77 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 https://doi.org/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 https://doi.org/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. https://doi.org/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. https://doi.org/10.1134/S001679321603004X
5. Analysis of Quasistationary Solar Wind Stream Forecasts for 2010–2019 Y. Shugai https://doi.org/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. https://doi.org/10.1134/S0038094616010032
7. Influence of coronal mass ejections on parameters of high-speed solar wind: a case study Y. Shugay et al. https://doi.org/10.1051/swsc/2018015
8. Statistical study of predictive parameters for geomagnetic storms during solar cycles 23–24 B. Tsegmed & B. Namuun https://doi.org/10.12737/szf-122202604
9. Properties of the Geomagnetic Storm Main Phase and the Corresponding Solar Wind Parameters on 21–22 October 1999 Q. Li et al. https://doi.org/10.3390/universe8070346
10. Predicted dependence of the cross polar cap potential saturation on the type of solar wind stream N. Nikolaeva et al. https://doi.org/10.1016/j.asr.2015.06.029
11. Dependence of radiation belt flux depletions at geostationary orbit on different solar drivers during intense geomagnetic storms S. Gokani et al. https://doi.org/10.3389/fspas.2022.952486
12. 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. https://doi.org/10.1134/S0010952513060038
13. The Magnetic Storm of August 25–26, 2018: Dayside High Latitude Geomagnetic Variations and Pulsations N. Kleimenova et al. https://doi.org/10.1134/S0016793219060070
14. Effects of Geometries and Substructures of ICMEs on Geomagnetic Storms J. Lee et al. https://doi.org/10.1007/s11207-018-1344-z
15. Understanding the variability of magnetic storms caused by ICMEs R. Benacquista et al. https://doi.org/10.5194/angeo-35-147-2017
16. Relationship between substorm activity and the interplanetary medium parameters during the main phase of strong magnetic storms R. Boroyev https://doi.org/10.1016/j.asr.2018.09.001
17. 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 https://doi.org/10.12737/stp-61202004
18. Hysteresis cycles and invariance of the Dst index form during geomagnetic storm development N. Kurazhkovskaya et al. https://doi.org/10.12737/szf-112202504
19. Why have geomagnetic storms been so weak during the recent solar minimum and the rising phase of cycle 24? E. Kilpua et al. https://doi.org/10.1016/j.jastp.2013.11.001
20. The relationship between geomagnetic indices and the interplanetary medium parameters in magnetic storm main phases during CIR and ICME events R. Boroyev et al. https://doi.org/10.1016/j.jastp.2020.105290
21. Statistical study of interplanetary condition effect on geomagnetic storms: 2. Variations of parameters Y. Yermolaev et al. https://doi.org/10.1134/S0010952511010035
22. Relationship between geomagnetic storm development and the solar wind parameter ß N. Kurazhkovskaya et al. https://doi.org/10.12737/stp-74202104
23. 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. https://doi.org/10.1134/S0016793212010082
24. Occurrence rate of extreme magnetic storms Y. Yermolaev et al. https://doi.org/10.1002/jgra.50467
25. Geoeffectiveness of stream interaction regions during 2007–2008 E. Sanchez‐Garcia et al. https://doi.org/10.1002/2016SW001559
26. 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. https://doi.org/10.3847/1538-4357/abbdf5
27. Features of turbulence development in the near-Earth space during May 2024 super storm L. Rakhmanova et al. https://doi.org/10.1186/s40623-026-02450-7
28. 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 https://doi.org/10.12737/szf-61202004
29. Non-Parker Spiral Interplanetary Magnetic Field Configurations Observed in Near-Earth Space: Statistical Features of Their Occurrence and Solar Wind Conditions J. Park et al. https://doi.org/10.3847/1538-4365/adea79
30. Substorm activity during the main phase of magnetic storms induced by the CIR and ICME events R. Boroyev & M. Vasiliev https://doi.org/10.1016/j.asr.2017.10.031
31. Geoeffective Properties of Solar Transients and Stream Interaction Regions E. Kilpua et al. https://doi.org/10.1007/s11214-017-0411-3
32. Studying auroral activity using the SME index at the magnetic storm main phase during CIR and ICME events R. Boroev & M. Vasiliev https://doi.org/10.12737/stp-74202103
33. 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. https://doi.org/10.3847/1538-4357/ac50a8
34. Role of the variable solar wind in the dynamics of small-scale magnetosheath structures L. Rakhmanova et al. https://doi.org/10.3389/fspas.2023.1121230
35. Unraveling the drivers of the storm time radiation belt response E. Kilpua et al. https://doi.org/10.1002/2015GL063542
36. Dynamics of large‐scale solar wind streams obtained by the double superposed epoch analysis Y. Yermolaev et al. https://doi.org/10.1002/2015JA021274
37. North–South IMF Disturbance Detection via an Adaptive Filter Approach E. Schmölter & J. Berdermann https://doi.org/10.3390/atmos13091482
38. The polytropic behaviour and turbulence properties of sub-Alfvénic intervals K. Choraghe et al. https://doi.org/10.1093/mnras/stag228
39. 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. https://doi.org/10.1007/s11207-017-1205-1
40. The auroral activity during the main phase of magnetic storms R. Boroyev & M. Vasiliev https://doi.org/10.1016/j.asr.2022.10.034
41. Does the duration of the magnetic storm recovery phase depend on the storm development rate in its main phase? Y. Yermolaev et al. https://doi.org/10.1134/S0016793215040039
42. 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. https://doi.org/10.1134/S0016793218040138
43. Statistical Study of the Effect of Different Solar Wind Types on Magnetic Storm Generation During 1995–2016 L. Dremukhina et al. https://doi.org/10.1134/S0016793218060038
44. Statistical study of predictive parameters for geomagnetic storms during solar cycles 23–24 B. Tsegmed & B. Namuun https://doi.org/10.12737/stp-122202604
45. Prediction of the Dst Index and Analysis of Its Dependence on Solar Wind Parameters Using Neural Network A. Lethy et al. https://doi.org/10.1029/2018SW001863
46. Some problems of identifying types of large-scale solar wind and their role in the physics of the magnetosphere Y. Yermolaev et al. https://doi.org/10.1134/S0010952517030029
47. Studying auroral activity using the SME index at the magnetic storm main phase during CIR and ICME events R. Boroev & M. Vasiliev https://doi.org/10.12737/szf-74202103
48. 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. https://doi.org/10.1134/S0016793214020145
49. Зависит ли генерация магнитной бури от типа солнечного ветра?, "Геомагнетизм и аэрономия" Н. Николаева et al. https://doi.org/10.7868/S0016794017050169
50. Relationship between the Parameters of Various Solar Wind Types and Geomagnetic Activity Indices L. Dremukhina et al. https://doi.org/10.1134/S0010952518060011
51. What Solar–Terrestrial Link Researchers Should Know about Interplanetary Drivers Y. Yermolaev et al. https://doi.org/10.3390/universe7050138
52. Geosynchronous Magnetopause Crossings and Their Relationships With Magnetic Storms and Substorms A. Samsonov et al. https://doi.org/10.1029/2020SW002704
53. Empirical Modeling of the Geomagnetosphere for SIR and CME‐Driven Magnetic Storms V. Andreeva & N. Tsyganenko https://doi.org/10.1029/2018JA026008
54. Dynamics of Large-Scale Solar-Wind Streams Obtained by the Double Superposed Epoch Analysis: 3. Deflection of the Velocity Vector Y. Yermolaev et al. https://doi.org/10.1007/s11207-018-1310-9
55. Dynamics of Large‐Scale Solar‐Wind Streams Obtained by the Double Superposed Epoch Analysis: 4. Helium Abundance Y. Yermolaev et al. https://doi.org/10.1029/2020JA027878
56. 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. https://doi.org/10.1007/s11207-015-0671-6
57. Relationship between geomagnetic storm development and the solar wind parameter β N. Kurazhkovskaya et al. https://doi.org/10.12737/szf-74202104
58. Characteristics and development of the main phase disturbance in geomagnetic storms (Dst⩽-50nT) O. Ahmed et al. https://doi.org/10.1016/j.asr.2024.01.050
59. Dynamics of Interplanetary Parameters and Geomagnetic Indices during Magnetic Storms Induced by Different Types of Solar Wind L. Dremukhina et al. https://doi.org/10.1134/S0016793219060069
60. Impact of solar wind parameters on geomagnetic activity during the main phase of strong magnetic storms R. Boroyev https://doi.org/10.1016/j.jastp.2025.106485
61. Influence of the interplanetary driver type on the durations of the main and recovery phases of magnetic storms Y. Yermolaev et al. https://doi.org/10.1002/2014JA019826
62. Geomagnetic storm forecasting service StormFocus: 5 years online T. Podladchikova et al. https://doi.org/10.1051/swsc/2018017
63. Catalogs of Solar Wind Types and Their Role in Solar–Terrestrial Physics I. Lodkina et al. https://doi.org/10.1134/S0010952524600215
64. Recovery phase of magnetic storms induced by different interplanetary drivers Y. Yermolaev et al. https://doi.org/10.1029/2012JA017716
65. Double Superposed Epoch Analysis of Geomagnetic Storms and Corresponding Solar Wind and IMF in Solar Cycles 23 and 24 V. Manu et al. https://doi.org/10.1029/2022SW003314
66. Statistic study of the geoeffectiveness of compression regions CIRs and Sheaths Y. Yermolaev et al. https://doi.org/10.1016/j.jastp.2018.01.027
67. Changes in and Recovery of the Turbulence Properties in the Magnetosheath for Different Solar Wind Streams L. Rakhmanova et al. https://doi.org/10.3390/universe10050194
68. Hysteresis cycles and invariance of the Dst index form during geomagnetic storm development N. Kurazhkovskaya et al. https://doi.org/10.12737/stp-112202504
69. Relationships Between Interplanetary Coronal Mass Ejection Characteristics and Geoeffectiveness in the Rising Phase of Solar Cycles 23 and 24 M. Lawrance et al. https://doi.org/10.1007/s11207-016-0911-4
70. Properties and geoeffectiveness of magnetic clouds during solar cycles 23 and 24 N. Gopalswamy et al. https://doi.org/10.1002/2015JA021446
71. Magnetic field fluctuation properties of coronal mass ejection-driven sheath regions in the near-Earth solar wind E. Kilpua et al. https://doi.org/10.5194/angeo-38-999-2020
72. 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. https://doi.org/10.1134/S0016793220060031
73. 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. https://doi.org/10.1134/S0010952515020070
74. Geomagnetic storm forecasting from solar coronal holes S. Nitti et al. https://doi.org/10.1093/mnras/stac3533
75. Geoeffectiveness and efficiency of CIR, sheath, and ICME in generation of magnetic storms Y. Yermolaev et al. https://doi.org/10.1029/2011JA017139
76. Does magnetic storm generation depend on the solar wind type? N. Nikolaeva et al. https://doi.org/10.1134/S0016793217050152
77. Correlation between auroral activity and rate of development of a storm in its main phase Р. Бороев & R. Boroev https://doi.org/10.12737/24270