UDC 539.12

PROBLEMS OF PHYSICS OF PC1 GEOMAGNETIC PULSATIONS: ON THE 90TH ANNIVERSARY OF DISCOVERY OF PEARLS Problems of physics of Pc1 geomagnetic pulsations: On the 90th anniversary of discovery of pearls

Published in Solar-Terrestrial Physics · Volume 12, Issue 3, 2026 · Pages 30–36 · Rubric: Results of current research
DOI: https://doi.org/10.12737/stp-123202603 · EDN: VLHJGB
Received: 11.12.2025 Accepted: 16.02.2026 Published: 19.09.2026 Language of publication: ENG
“Pearl necklaces”, or simply “pearls”, are undoubtedly the true adomment of the rich diversity of ultra-low-frequency electromagnetic waves in Earth’s magnetosphere. They are noted for outstanding beauty of their form and the mystery of their origin. Pearls were first observed by E. Sucksdorff and L. Harang in 1936. This article celebrates the anniversary of their discovery. It briefly outlines the so-called standard model of pearl excitation and propagation. The key importance of the standard model’s fundamental principles in planning research and interpreting the results obtained is emphasized. We point out difficulties with the standard model, particularly the deviation from antisymmetry in the appearance of pearls at conjugate points. An alternative model is proposed which is based on the concept of an ion-cyclotron resonator located in the equatorial zone of the outer radiation belt. It is hypothesized that the excitation of a discrete sequence of pearls is caused by ponderomotive self-Q-modulation of the ion-cyclotron resonator.
magnetosphere, radiation belt, ion-cyclotron wave, Alfvén wave, ion-cyclotron resonator, ponderomotive force
Funding
The study was carried out under the Government assignment of the Ministry of Science and Higher Education of Schmidt Institute of Physics of the Earth RAS and under the Government assignment of the Ministry of Science and Higher Education of the Institute of Solar-Terrestrial Physics SB RAS (Subsidy No. 075-GZ/Ts3569/278)
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