Zobrazeno 1 - 10
of 20
pro vyhledávání: '"D. V. Erofeev"'
Publikováno v:
Izvestiya vysshikh uchebnykh zavedenii. Radiofizika. 64:567-576
Publikováno v:
Proceedings of Tomsk State University of Control Systems and Radioelectronics. 23:7-14
Autor:
D. V. Erofeev
Publikováno v:
Geomagnetism and Aeronomy. 59:1081-1087
The arc-polarized Alfven waves observed in the near-Earth region of the heliosphere are studied with instruments of the WIND spacecraft in 1995–2011. Statistical distributions of the parameters characterizing the duration, amplitude, and nature of
Autor:
D. V. Erofeev
Publikováno v:
Geomagnetism and Aeronomy. 59:7-15
The behavior of the correlation between the radial BR and normal BN components of the interplanetary magnetic field (IMF) in the dependence on the time, the flow type of the solar wind, and the frequency of fluctuations has been studied with consider
Autor:
D. V. Erofeev
Publikováno v:
Geomagnetism and Aeronomy. 57:864-868
We consider a model that couples the magnetic field fluctuations in the heliosphere with random shifts of force line footpoints on the Sun. This model generalizes the Giacalone (2001) model by taking into account the large-scale inhomogeneity of the
Publikováno v:
Proceedings of Tomsk State University of Control Systems and Radioelectronics. 20:11-16
Autor:
D. V. Erofeev
Publikováno v:
Geomagnetism and Aeronomy. 56:1118-1123
In this paper, the heliolatitude dependence of the anisotropy of hourly interplanetary magnetic field fluctuations under conditions characteristic of low solar activity is studied. Measurements carried out by the Ulysses spacecraft in 1992–1994 and
Autor:
D. V. Erofeev
Publikováno v:
Geomagnetism and Aeronomy. 55:914-919
The ratio of regular and stochastic components in the behavior of the longitudinal-temporal distribution of solar activity is studied with the use of correlation and spectral analysis of data on sunspot groups for 12 solar cycles. It was found that d
Autor:
D. V. Erofeev
Publikováno v:
Geomagnetism and Aeronomy. 54:1032-1038
The variation in the IMF direction distribution during the 22-year solar magnetic cycle has been studied. Data obtained in near-Earth orbits and measurements in the heliospheric regions located far from the Earth, performed with the Helios and Ulysse
Autor:
D. V. Erofeev
Publikováno v:
Geomagnetism and Aeronomy. 53:822-826
Compressible fluctuations in solar wind plasma are analyzed on the basis of the 1995–2010 WIND and Advanced Composition Explorer (ACE) spacecraft data. In the low-speed solar wind (V0 < 430 km/s), correlations between fluctuations in the magnetic f