74 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
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
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.
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.
5. Analysis of Quasistationary Solar Wind Stream Forecasts for 2010–2019 Y. Shugai
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.
7. Influence of coronal mass ejections on parameters of high-speed solar wind: a case study Y. Shugay et al.
8. Properties of the Geomagnetic Storm Main Phase and the Corresponding Solar Wind Parameters on 21–22 October 1999 Q. Li et al.
9. Predicted dependence of the cross polar cap potential saturation on the type of solar wind stream N. Nikolaeva et al.
10. Dependence of radiation belt flux depletions at geostationary orbit on different solar drivers during intense geomagnetic storms S. Gokani et al.
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.
12. The Magnetic Storm of August 25–26, 2018: Dayside High Latitude Geomagnetic Variations and Pulsations N. Kleimenova et al.
13. Effects of Geometries and Substructures of ICMEs on Geomagnetic Storms J. Lee et al.
14. Understanding the variability of magnetic storms caused by ICMEs R. Benacquista et al.
15. Relationship between substorm activity and the interplanetary medium parameters during the main phase of strong magnetic storms R. Boroyev
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
17. Hysteresis cycles and invariance of the Dst index form during geomagnetic storm development N. Kurazhkovskaya et al.
18. Why have geomagnetic storms been so weak during the recent solar minimum and the rising phase of cycle 24? E. Kilpua et al.
19. The relationship between geomagnetic indices and the interplanetary medium parameters in magnetic storm main phases during CIR and ICME events R. Boroyev et al.
20. Statistical study of interplanetary condition effect on geomagnetic storms: 2. Variations of parameters Y. Yermolaev et al.
21. Relationship between geomagnetic storm development and the solar wind parameter ß N. Kurazhkovskaya et al.
22. 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.
23. Occurrence rate of extreme magnetic storms Y. Yermolaev et al.
24. Geoeffectiveness of stream interaction regions during 2007–2008 E. Sanchez‐Garcia et al.
25. 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.
26. 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
27. 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.
28. Substorm activity during the main phase of magnetic storms induced by the CIR and ICME events R. Boroyev & M. Vasiliev
29. Geoeffective Properties of Solar Transients and Stream Interaction Regions E. Kilpua et al.
30. Studying auroral activity using the SME index at the magnetic storm main phase during CIR and ICME events R. Boroev & M. Vasiliev
31. 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.
32. Role of the variable solar wind in the dynamics of small-scale magnetosheath structures L. Rakhmanova et al.
33. Unraveling the drivers of the storm time radiation belt response E. Kilpua et al.
34. Dynamics of large‐scale solar wind streams obtained by the double superposed epoch analysis Y. Yermolaev et al.
35. North–South IMF Disturbance Detection via an Adaptive Filter Approach E. Schmölter & J. Berdermann
36. The polytropic behaviour and turbulence properties of sub-Alfvénic intervals K. Choraghe et al.
37. 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.
38. The auroral activity during the main phase of magnetic storms R. Boroyev & M. Vasiliev
39. Does the duration of the magnetic storm recovery phase depend on the storm development rate in its main phase? Y. Yermolaev et al.
40. 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.
41. Statistical Study of the Effect of Different Solar Wind Types on Magnetic Storm Generation During 1995–2016 L. Dremukhina et al.
42. Prediction of the Dst Index and Analysis of Its Dependence on Solar Wind Parameters Using Neural Network A. Lethy et al.
43. Some problems of identifying types of large-scale solar wind and their role in the physics of the magnetosphere Y. Yermolaev et al.
44. Studying auroral activity using the SME index at the magnetic storm main phase during CIR and ICME events R. Boroev & M. Vasiliev
45. 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.
46. Зависит ли генерация магнитной бури от типа солнечного ветра?, "Геомагнетизм и аэрономия" Н. Николаева et al.
47. Relationship between the Parameters of Various Solar Wind Types and Geomagnetic Activity Indices L. Dremukhina et al.
48. What Solar–Terrestrial Link Researchers Should Know about Interplanetary Drivers Y. Yermolaev et al.
49. Geosynchronous Magnetopause Crossings and Their Relationships With Magnetic Storms and Substorms A. Samsonov et al.
50. Empirical Modeling of the Geomagnetosphere for SIR and CME‐Driven Magnetic Storms V. Andreeva & N. Tsyganenko
51. Dynamics of Large-Scale Solar-Wind Streams Obtained by the Double Superposed Epoch Analysis: 3. Deflection of the Velocity Vector Y. Yermolaev et al.
52. Dynamics of Large‐Scale Solar‐Wind Streams Obtained by the Double Superposed Epoch Analysis: 4. Helium Abundance Y. Yermolaev et al.
53. 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.
54. Relationship between geomagnetic storm development and the solar wind parameter β N. Kurazhkovskaya et al.
55. Characteristics and development of the main phase disturbance in geomagnetic storms (Dst⩽-50nT) O. Ahmed et al.
56. Dynamics of Interplanetary Parameters and Geomagnetic Indices during Magnetic Storms Induced by Different Types of Solar Wind L. Dremukhina et al.
57. Impact of solar wind parameters on geomagnetic activity during the main phase of strong magnetic storms R. Boroyev
58. Influence of the interplanetary driver type on the durations of the main and recovery phases of magnetic storms Y. Yermolaev et al.
59. Geomagnetic storm forecasting service StormFocus: 5 years online T. Podladchikova et al.
60. Catalogs of Solar Wind Types and Their Role in Solar–Terrestrial Physics I. Lodkina et al.
61. Recovery phase of magnetic storms induced by different interplanetary drivers Y. Yermolaev et al.
62. Double Superposed Epoch Analysis of Geomagnetic Storms and Corresponding Solar Wind and IMF in Solar Cycles 23 and 24 V. Manu et al.
63. Statistic study of the geoeffectiveness of compression regions CIRs and Sheaths Y. Yermolaev et al.
64. Changes in and Recovery of the Turbulence Properties in the Magnetosheath for Different Solar Wind Streams L. Rakhmanova et al.
65. Hysteresis cycles and invariance of the Dst index form during geomagnetic storm development N. Kurazhkovskaya et al.
66. Relationships Between Interplanetary Coronal Mass Ejection Characteristics and Geoeffectiveness in the Rising Phase of Solar Cycles 23 and 24 M. Lawrance et al.
67. Properties and geoeffectiveness of magnetic clouds during solar cycles 23 and 24 N. Gopalswamy et al.
68. Magnetic field fluctuation properties of coronal mass ejection-driven sheath regions in the near-Earth solar wind E. Kilpua et al.
69. 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.
70. 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.
71. Geomagnetic storm forecasting from solar coronal holes S. Nitti et al.
72. Geoeffectiveness and efficiency of CIR, sheath, and ICME in generation of magnetic storms Y. Yermolaev et al.
73. Does magnetic storm generation depend on the solar wind type? N. Nikolaeva et al.
74. Correlation between auroral activity and rate of development of a storm in its main phase Р. Бороев & R. Boroev