Yazev S.А., Isaeva E.S., Khos-Erdene B. Solar activity cycle 25: the first three years
| 3–9
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Eselevich V.G., Parkhomov V.A. Role of alpha particles in penetration of solar wind diamagnetic structures into the magnetosphere
| 10-20
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Kovalev I.I., Olemskoy S.V., Sdobnov V.E. Monitoring of magnetospheric parameters based on cosmic ray effects in August 2018
| 21-24
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Guglielmi A.V., Feygin F.Z. Partial ponderomotive forces of Alfvén waves in near-Earth plasma
| 25-29
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Akhmetov O.I., Mingalev I.V., Mingalev O.V., Belakhovsky V.B., Maurchev E.A., Larchenko A.V., Suvorova Z.V., Balabin Yu.V. Influence of strong solar proton events on propagation of radio signals in the VLF range in a high-latitude region
| 30-42
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Potapov A.S., Polyushkina T.N., Guglielmi A.V., Ratovsky K.G., Moskalev I.S. Spectral analysis of IAR oscillations to determine the value and variability of the peak electron density NmF2
| 43-53
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Belakhovsky V.B., Budnikov P.A., Kalishin A.S., Pilgaev S.V., Roldugin A.V. Influence of geomagnetic disturbances on scintillations of GLONASS and GPS signals as observed on the Kola peninsula
| 54-67
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Kurazhkovskaya N.A., Kurazhkovskii A.Yu. Hysteresis effect between geomagnetic activity indices (Ap, Dst) and interplanetary medium parameter in solar activity cycles
| 68-76
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Khabituev D.S., Chernigovskaya M.A. Retrospective analysis of long-term regional features of the dynamic regime of the ionosphere over the south of Eastern Siberia
| 77-85
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Gavrilov N.M., Kshevetskii S.P. Identification of spectrum of secondary acoustic-gravity waves in the middle and upper atmosphere in a high-resolution numerical model
| 86-92
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Selivanov V.N., Aksenovich T.V., Bilin V.A., Kolobov V.V., Sakharov Ya.A. Database of geomagnetically induced currents in the main transmission line "Northern Transit"
| 93-101
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18th Annual Conference “Plasma Physics in the Solar System”. February 6–10, 2023, Space Research Institute RAS, Moscow, Russia
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Zhdanov D.A., Altyntsev A.T., Meshalkina N.S., Anfinogentov S.A. Statistical analysis of microflares as observed by the 4–8 Ghz spectropolarimeter
| 102-111
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Borisenko A.V., Bogachev S.A. Relation between the area of polar coronal holes and the solar wind speed at a minimum between solar cycles 22 and 23
| 112-117
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Yagova N.V., Fedorov E.N., Pilipenko V.A., Mazur N.G. Natural electromagnetic oscillations in 4–12 Hz frequency range as measured by swarm satellites and carisma magnetometer network
| 118-126
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Editer's note
To the 85th anniversary of Geliy A. Zherebtsov
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