127 citations · 408 across the 11 of their papers we have counts for
11 papers
Dynamics of large-scale solar-wind streams obtained by the double superposed epoch analysis. 4. Helium abundance
Yu. I. Yermolaev, I. G. Lodkina, M. Yu. Yermolaev +7
This work is a continuation of our previous articles (Yermolaev et al. in J. Geophys. Res. 120, 7094, 2015; Yermolaev et al. in Solar Phys. 292, 193, 2017; Yermolaev et al. in Sola…
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. 2. CIR.vs.Sheath and MC.vs.Ejecta comparisons
Yu. I. Yermolaev, I. G. Lodkina, N. S. Nikolaeva +1
This work is a continuation of our previous paper [Yermolaevetal2015] which describes the average temporal profiles of interplanetary plasma and field parameters in large-scale sol…
Does generation of magnetic storm depend on type of solar wind?
N. S. Nikolaeva, Yu. I. Yermolaev, I. G. Lodkina
The purpose of this work is to draw attention of readers to a problem of possible differences in generation of magnetic storms induced by various large scale solar wind (SW) stream…
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…
Recovery phase of magnetic storms induced by different interplanetary drivers
Yu. I. Yermolaev, I. G. Lodkina, N. S. Nikolaeva +1
Statistical analysis of Dst behaviour during recovery phase of magnetic storms induced by different types of interplanetary drivers is made on the basis of OMNI data in period 1976…
Geoeffectiveness and efficiency of CIR, Sheath and ICME in generation of magnetic storms
Yu. I. Yermolaev, N. S. Nikolaeva, I. G. Lodkina +1
We investigate relative role of various types of solar wind streams in generation of magnetic storms. On the basis of the OMNI data of interplanetary measurements for the period of…
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…
The floor in the interplanetary magnetic field: Estimation on the basis of relative duration of ICME observations in solar wind during 1976-2000
Yu. I. Yermolaev, I. G. Lodkina, N. S. Nikolaeva +1
To measure the floor in interplanetary magnetic field and estimate the time- invariant open magnetic flux of Sun, it is necessary to know a part of magnetic field of Sun carried aw…