Vol. 64, No. 6, 2024
Mechanisms of Zebra Pattern Generation in Solar Radio Emission on the Background of Complex Dynamic Spectra
p. 793 abstract
Influence of Processes on the Sun and in the Interplanetary Medium on the Solar Proton Event on March 30, 2022
p. 802 abstract
Role of Middle-Scale Solar Wind Structures in the Turbulence Development Behind the Bow Shock
p. 814 abstract
Induced Proton Precipitations from the Inner Radiation Belt Registered in Oceania
p. 824 abstract
Statistical Studies of the Relationship between the Amplitude of Positive Magnetic Bays at Mid-Latitudes, Geomagnetic Activity, and Solar Wind Parameters
p. 833 abstract
Long-Term Trends in Ionospheric Solar Activity Indices
p. 845 abstract
Dynamics of the Weddel Sea Anomaly and Main Ionospheric Trough in the Southern Summer Hemisphere
p. 851 abstract
Geomagnetic Control of Equatorial Plasma Bubble Development
p. 860 abstract
Specific Features of Ionospheric Disturbances Accompanying the Magnetic Storm of January 14–20, 2022
p. 869 abstract
Intensive Substorms during the Main Phase of the Magnetic Storm on March 23–24, 2023
p. 881 abstract
Simple Model of the Evolution of Magnetic and Kinetic Energy of the Geodynamo
p. 890 abstract
Position of the Source of Dayside High-Latitude Magnetic Impulses in the Magnetosphere from DMSP Satellite Data
p. 897 abstract
Application of Artificial Neural Networks for Reconstruction of Vector Magnetic Field from Single-Component Data
p. 912 abstract
Fluxgate Magnetometers for Geophysical and Special Studies Based on a Universal Measuring Module (Review of Developments)
p. 920 abstract
Prediction of Range Error in GPS Signals during X-Class Solar Flares Occurred between January–April 2023 Using OKSM and RNN
p. 932 abstract
Forecast of Ionospheric TEC during Solar Storms in Low and Mid-Latitudes Using Kriging and Recurrent Neural Network
p. 952 abstract
Terdiurnal Signature of the Critical Frequency of the Sporadic E Layer in Mid-Latitude Regions Based on Ionosonde Observations
p. 971 abstract
Detection of Effects of Shallow Major Earthquakes (M ≥ 5.0, depth ≤ 30 km) Occurred in India, Nepal, and China on Ionosphere Using Statistical Approaches
p. 981 abstract