99 citations · 280 across the 7 of their papers we have counts for
7 papers
Interaction of CME/ICME with HSS solar wind from coronal holes: case study
Yu. I. Yermolaev, I. G. Lodkina, Yu. S. Shugay +6
In this paper we look for traces of interaction of CME/ICME with high-speed stream (HSS) of solar wind from coronal hole (CH) for two serial Carrington rotations (CRs) during Decem…
Dynamics of large-scale solar-wind streams obtained by the double superposed epoch analysis
Yu. I. Yermolaev, I. G. Lodkina, N. S. Nikolaeva +1
Using the OMNI data for period 1976-2000 we investigate the temporal profiles of 20 plasma and field parameters in the disturbed large-scale types of solar wind (SW): CIR, ICME (bo…
Influence of the interplanetary driver type on the durations of main and recovery phases of magnetic storms
Yu. I. Yermolaev, I. G. Lodkina, N. S. Nikolaeva +1
We study durations of main and recovery phases of magnetic storms induced by different types of large-scale solar-wind streams (Sheath, magnetic cloud (MC), Ejecta and CIR) on the…
Dependence of the cross polar cap potential saturation on the type of solar wind streams
N. S. Nikolaeva, Yu. I. Yermolaev, I. G. Lodkina
We compare of the cross polar cap potential (CPCP) saturation during magnetic storms induced by various types of the solar wind drivers. By using the model of Siscoe-Hill \citep{Hi…
Occurrence rate of extreme magnetic storms
Yu. I. Yermolaev, I. G. Lodkina, N. S. Nikolaeva +1
Statistical analysis of occurrence rate of magnetic storms induced by different types of interplanetary drivers is made on the basis of OMNI data for period 1976-2000. Using our ca…
Specific interplanetary conditions for CIR-, Sheath-, and ICME-induced geomagnetic storms obtained by double superposed epoch analysis
Yu. I. Yermolaev, N. S. Nikolaeva, I. G. Lodkina +1
The comparison of specific interplanetary conditions for 798 magnetic storms with Dst < -50 nT for the period 1976-2000 was made on the basis of the OMNI archive data.We categorize…
Comment on "A statistical comparison of solar wind sources of moderate and intense geomagnetic storms at solar minimum and maximum" by Zhang, J.-C., M. W. Liemohn, J. U. Kozyra, M. F. Thomsen, H. A. Elliott, and J. M. Weygand, JGR, 2006
Yu. I. Yermolaev, M. Yu. Yermolaev, I. G. Lodkina
Conditions in the solar wind resulting in magnetic storms on the Earth are a subject of long and intensive investigations. Recently Zhang et al. (2006), published a paper, where th…