68 citations as recorded by crossref.

1. Study of the geoeffectiveness of coronal mass ejections, corotating interaction regions and their associated structures observed during Solar Cycle 23 A. Badruddin & Z. Falak 10.1007/s10509-016-2839-4
2. PC index as a proxy of the solar wind energy that entered into the magnetosphere: 3. Development of magnetic storms O. Troshichev & D. Sormakov 10.1016/j.jastp.2017.10.012
3. Dynamics of Large-Scale Solar-Wind Streams Obtained by the Double Superposed Epoch Analysis: 5. Influence of the Solar Activity Decrease Y. Yermolaev et al. 10.3390/universe8090472
4. Does the duration of the magnetic storm recovery phase depend on the development rate in its main phase? 2. A new method Y. Yermolaev et al. 10.1134/S001679321603004X
5. Analysis of Quasistationary Solar Wind Stream Forecasts for 2010–2019 Y. Shugai 10.3103/S1068373921030055
6. The effect of solar activity on the evolution of solar wind parameters during the rise of the 24th cycle D. Rod’kin et al. 10.1134/S0038094616010032
7. Influence of coronal mass ejections on parameters of high-speed solar wind: a case study Y. Shugay et al. 10.1051/swsc/2018015
8. Properties of the Geomagnetic Storm Main Phase and the Corresponding Solar Wind Parameters on 21–22 October 1999 Q. Li et al. 10.3390/universe8070346
9. Predicted dependence of the cross polar cap potential saturation on the type of solar wind stream N. Nikolaeva et al. 10.1016/j.asr.2015.06.029
10. Dependence of radiation belt flux depletions at geostationary orbit on different solar drivers during intense geomagnetic storms S. Gokani et al. 10.3389/fspas.2022.952486
11. Modeling the time behavior of the D st index during the main phase of magnetic storms generated by various types of solar wind N. Nikolaeva et al. 10.1134/S0010952513060038
12. The Magnetic Storm of August 25–26, 2018: Dayside High Latitude Geomagnetic Variations and Pulsations N. Kleimenova et al. 10.1134/S0016793219060070
13. Effects of Geometries and Substructures of ICMEs on Geomagnetic Storms J. Lee et al. 10.1007/s11207-018-1344-z
14. Understanding the variability of magnetic storms caused by ICMEs R. Benacquista et al. 10.5194/angeo-35-147-2017
15. Relationship between substorm activity and the interplanetary medium parameters during the main phase of strong magnetic storms R. Boroyev 10.1016/j.asr.2018.09.001
16. RELATIONSHIP OF THE ASY-H INDEX WITH INTERPLANETARY MEDIUM PARAMETERS AND AURORAL ACTIVITY IN MAGNETIC STORM MAIN PHASES DURING CIR AND ICME EVENTS R. Boroev & M. Vasiliev 10.12737/stp-61202004
17. Why have geomagnetic storms been so weak during the recent solar minimum and the rising phase of cycle 24? E. Kilpua et al. 10.1016/j.jastp.2013.11.001
18. The relationship between geomagnetic indices and the interplanetary medium parameters in magnetic storm main phases during CIR and ICME events R. Boroyev et al. 10.1016/j.jastp.2020.105290
19. Relationship between geomagnetic storm development and the solar wind parameter ß N. Kurazhkovskaya et al. 10.12737/stp-74202104
20. Dependence of geomagnetic activity during magnetic storms on the solar wind parameters for different types of streams: 2. Main phase of storm N. Nikolaeva et al. 10.1134/S0016793212010082
21. Occurrence rate of extreme magnetic storms Y. Yermolaev et al. 10.1002/jgra.50467
22. Geoeffectiveness of stream interaction regions during 2007–2008 E. Sanchez‐Garcia et al. 10.1002/2016SW001559
23. Properties of the Sheath Regions of Coronal Mass Ejections with or without Shocks from STEREO in situ Observations near 1 au T. Salman et al. 10.3847/1538-4357/abbdf5
24. Relationship of the ASY-H index with interplanetary medium parameters and auroral activity in magnetic storm main phases during CIR and ICME events R. Boroev & M. Vasiliev 10.12737/szf-61202004
25. Substorm activity during the main phase of magnetic storms induced by the CIR and ICME events R. Boroyev & M. Vasiliev 10.1016/j.asr.2017.10.031
26. Geoeffective Properties of Solar Transients and Stream Interaction Regions E. Kilpua et al. 10.1007/s11214-017-0411-3
27. Studying auroral activity using the SME index at the magnetic storm main phase during CIR and ICME events R. Boroev & M. Vasiliev 10.12737/stp-74202103
28. Can We Estimate the Intensities of Great Geomagnetic Storms (ΔSYM-H ≤ −200 nT) with the Burton Equation or the O’Brien and McPherron Equation? M. Zhao et al. 10.3847/1538-4357/ac50a8
29. Role of the variable solar wind in the dynamics of small-scale magnetosheath structures L. Rakhmanova et al. 10.3389/fspas.2023.1121230
30. Unraveling the drivers of the storm time radiation belt response E. Kilpua et al. 10.1002/2015GL063542
31. Dynamics of large‐scale solar wind streams obtained by the double superposed epoch analysis Y. Yermolaev et al. 10.1002/2015JA021274
32. North–South IMF Disturbance Detection via an Adaptive Filter Approach E. Schmölter & J. Berdermann 10.3390/atmos13091482
33. Dynamics of Large-Scale Solar-Wind Streams Obtained by the Double Superposed Epoch Analysis: 2. Comparisons of CIRs vs. Sheaths and MCs vs. Ejecta Y. Yermolaev et al. 10.1007/s11207-017-1205-1
34. The auroral activity during the main phase of magnetic storms R. Boroyev & M. Vasiliev 10.1016/j.asr.2022.10.034
35. Does the duration of the magnetic storm recovery phase depend on the storm development rate in its main phase? Y. Yermolaev et al. 10.1134/S0016793215040039
36. The Influence of Parameters of the Interplanetary Medium and Magnetosheath Boundaries on the Correlation Coefficient between the Ion Flux Measured in the Solar Wind and the Magnetosheath L. Rakhmanova et al. 10.1134/S0016793218040138
37. Statistical Study of the Effect of Different Solar Wind Types on Magnetic Storm Generation During 1995–2016 L. Dremukhina et al. 10.1134/S0016793218060038
38. Prediction of the Dst Index and Analysis of Its Dependence on Solar Wind Parameters Using Neural Network A. Lethy et al. 10.1029/2018SW001863
39. Some problems of identifying types of large-scale solar wind and their role in the physics of the magnetosphere Y. Yermolaev et al. 10.1134/S0010952517030029
40. Studying auroral activity using the SME index at the magnetic storm main phase during CIR and ICME events R. Boroev & M. Vasiliev 10.12737/szf-74202103
41. Dependence of geomagnetic activity during magnetic storms on solar-wind parameters for different types of streams: 4. Simulation for magnetic clouds N. Nikolaeva et al. 10.1134/S0016793214020145
42. Зависит ли генерация магнитной бури от типа солнечного ветра?, "Геомагнетизм и аэрономия" Н. Николаева et al. 10.7868/S0016794017050169
43. Relationship between the Parameters of Various Solar Wind Types and Geomagnetic Activity Indices L. Dremukhina et al. 10.1134/S0010952518060011
44. What Solar–Terrestrial Link Researchers Should Know about Interplanetary Drivers Y. Yermolaev et al. 10.3390/universe7050138
45. Geosynchronous Magnetopause Crossings and Their Relationships With Magnetic Storms and Substorms A. Samsonov et al. 10.1029/2020SW002704
46. Empirical Modeling of the Geomagnetosphere for SIR and CME‐Driven Magnetic Storms V. Andreeva & N. Tsyganenko 10.1029/2018JA026008
47. Dynamics of Large-Scale Solar-Wind Streams Obtained by the Double Superposed Epoch Analysis: 3. Deflection of the Velocity Vector Y. Yermolaev et al. 10.1007/s11207-018-1310-9
48. Dynamics of Large‐Scale Solar‐Wind Streams Obtained by the Double Superposed Epoch Analysis: 4. Helium Abundance Y. Yermolaev et al. 10.1029/2020JA027878
49. Empirical Relationship Between CME Parameters and Geo-effectiveness of Halo CMEs in the Rising Phase of Solar Cycle 24 (2011 – 2013) A. Shanmugaraju et al. 10.1007/s11207-015-0671-6
50. Relationship between geomagnetic storm development and the solar wind parameter β N. Kurazhkovskaya et al. 10.12737/szf-74202104
51. Characteristics and development of the main phase disturbance in geomagnetic storms (Dst⩽-50nT) O. Ahmed et al. 10.1016/j.asr.2024.01.050
52. Dynamics of Interplanetary Parameters and Geomagnetic Indices during Magnetic Storms Induced by Different Types of Solar Wind L. Dremukhina et al. 10.1134/S0016793219060069
53. Impact of solar wind parameters on geomagnetic activity during the main phase of strong magnetic storms R. Boroyev 10.1016/j.jastp.2025.106485
54. Influence of the interplanetary driver type on the durations of the main and recovery phases of magnetic storms Y. Yermolaev et al. 10.1002/2014JA019826
55. Geomagnetic storm forecasting service StormFocus: 5 years online T. Podladchikova et al. 10.1051/swsc/2018017
56. Recovery phase of magnetic storms induced by different interplanetary drivers Y. Yermolaev et al. 10.1029/2012JA017716
57. Double Superposed Epoch Analysis of Geomagnetic Storms and Corresponding Solar Wind and IMF in Solar Cycles 23 and 24 V. Manu et al. 10.1029/2022SW003314
58. Statistic study of the geoeffectiveness of compression regions CIRs and Sheaths Y. Yermolaev et al. 10.1016/j.jastp.2018.01.027
59. Changes in and Recovery of the Turbulence Properties in the Magnetosheath for Different Solar Wind Streams L. Rakhmanova et al. 10.3390/universe10050194
60. Relationships Between Interplanetary Coronal Mass Ejection Characteristics and Geoeffectiveness in the Rising Phase of Solar Cycles 23 and 24 M. Lawrance et al. 10.1007/s11207-016-0911-4
61. Properties and geoeffectiveness of magnetic clouds during solar cycles 23 and 24 N. Gopalswamy et al. 10.1002/2015JA021446
62. Magnetic field fluctuation properties of coronal mass ejection-driven sheath regions in the near-Earth solar wind E. Kilpua et al. 10.5194/angeo-38-999-2020
63. Differences in the Dynamics of the Asymmetrical Part of the Magnetic Disturbance during the Periods of Magnetic Storms Induced by Different Interplanetary Sources L. Dremukhina et al. 10.1134/S0016793220060031
64. Modeling of the corrected D st * index temporal profile on the main phase of the magnetic storms generated by different types of solar wind N. Nikolaeva et al. 10.1134/S0010952515020070
65. Geomagnetic storm forecasting from solar coronal holes S. Nitti et al. 10.1093/mnras/stac3533
66. Geoeffectiveness and efficiency of CIR, sheath, and ICME in generation of magnetic storms Y. Yermolaev et al. 10.1029/2011JA017139
67. Does magnetic storm generation depend on the solar wind type? N. Nikolaeva et al. 10.1134/S0016793217050152
68. Correlation between auroral activity and rate of development of a storm in its main phase Р. Бороев & R. Boroev 10.12737/24270