 55, no. 3, pp. 287--294, 2015. DOI: 10.1134/S0016793215030081
• Dynamics of Microwave Sources Associated with the Neutral Line and the Magnetic-Field Parameters of Sunspots as a Factor in Predicting Large Flares. Solar Physics, vol. 290, no. 1, pp. 53--77, 2015. DOI: 10.1007/s11207-014-0605-8
2014
• The properties of solar cycle 24 and their connection with common relationships of cycles 19-23. vol. 572, pp. 012004, 2014. DOI: 10.1088/1742-6596/572/1/012004
• Coronal holes, large-scale magnetic field, and activity complexes in solar cycle 23. Geomagnetism and Aeronomy, vol. 54, pp. 953--958, 2014. DOI: 10.1134/S0016793214070135
• Applying an Automatic Image-Processing Method to Synoptic Observations. Solar Physics, vol. 289, pp. 1403--1412, 2014. DOI: 10.1007/s11207-013-0404-7
• Activity indices in solar cycle 24 and their correlation with general regularities of cycles 19–23 according to mountain astronomical station data. Geomagnetism and Aeronomy, vol. 54, no. 8, pp. 1014--1018, 2014. DOI: 10.1134/S0016793214080131
• Coronal Holes in Solar Cycles 21 to 23. Solar Physics, vol. 289, no. 4, pp. 1349--1358, 2014. DOI: 10.1007/s11207-013-0387-4
• Global magnetic field cycle evolution and prominence eruptions. vol. 300, pp. 168--171, 2014. DOI: 10.1017/S1743921313010922
• Solar Cycle Indices from the Photosphere to the Corona: Measurements and Underlying Physics. Space Science Reviews, vol. 186, no. 1, pp. 105--135, 2014. DOI: 10.1007/s11214-014-0089-8
• Peculiarities of the development of active regions on the Sun prior to strong X-class flares: Joint analysis of data from the RATAN-600 radio telescope and SDO space observatory. Cosmic Research, vol. 52, no. 1, pp. 1--14, 2014. DOI: 10.1134/S0010952514010018
2013
• Long-term variations in sunspot characteristics. Geomagnetism and Aeronomy, vol. 53, pp. 953--956, 2013. DOI: 10.1134/S0016793213080264
• Indirect comparison of Debrecen and Greenwich daily sums of sunspot areas. Monthly Notices of the Royal Astronomical Society, vol. 434, pp. 1713--1720, 2013. DOI: 10.1093/mnras/stt1134
• Areas of Sunspot Groups According to Catalogues of Sun Service in 1942-1952. Visnik Kiiv. Univ., Fiz.-Mat. Nauki, Astron, vol. 50, pp. 55--62, 2013.
• The Peculiarities Of The Initial Phase Of The 24-th Solar Activity Cycle. Journal of Physics: Conference Series, vol. 461, no. 1, pp. 012011, 2013. DOI: 10.1088/1742-6596/461/1/012011
• High-latitude coronal holes and polar faculae in the 21st–23rd solar activity cycles. Geomagnetism and Aeronomy, vol. 53, no. 7, pp. 896--900, 2013. DOI: 10.1134/S0016793213070098
• New generation solar telescope of operative predictions. Optoelectronics, Instrumentation and Data Processing, vol. 49, no. 6, pp. 578--584, 2013. DOI: 10.3103/S8756699013060071
2012
• Specific features of radio emissions of coronal holes based on eclipse and noneclipse observations at a solar activity minimum. Geomagnetism and Aeronomy, vol. 52, pp. 142--149, 2012. DOI: 10.1134/S0016793212020132
• On the solar activity cycles 23–24. Bulletin of the Lebedev Physics Institute, vol. 39, no. 4, pp. 95--99, 2012. DOI: 10.3103/S106833561204001X
• ON A POSSIBLE EXPLANATION OF THE LONG-TERM DECREASE IN SUNSPOT FIELD STRENGTH. The Astrophysical Journal Letters, vol. 758, no. 1, pp. L20, 2012. DOI: 10.1088/2041-8205/758/1/L20
• Долговременные вариации атмосферного ореола по данным наблюдений солнечной короны на Горной станции ГАО РАН в период 1957-2010 гг.. Оптика Атмосферы И Океана, vol. 25, no. 5, pp. 434--437, 2012.
• Variations in the large-scale polar solar magnetic flux: The average annual series of the Π index in 1858–2006. Geomagnetism and Aeronomy, vol. 52, no. 4, pp. 431--437, 2012. DOI: 10.1134/S0016793212040056
• Advances in Solar Research at Eclipses from Ground and from Space: Proceedings of the NATO Advanced Study Institute on Advances in Solar Research at Eclipses from Ground and from Space Bucharest, Romania 9–20 August, 1999. 2012.
2011
• Green and Red Coronal Line Data Explored Over the Period of about 6 Last Activity Cycles with Wavelet Methods and Recurrence Plots. pp. 4, 2011.
• Observations of March 29, 2006 solar eclipse in the radio range at wavelengths of 3.2 and 4.9 cm. Cosmic Research, vol. 49, pp. 93--98, 2011. DOI: 10.1134/S0010952511010084
2010
• On the existence of the east-west asymmetry in the optical observations of the solar corona. Geomagnetism and Aeronomy, vol. 50, pp. 848--853, 2010. DOI: 10.1134/S0016793210070030
• Solar Cycle Prediction. Living Reviews in Solar Physics, vol. 7, pp. 6, 2010. DOI: 10.12942/lrsp-2010-6
2009
• Some notes concerning the prediction of the amplitude of the solar activity cycles. Astrophysics and Space Science, vol. 323, pp. 221--224, 2009. DOI: 10.1007/s10509-009-0056-0
• The Minimum Activity Epoch as a Precursor of the Solar Activity. Solar Physics, vol. 260, no. 2, pp. 465--477, 2009. DOI: 10.1007/s11207-009-9451-5
• A Century of Solar Ca ii Measurements and Their Implication for Solar UV Driving of Climate. Solar Physics, vol. 255, no. 2, pp. 229--238, 2009. DOI: 10.1007/s11207-009-9330-0
• A homogeneous database of sunspot areas covering more than 130 years. Journal of Geophysical Research (Space Physics), vol. 114, pp. A07104, 2009. DOI: 10.1029/2009JA014299
2008
• Global solar activity on long time scales. Astrophysical Bulletin, vol. 63, pp. 43--55, 2008. DOI: 10.1007/s11755-008-1005-7
• Reconstruction of space weather physical parameters on 400-year scale. Cosmic Research, vol. 46, no. 4, pp. 283--293, 2008. DOI: 10.1134/S0010952508040011
2007
• Some notes concerning the prediction of the amplitude of the two solar activity cycles. 2007. DOI: 10.48550/arXiv.0706.1624
• Series of classical solar activity indices: Kislovodsk data. Solar System Research, vol. 41, pp. 81--86, 2007. DOI: 10.1134/S0038094607010091
2006
• Temperature of Polar Corona of the Sun According to Kislovodsk Observations During 1957 2002. Solar Physics, vol. 237, pp. 201--210, 2006. DOI: 10.1007/s11207-006-1680-2
• A Wavelet Approach to the long-term Data of the green coronal Brightness. vol. 36, pp. 3525, 2006.
• Decrease of hot regions in the polar corona of the Sun during 1957 2002. vol. 233, pp. 247--250, 2006. DOI: 10.1017/S1743921306001943
• Long-term variations in the rotation of the solar corona. Astronomy Reports, vol. 50, no. 4, pp. 325--332, 2006. DOI: 10.1134/S1063772906040068
2005
• The proportion of hot and cold regions in the polar solar corona during 1957 2002. Astronomy Reports, vol. 49, pp. 932--938, 2005. DOI: 10.1134/1.2127996
• Reexamination of the coronal index of solar activity. Journal of Geophysical Research (Space Physics), vol. 110, pp. A08106, 2005. DOI: 10.1029/2005JA011146
• On the long-term variability of the green corona accordingly to four existing databases. Kinematika i Fizika Nebesnykh Tel Supplement, vol. 5, pp. 129--133, 2005.
2004
• On the green corona variability as reported by four groups of observers - an attempt of comparison. vol. 35, pp. 2633, 2004.
• Debrecen Photoheliographic Data for the Years 1993-1995. Publications of Debrecen Heliophysical Observatory, vol. 17-19, pp. 1, 2004.
• Cyclical evolution of solar corona by observation in line FeXIV 5303Å. vol. 223, pp. 255--256, 2004. DOI: 10.1017/S1743921304005800
2003
• Temperature of polar corona of the Sun during the last 50 years (1952-2001). vol. 535, pp. 217--228, 2003.
2002
• On a decrease of high-latitude corona temperature of the Sun in the last 50 years. vol. 477, pp. 241--244, 2002.
• A study of the development of global solar activity in the 23rd solar cycle based on radio observations with the Nobeyama radio heliograph - I. Latitude distribution of the active and dark regions. Astronomy Astrophysics, vol. 389, no. 2, pp. 618--623, 2002. DOI: 10.1051/0004-6361:20020666
• Increase of the Magnetic Flux From Polar Zones of the sun in the Last 120 Years. Solar Physics, vol. 206, no. 2, pp. 383--399, 2002. DOI: 10.1023/A:1015062615953
2001
• Debrecen Photoheliographic Data for the year 1988. Publications of Debrecen Heliophysical Observatory, vol. 12, 2001.
• Millimeter-radio, SOHO/EIT 171 Å features and the polar faculae in the polar zones of the Sun. Astronomy Astrophysics, vol. 366, no. 2, pp. 676--685, 2001. DOI: 10.1051/0004-6361:20000265
• The increase in the magnetic flux from the polar regions of the Sun over the last 120 years. Astronomy Reports, vol. 45, no. 9, pp. 746--750, 2001. DOI: 10.1134/1.1398924
• On the Sudden Depression of Radio Emission From Plasma Above a Fast-Moving Sunspot. Solar Physics, vol. 201, no. 1, pp. 137--152, 2001. DOI: 10.1023/A:1010320428861
• Comparison of sunspot area data bases. Monthly Notices of the Royal Astronomical Society, vol. 323, pp. 223--230, 2001. DOI: 10.1046/j.1365-8711.2001.04195.x
2000
• Longitude and Latitude Structure of the Polar Activity of the Sun in the 21st Cycle. Astronomy Reports, vol. 44, pp. 487--493, 2000. DOI: 10.1134/1.163873
1999
• Observations of Peculiarities of Sunspot Fragment Patterns. Solar Physics, vol. 186, no. 1, pp. 193--205, 1999. DOI: 10.1023/A:1005153931561
1998
• Coronal observations, January - December 1995.. Quarterly Bulletin on Solar Activity, vol. 37, pp. 1--22, 1998.
• Coronal observations, January - December 1994.. Quarterly Bulletin on Solar Activity, vol. 36, pp. 1--25, 1998.
• Coronal observations (maps), July - December 1993.. Quarterly Bulletin on Solar Activity, vol. 35, pp. 18--24, 1998.
• Coronal observations (maps), July - December 1992.. Quarterly Bulletin on Solar Activity, vol. 34, pp. 25--28, 1998.
• Debrecen Photoheliographic Data for the year 1987 on the basis of photographic observations taken at the observatories of Debrecen and Gyula (Hungary), as well as Abastumani (Georgia), Ebro (Spain), Kiev (Ukraine), Kislovodsk (Russia), Kodaikanal (India) and Tashkent (Uzbekistan).. Publications of Debrecen Heliophysical Observatory, vol. 11, 1998.
• The Role of Chromospheric Cavities in the Structure of Background Solar Magnetic Fields. Geomagnetism and Aeronomy, vol. 38, pp. 89, 1998.
• A new database of the green-line corona brightness as compiled for the last five solar cycles and its possible utilization in the ISCS project. Astronomical Astrophysical Transactions, vol. 16, no. 1, pp. 75--80, 1998. DOI: 10.1080/10556799808208146
• Torsional Oscillation Pattern in the Large - Scale Magnetic Field (1910 - 1993) and in the Solar Corona (1940 - 1993). Synoptic Solar Physics, vol. 140, pp. 65, 1998.
1997
• Possible east side predominance of the optical emissions of the solar corona. New Astronomy, vol. 2, pp. 437--447, 1997. DOI: 10.1016/S1384-1076(97)00027-4
• Differential rotation of the red solar corona (FeX 6374 A) in 1957-1994. Astronomicheskii Zhurnal, vol. 74, pp. 621, 1997.
• The differential rotation of the Red Solar Corona (Fe X 6374 Å) from 1957-1994. Astronomy Reports, vol. 41, pp. 548--551, 1997.
1996
• Implications for preferred longitudes in the coronal optical intensities. Advances in Space Research, vol. 17, pp. 277--280, 1996. DOI: 10.1016/0273-1177(95)00584-2
• Unequal optical emissions between the east and the west part of the solar corona. Advances in Space Research, vol. 17, pp. 273--276, 1996. DOI: 10.1016/0273-1177(95)00583-Z
• Polar Faculae and Sunspot Cycles. Solar Physics, vol. 163, pp. 267--289, 1996. DOI: 10.1007/BF00148001
• Debrecen Photoheliographic Data for the year 1986 on the basis of photographic observations taken at the observatories of Debrecen and Gyula (Hungary), as well as Kislovodsk (Russia).. Publications of Debrecen Heliophysical Observatory, vol. 10, 1996.
1995
• Torsional mode in the solar-corona intensity variations in the Fe XIV 5303 A line between 1957 and 1991. Astronomicheskii Zhurnal, vol. 72, pp. 749, 1995.
• Noise Storms and the Structure of Microwave Emission of Solar Active Regions. Solar Physics, vol. 160, pp. 133--149, 1995. DOI: 10.1007/BF00679101
• Aspects of the long-term cosmic-ray modulation. Solar Physics, vol. 157, no. 1, pp. 375--387, 1995. DOI: 10.1007/BF00680628
1994
• Coronal loops and prominences as observed with RATAN-600. Space Science Reviews, vol. 70, no. 1, pp. 193--198, 1994. DOI: 10.1007/BF00777867
1993
• Intensities of the solar corona in monochromatic emission at position angles every 5 degrees.. Quarterly Bulletin on Solar Activity, vol. 35, pp. 1--17, 1993.
1992
• The Peculiarities of Rotation of the Solar Polar Regions. Solar Physics, vol. 139, pp. 233--245, 1992. DOI: 10.1007/BF00159150
• Global solar cycle in the distribution of the green coronal emission period: 1940 1989. Solar Physics, vol. 137, pp. 395--400, 1992. DOI: 10.1007/BF00161858
• Intensité de la couronne solaire en lumière monochromatique, selon des angles de position variant de 5° en 5°. Jan - Dec 1992.. Quarterly Bulletin on Solar Activity, vol. 34, pp. 1--24, 1992.
• Rapid motion of filaments - Eruptive prominences. Astronomicheskii Zhurnal, vol. 69, pp. 181--191, 1992.
• Very Large Array-RATAN 600 observations of a solar active region. Solar Physics, vol. 141, no. 2, pp. 303--323, 1992. DOI: 10.1007/BF00155182
1991
• Intensité de la couronne solaire en lumière monochromatique, selon des angles de position variant de 5° en 5°. Jan - Dec 1991.. Quarterly Bulletin on Solar Activity, vol. 33, pp. 1--30, 1991.
1990
• Structure elements of the photosphere and their variations with the solar activity cycle.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 10, pp. 85--90, 1990.
• Peculiarities of oscillatory processes in sunspot groups SD 135/1984 and SD 136/1984.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 9, pp. 91--96, 1990.
• On the contrast dependence of polar faculae.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 3, pp. 81--84, 1990.
• Intensité de la couronne solaire en lumière monochromatique, selon des angles de position variant de 5° en 5°. Jan - Dec 1990.. Quarterly Bulletin on Solar Activity, vol. 32, pp. 1--31, 1990.
1989
• Investigation of the rotation of solar atmosphere polar regions.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 8, pp. 111--118, 1989.
• Do polar faculae on the sun predict a sunspot cycle?. Solar Physics, vol. 119, pp. 45--54, 1989. DOI: 10.1007/BF00146211
• Intensité de la couronne solaire en lumière monochromatique, selon des angles de position variant de 5° en 5°. Jan - Dec 1989.. Quarterly Bulletin on Solar Activity, vol. 31, pp. 1--31, 1989.
1988
• Intensité de la couronne solaire en lumière monochromatique, selon des angles de position variant de 5° en 5°. Jan - Dec 1988.. Quarterly Bulletin on Solar Activity, vol. 30, pp. 1--32, 1988.
• Peculiarities of the chromospheric structure of polar regions on the Sun.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1988, pp. 80--84, 1988.
1987
• On the relationship between polar faculae, X-ray bright points and ephemeral active regions on the sun.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1987, pp. 62--70, 1987.
• Note on the forecast of strong fluctuations of solar activity in solar cycle 22.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1987, pp. 73--80, 1987.
1986
• On the latitude migration of polar faculae in the solar activity cycle period: 1970–1978. Journal of Astrophysics and Astronomy, vol. 7, pp. 113--118, 1986. DOI: 10.1007/BF02715034
• Wolf numbers in solar cycle No. 21.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1986, pp. 57--62, 1986.
1985
• Comparison of Coronal Station Scales Emission Line 530.3-NM 1977-1983. Contributions of the Astronomical Observatory Skalnate Pleso, vol. 13, pp. 127, 1985.
• Latitudinal migration of polar faculae during their activity cycle. Period 1970 - 1978.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1985, pp. 71--77, 1985.
• Some results of a study of a solar flare in a sunspot umbra.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1985, pp. 60--64, 1985.
• Doppler velocity measurements in prominences using a Fabry-Perot interferometer.. Abastumanskaia Astrofizicheskaia Observatoriia Byulleten, vol. 60, pp. 183--186, 1985.
1984
• Comparative magnetographic observations in different prominence lines. Astronomy and Astrophysics, vol. 140, pp. 112--118, 1984.
• Stability of the Photometric Observations of the Solar Corona and Variations of its Intensity in the Solar CYCLE-21. Solar Physics, vol. 90, pp. 177--184, 1984. DOI: 10.1007/BF00153793
• Spectrum-time analysis of the radio emission of the sun at λ = 3 cm wavelength.. Akademiia Nauk Azerbaidzhanskoi SSR Doklady, vol. 40, pp. 35--39, 1984.
• On the method of the Mountain Kislovodsk Station of the Pulkovo Observatory for the construction of "Synoptic Charts of Active Solar Features".. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1984, pp. 59--61, 1984.
• On the problem of a relationship between a loop prominence and a surge.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1983, pp. 91--94, 1984.
• Spectrum-time analysis of the radio emission of the sun at λ = 3 cm wavelength.. Akademiia Nauk Azerbaidzhanskoi SSR Doklady, vol. 40, pp. 35--39, 1984.
1983
• Stability of the photometric out-of-eclipse observations of the solarcorona and variations of its intensity in the 21st solar cycle.. Publications of Debrecen Heliophysical Observatory, vol. 5, pp. 503--510, 1983.
• On a connection between polar faculae and sunspot activity. II.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1983, pp. 97--101, 1983.
• A comparison of the distribution of background field polarity on Hα-synoptic charts with magnetographic observations of magnetic fields.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1982, pp. 94--97, 1983.
1982
• Magnetic field in solar prominences measured with a new spectrally scanning magnetograph. Astronomy and Astrophysics, vol. 114, pp. 347--350, 1982.
• Comparison of the 530.3 NM - Coronal Brightness Estimates of the Wendelstein Solar Observatory and of the 530.3 NM - Coronal Measurements of Alma-Ata, Kislovodsk, Lomnický Štít, Norikura, with the Wendelstein 530.3 NM -Coronal Photometer. Bulletin of the Astronomical Institutes of Czechoslovakia, vol. 33, pp. 60, 1982.
• Morphology of H-alpha filaments and filament channel systems. Journal of Astrophysics and Astronomy, vol. 3, no. 4, pp. 379--382, 1982. DOI: 10.1007/BF02714879
1981
1980
• On the Large Scale Brightness Fluctuations in the Solar Atmosphere. Solar Physics, vol. 68, pp. 237--242, 1980. DOI: 10.1007/BF00156862
• Methods of observation and prediction of solar radio bursts at 5.0 cm at the Kislovodsk Station of the Pulkovo Observatory.. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1979, pp. 99--107, 1980.
• Methods of Observation and Prediction of Solar Radio Bursts at 5.0-CM in the Kislovodsk Station of the Pulkovo Observatory. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 10, pp. 99, 1980.
1978
• Long-term correlation between latitude-dependent solar activity and solar wind streams.. The Astrophysical Journal, vol. 223, pp. 601--604, 1978. DOI: 10.1086/156295
1975
• On the Correlation of Coronal Green-Line Intensity and Solar Wind Velocity. Solar Physics, vol. 41, pp. 349--366, 1975. DOI: 10.1007/BF00154071
1973
• Filter observations of prominences in the D3 and Hα lines. Solar Physics, vol. 28, no. 2, pp. 377--388, 1973. DOI: 10.1007/BF00152308
1972
• On photographing the form of the solar corona taken in the 5302 Å line at the High-Altitude Station (near Kislovodsk).. Byulletin Solnechnye Dannye Akademie Nauk SSSR, vol. 1972, pp. 105, 1972.
1971
• The longitudinal distribution of the green corona activity. Solar Physics, vol. 18, no. 1, pp. 72--83, 1971. DOI: 10.1007/BF00146034
1970
• The observation of the chromospheric fine structure by the 53-cm lyot coronagraph. Solar Physics, vol. 12, no. 3, pp. 379--390, 1970. DOI: 10.1007/BF00148021
1967
• The Lyot-Coronagraph with 53 cm Objective. Solar Physics, vol. 2, pp. 223--226, 1967. DOI: 10.1007/BF00155923
• On the photometry of coronal emission line 5303 Å on MT Lomnický Štít. Bulletin of the Astronomical Institute of Czechoslovakia, vol. 18, pp. 51, 1967.
1966
• The Relation between Proton Flares and the Corona over the 11-Year Cycle. Soviet Astronomy, vol. 10, pp. 304, 1966.
• Coronal Emission Line Intensity as an Index of Solar Corpuscular Radiation. Soviet Astronomy, vol. 9, pp. 765, 1966.
1965
• Solar constant and sunspots. Pure and Applied Geophysics PAGEOPH, vol. 62, no. 1, pp. 207--214, 1965. DOI: 10.1007/BF00875302