Zobrazeno 1 - 10
of 127
pro vyhledávání: '"Lodkina I. G."'
Autor:
Yermolaev Y. I., Lodkina I. G., Khokhlachev A. A., Yermolaev M. Y., Riazantseva M. O., Rakhmanova L. S., Borodkova N. L., Sapunova O. V., Moskaleva A. V.
Publikováno v:
Solar-Terrestrial Physics, Vol 9, Iss 4, Pp 55-62 (2023)
Solar activity and solar wind parameters decreased significantly in solar cycles (SCs) 23–24. In this paper, we analyze solar wind measurements at the rising phase of SC 25 and compare them with similar data from the previous cycles. For this purpo
Externí odkaz:
https://doaj.org/article/046253339960425ebc0973672abf12b1
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 by Song et al. (2021). Possible violations of the used assumptions do
Externí odkaz:
http://arxiv.org/abs/2107.14002
Autor:
Yermolaev, Yu. I., Lodkina, I. G.
A recent paper by Owens (2018) presents a statistical analysis of the properties of interplanetary coronal mass ejections (ICMEs) and variations in their compositions and ion charge-state signatures using data from the Advanced Composition Explorer (
Externí odkaz:
http://arxiv.org/abs/2008.05160
Autor:
Yermolaev, Yu. I., Lodkina, I. G., Yermolaev, M. Yu., Riazantseva, M. O., Rakhmanova, L. S., Borodkova, N. L., Shugay, Yu. S., Slemzin, V. A., Veselovsky, I. S., Rodkin, D. G.
Publikováno v:
Journal of Geophysical Research: Space Physics, 2020
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 Solar Phys. 293, 91, 2018), which describe the average temporal profiles o
Externí odkaz:
http://arxiv.org/abs/1807.03579
Publikováno v:
Solar Physics, 2018
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 average temporal profiles of interplanetary plasma and field parameters in
Externí odkaz:
http://arxiv.org/abs/1802.08875
Autor:
Yermolaev, Yu. I., Lodkina, I. G., Shugay, Yu. S., Slemzin, V. A., Veselovsky, I. S., Rodkin, D. G., Nikolaeva, N. S., Borodkova, N. L., Yermolaev, M. Yu.
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 December 2011 - January 2012. We analyze two cases. (1) In CR 2118 instead
Externí odkaz:
http://arxiv.org/abs/1610.03757
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 solar-wind (SW) streams: CIR, ICME (both MC and Ejecta) and Sheath as wel
Externí odkaz:
http://arxiv.org/abs/1602.08899
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) streams: CIR, Sheath and ICME (including MC and Ejecta). Recently we showed
Externí odkaz:
http://arxiv.org/abs/1602.05826
Publikováno v:
J. Geophys. Res. Space Physics, 2015, 120
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 (both MC and Ejecta) and Sheath as well as the interplanetary shock (IS).
Externí odkaz:
http://arxiv.org/abs/1503.08287
Publikováno v:
Journal of Geophysical Research: Space Physics, Volume 119, Issue 10, pp. 8126-8136, 2014
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 basis of OMNI data base during 1976-2000. Durations of both main and r
Externí odkaz:
http://arxiv.org/abs/1312.7787