Zobrazeno 1 - 10
of 209
pro vyhledávání: '"VESELOVSKY, I. A."'
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
The paper addressed to the problem of the solar wind behaviour during the Maunder Minimum. Records on plasma tails of comets would allow to shed light on the physical parameters of the solar wind in the past. We analyse descriptions and drawings of c
Externí odkaz:
http://arxiv.org/abs/1805.04684
We analyzed statistics, solar sources and properties of interplanetary coronal mass ejections (ICMEs) in the solar wind. In comparison with the first eight years of Cycle 23, during the same period of Cycle 24 the yearly numbers of ICMEs were less co
Externí odkaz:
http://arxiv.org/abs/1802.05942
Autor:
Astapov, I. I., Barbashina, N. S., Borog, V. V., Veselovsky, I. S., Osetrova, N. V., Petrukhin, A. A., Shutenko, V. V.
According to CACTus catalog, during periods of a high solar activity every day up to tens of coronal mass ejections are observed. Such ejections have an impact on the flux of cosmic rays that permeate the space around us. Unlike most ground cosmic ra
Externí odkaz:
http://arxiv.org/abs/1701.00070
Autor:
Rodkin, D., Goryaev, F., Pagano, P., Gibb, G., Slemzin, V., Shugay, Yu., Veselovsky, I., Mackay, D. H.
We present study of the complex event consisting of several solar wind transients detected by Advanced Composition Explorer (ACE) on 4 -- 7 August 2011, that caused a geomagnetic storm with Dst$=-$110 nT. The supposed coronal sources -- three flares
Externí odkaz:
http://arxiv.org/abs/1610.05048
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
Autor:
Dmitriev, A. V., Suvorova, A. V., Chao, J. -K., Wang, C. B., Rastaetter, L., Panasyuk, M. I., Lazutin, L. L., Kovtyukh, A. S., Veselovsky, I. S., Myagkova, I. N.
Dynamics of the dayside magnetosphere and proton radiation belt was analyzed during unusual magnetic storm on 21 January 2005. We have found that during the storm from 1712 to 2400 UT, the subsolar magnetopause was continuously located inside geosync
Externí odkaz:
http://arxiv.org/abs/1402.0927
Publikováno v:
in Handbook on Solar Wind: Effects, Dynamics and Interactions, Ed. Hans E. Johannson, NOVA Science Publishers, Inc., New York, p. 81-144, 2009
The review presents analysis and physical interpretation of available statistical data about solar wind plasma and interplanetary magnetic field (IMF) properties as measured in-situ at 1 A.U. by numerous space experiments during time period from 1964
Externí odkaz:
http://arxiv.org/abs/1301.2929
From a broader perspective, the heliosphere and planetary magnetospheres provide a test bed to explore the plasma physics of the Universe. In particular, the underlying nonlinear coupling of different spatial and temporal scales plays a key role in d
Externí odkaz:
http://arxiv.org/abs/1005.4899
Autor:
Veselovsky, I. S.1,2 (AUTHOR) veselov@dec1.sinp.msu.ru, Kaportseva, K. B.3 (AUTHOR), Lukashenko, A. T.1 (AUTHOR) a_lu@mail.ru
Publikováno v:
Solar System Research. Jan2019, Vol. 53 Issue 1, p56-67. 12p.