activity
20162021
collaborators

5 papers

astro-ph.SR2021

On the Probability of <<The Inhomogeneity of Composition Along the Magnetic Cloud Axis>>

Yu. I. Yermolaev, A. A. Khokhlachev, I. G. Lodkina

In the present work, we study the possibility of assessing the inhomogeneities of the ionic composition along the axis of the magnetic cloud using the method that was recently used…

astro-ph.SR2021

Drop of solar wind at the end of the 20th century

Yuri I. Yermolaev, Irina G. Lodkina, Alexander A. Khokhlachev +6

Variations in the solar wind (SW) parameters with scales of several years are an important characteristic of solar activity and the basis for a long-term space weather forecast. We…

physics.space-ph2018

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…

physics.space-ph2018

Dynamics of large-scale solar-wind streams obtained by the double superposed epoch analysis. 3. Deflection of speed vector

Yu. I. Yermolaev, I. G. Lodkina, M. Yu. Yermolaev

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), which describe the avera…

physics.space-ph2016

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…