Zobrazeno 1 - 10
of 66
pro vyhledávání: '"YU. Yermolaev"'
Autor:
S. Savin, L. Zelenyi, S. Romanov, I. Sandahl, J. Pickett, E. Amata, L. Avanov, J. Blecki, E. Budnik, J. Büchner, C. Cattell, G. Consolini, J. Fedder, S. Fuselier, H. Kawano, S. Klimov, V. Korepanov, D. Lagoutte, F. Marcucci, M. Mogilevsky, Z. Nemecek, B. Nikutowski, M. Nozdrachev, M. Parrot, J. L. Rauch, V. Romanov, T. Romantsova, C. T. Russell, J. Safrankova, J. A. Sauvaud, A. Skalsky, V. Smirnov, K. Stasiewicz, J. G. Trotignon, YU. Yermolaev
Publikováno v:
Annales Geophysicae, Vol 22, Pp 183-212 (2004)
We advance the achievements of Interball-1 and other contemporary missions in exploration of the magnetosheath-cusp interface. Extensive discussion of published results is accompanied by presentation of new data from a case study and a comparison o
Externí odkaz:
https://doaj.org/article/798c33191cd440f2aa5601f32ab42018
Autor:
S. Savin, J. Büchner, G. Consolini, B. Nikutowski, L. Zelenyi, E. Amata, H. U. Auster, J. Blecki, E. Dubinin, K. H. Fornacon, H. Kawano, S. Klimov, F. Marcucci, Z. Nemecek, A. Pedersen, J. L. Rauch, S. Romanov, J. Safrankova, J. A. Sauvaud, A. Skalsky, P. Song, Yu. Yermolaev
Publikováno v:
Nonlinear Processes in Geophysics, Vol 9, Iss 5/6, Pp 443-451 (2002)
We study properties of nonlinear magnetic fluctuations in the turbulent boundary layer (TBL) over polar cusps during a typical TBL crossing on 19 June 1998. Interball-1data in the summer TBL are compared with that of Geotail in solar wind (SW) and Po
Externí odkaz:
https://doaj.org/article/ce3977818c2c4e37ac68ecabcaa069b5
Publikováno v:
Annales Geophysicae, Vol 17, Pp 1145-1154 (1999)
Compressional waves with periods greater than 2 min (about 10-30 min) at low geomagnetic latitudes, namely compressional Pc5 waves, are studied. The data set obtained with magnetometer MIF-M and plasma analyzer instrument CORALL on board the Inter
Externí odkaz:
https://doaj.org/article/2a8aabd448274867a61918856cd3ca18
Publikováno v:
Universe, Vol 8, Iss 10, p 495 (2022)
Based on the data of the solar wind (SW) measurements of the OMNI database for the period 1976–2019, we investigate the behavior of SW types, as well as plasma and interplanetary magnetic field (IMF) parameters, for 21–24 solar cycles (SCs). Our
Externí odkaz:
https://doaj.org/article/f39692e7093c47f7bb3df26ab4930059
Autor:
Yuri I. Yermolaev, Irina G. Lodkina, Alexander A. Khokhlachev, Michael Yu. Yermolaev, Maria O. Riazantseva, Liudmila S. Rakhmanova, Natalia L. Borodkova, Olga V. Sapunova, Anastasiia V. Moskaleva
Publikováno v:
Universe, Vol 8, Iss 9, p 472 (2022)
In solar cycles 23–24, solar activity noticeably decreased and, as a result, solar wind parameters decreased. Based on the measurements of the OMNI base for the period 1976–2019, the time profiles of the main solar wind parameters and magnetosphe
Externí odkaz:
https://doaj.org/article/22d397b92a7a45e29a8e2f104b9c011d
Publikováno v:
ACTUAL PROBLEMS OF CONTINUUM MECHANICS: EXPERIMENT, THEORY, AND APPLICATIONS.
Publikováno v:
Cosmic Research. 58:492-500
One perturbed type of solar wind and magnetospheric disturbance drivers is the compression region in front of fast ICMEs—the Sheath region. In front of this region, an interplanetary shock is observed in approximately half of cases. However, the pa
Publikováno v:
Cosmic Research. 58:338-356
This paper is a continuation of our works [1, 2], in which we discussed some incorrect approaches to identifying large-scale types of solar wind and related incorrect conclusions drawn when analyzing the solar-terrestrial physics data. In this paper,
Autor:
I. G. Lodkina, Yu. Yermolaev
Publikováno v:
Космические исследования. 56:410-419
Publikováno v:
HIGH-ENERGY PROCESSES IN CONDENSED MATTER (HEPCM 2020): Proceedings of the XXVII Conference on High-Energy Processes in Condensed Matter, dedicated to the 90th anniversary of the birth of RI Soloukhin.