11 citations as recorded by crossref.

1. Evidence for subauroral proton flashes on the dayside as the result of the ion cyclotron interaction T. Yahnina et al. 10.1029/2008JA013099
2. Proton precipitation to the equator of the isotropic boundary during the geomagnetic storm on November 20–29, 2003 T. Yahnina & A. Yahnin 10.1134/S0010952514010092
3. Energetic proton precipitation related to ion–cyclotron waves A. Yahnin & T. Yahnina 10.1016/j.jastp.2007.02.010
4. Generation of a burst of geomagnetic pulsations in the 1–3 Hz frequency range in the daytime sector as a result of dramatic increases in the solar wind dynamic pressure B. Tsegmed 10.1134/S0016793211080305
5. Position of the Source of Dayside High-Latitude Magnetic Impulses in the Magnetosphere from DMSP Satellite Data V. Safargaleev 10.1134/S001679322460022X
6. 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 V. Safargaleev 10.1134/S0016793222060123
7. Hertz Range Pulsations during Recovery Phase of the Magnetic Storm on September 7–8, 2017, and Relation between their Dynamics and Changes in the Parameters of the Interplanetary Medium V. Safargaleev & P. Tereshchenko 10.1134/S0016793219030125
8. Bursts of geomagnetic pulsations in the frequency range 0.2-5 Hz excited by large changes of the solar wind pressure V. Parkhomov et al. 10.1134/S0010952510010077
9. Sporadic Geomagnetic Pulsations at Frequencies of up to 15 HZ in the Magnetic Storm of November 7–14, 2004: Features of the Amplitude and Polarization Spectra and their Connection with Ion–Cyclotron Waves in the Magnetosphere E. Ermakova et al. 10.1007/s11141-016-9628-3
10. Relation between sudden increases in the solar wind dynamic pressure, auroral proton flashes, and geomagnetic pulsations in the Pc1 range T. Popova et al. 10.1134/S0016793210050038
11. Proton Auroras Equatorward of the Oval as a Manifestation of the Ion-Cyclotron Instability in the Earth’s Magnetosphere (Brief Review) A. Yahnin et al. 10.1134/S001679321805016X