Works matching IS 00167932 AND DT 2020 AND VI 60 AND IP 7
Results: 31
Features of the Earth's Solar Climate Changes in the Present Epoch.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 993, doi. 10.1134/S0016793220070117
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Path Integral Method in the Mean-field Model for the Magnetic Vector Potential.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 989, doi. 10.1134/S0016793220070300
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Properties of the Variability of the Solar Constant as an Index of Solar Activity.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 982, doi. 10.1134/S0016793220070208
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Influence of Solar-Geophysical Factors on the State of the Stratospheric Polar Vortex.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 974, doi. 10.1134/S0016793220070282
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Solar-Flux Variation in Helium Lines According to SDO/EVE Data in the 24th Cycle and the Forecast for Different Levels of Solar Activity. Lyman Decrements of Hydrogen and Helium Lines.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 966, doi. 10.1134/S0016793220070099
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Gamma Rays Generated in Nuclear Interactions of Protons Accelerated during Solar Flares.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 958, doi. 10.1134/S0016793220070270
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Influence of Cycle Variations in the Global Solar Magnetic Field on Characteristics of the Interplanetary Plasma.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 948, doi. 10.1134/S0016793220070063
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Long-term Activity in Photospheres of Low-mass Stars with Strong Magnetic Fields.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 942, doi. 10.1134/S0016793220070075
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Characteristics of Soft X-Ray Radiation of the Solar Active Region NOAA 1024 Registered by the PINGVIN-M Device in July 2009.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 936, doi. 10.1134/S001679322007021X
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Energetics of X-Class Flares at the Minima of 22, 23, and 24 Solar Cycles.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 929, doi. 10.1134/S001679322007018X
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Study of Long-Duration Flares and Associated Chromospheric and Coronal Ejections in Solar Cycles 23 and 24.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 921, doi. 10.1134/S0016793220070221
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Evolution of Electric Current and Resistance in the Flare Loop in the Course of Loop Shrinkage.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 915, doi. 10.1134/S0016793220070312
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The Color of Solar Corona Structures.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 909, doi. 10.1134/S0016793220070142
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Modified 3D Model of a Facular KNOT.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 904, doi. 10.1134/S0016793220070233
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Source of Electromagnetic Radiation in Corona and Impedance of the Stationary Magnetic Reconnection Area.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 896, doi. 10.1134/S0016793220070129
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Electron Energy Spectra and e–e Bremsstrahlung from Anisotropic Electron Distributions in Extreme Solar Flares.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 889, doi. 10.1134/S0016793220070191
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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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24th Cycle of Solar Activity: Geoefficiency of Flares.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 876, doi. 10.1134/S0016793220070087
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Comparative Analysis of Terrestrial and Satellite Observations of Photospheric Magnetic Field in an Appendix to Simulation of Parameters of Coronal Holes and Solar Wind.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 872, doi. 10.1134/S0016793220070051
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Relationship of the Magnetic-Field Strength and the Brightness of the Sunspot Umbra and the Center of a Facular Knot.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 865, doi. 10.1134/S0016793220070324
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Anomalies of Shape of 11-year Solar Cycle in Sunspot Number Series.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 860, doi. 10.1134/S0016793220070130
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Signs of Preflare Situation in Solar Ultraviolet and Microwave Emission.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 853, doi. 10.1134/S001679322007004X
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Solar-Flare Precursors in the Microwave Range.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 846, doi. 10.1134/S0016793220070038
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Radiocarbon Data from the Late 18th Century as a Reflection of Solar Activity Variation, Natural Climate Change, and Anthropogenic Activity.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 840, doi. 10.1134/S0016793220070166
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Periods of Extremely High Rates of the Production of Cosmogenic 14C and Temperature Variation According to Data on the 40Ar Content in the Ice Layers for the Last 4000 Years.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 835, doi. 10.1134/S0016793220070105
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Manifestations in the Solar Corona of the Process of Magnetic-Field Generation.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 831, doi. 10.1134/S0016793220070178
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Polar and Low-Latitude Faculae in Activity Cycles 23–24.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 825, doi. 10.1134/S0016793220070245
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Asymmetry of Sunspot Distribution in Solar Cycles 12–24 and the Gnevyshev–Ohl Rule.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 816, doi. 10.1134/S0016793220070294
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Calculation of the Main Parameters of a Magnetic Flux Tube within the Model of Cylindrically Symmetric Equilibria of Two-Component Plasma.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 811, doi. 10.1134/S0016793220070269
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Heat Fluxes in Collisionless Magnetohydrodynamic Shock Waves.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 804, doi. 10.1134/S0016793220070154
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Self-Organized Criticality of Solar Magnetism.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 801, doi. 10.1134/S0016793220070026
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