Vol. 62, No. 1-2, 2022
The Simplest Solar Dynamo and a New Stabilization Mechanism
p. 1 abstract
Statistical and Probabilistic Characteristics of Wolf Numbers and Their Time Derivatives
p. 6 abstract
Features of the Behavior of Time Parameters of Forbush Decreases Associated with Different Types of Solar and Interplanetary Sources
p. 17 abstract
Relationship of the SAR Arc Dynamics to Substorm Injection Based on the Aurorae Observation. Magnetospheric Phenomena in the Plasmapause Vicinity
p. 32 abstract
Features of the Generation of Ultralow-Frequency Electromagnetic Waves in the Earth’s Magnetosphere with Consideration of the Final Plasma Pressure of Hot Particles
p. 50 abstract
Simulation of Medium Wave Propagation in the Magnetosphere
p. 58 abstract
Solar-Activity Index for the E-Layer Critical Frequency at Middle Latitudes
p. 66 abstract
Relationship between the Drift of Medium-Scale Irregularities and the Orientation of Transverse Anisotropy of Small-Scale Irregularities in the F Region of the Midlatitude Ionosphere
p. 71 abstract
Model of the Equatorial Anomaly in foF2 Based on Interkosmos-19 Data for High Solar Activity
p. 86 abstract
Dependence of D-Region Perturbations of the Midlatitude Ionosphere on the Spectral Composition of the X-Ray Radiation of Solar Flares According to Experimental Data
p. 98 abstract
Effect of Weak Magnetic Storms on the Propagation of HF Radio Waves
p. 104 abstract
Characteristics of Low-Frequency Radiation Excited by the Impact of an Oscillating, High-Frequency Beam on the Ionosphere According to In Situ Measurements
p. 116 abstract
Analysis of Y-component of Geomagnetic Field and SYM-H Index Using Wavelet Multiresolution Analysis
p. 125 abstract
Tracking IMF Fluctuations Nearby Sun Using Wavelet Analysis: Parker Solar Probe First Encounter Data
p. 138 abstract