Vol. 62, No. 6, 2022
Spatial Evolution and Structure of High-Speed Flows of Solar Wind from Coronal Holes
p. 675 abstract
Correlation of Time Series of Wolf Numbers and their Derivatives
p. 685 abstract
Estimation of the Propagation Time of the Solar Wind Pressure Pulse between a Shock Wave and the Magnetopause Based on Simultaneous Satellite and Ground-Based Observations
p. 694 abstract
The Influence of Extreme Levels of the Solar Wind Dynamic Pressure on the Structure of Nightside Auroral Precipitation
p. 704 abstract
Observations of Geomagnetic Induced Currents in Northwestern Russia: Case Studies
p. 711 abstract
A Short-Term Forecast for Parameters of the F2 Layer
p. 724 abstract
A Method for Correcting Neutron Monitor Data for the Snow Effect
p. 737 abstract
Observation of an Excess of Positive Air Ions in Underground Cavities
p. 743 abstract
Determining the Position of the South Magnetic Pole from the Data of the Russian Round-the-World Expeditions of 1820 (Bellingshausen) and 2020 (Admiral Vladimirskii). I. The Bellingshausen Expedition
p. 756 abstract
The Depths to the Lithospheric Magnetic Sources Along the Kovdor–GSZ-76 Profile (Baltic Shield–Barents Sea)
p. 767 abstract
Turbulent Origin in the Influence of Seismic Activity on Irregularities of the Es Sporadic Layer
p. 779 abstract
Interpretation of Ionospheric Disturbances During the Largest Earthquake by the Using the Differentiated Approach for the Special Methods to Processing Satellite Radio Signals
p. 783 abstract
Analyzing the Effects of Geomagnetic Storms on the F2-region Ionosphere in South Pacific Region
p. 802 abstract
Erratum to: Geomagnetic Storm Prediction Based on the Neural Network Digital Processing of Joint Observations of the URAGAN Muon Hodoscope and Neutron Monitor Stations
p. 815 abstract
Erratum to: The Superposition of Auroral Currents in the Region of the Harang Discontinuity
p. 816 abstract