Zobrazeno 1 - 7
of 7
pro vyhledávání: '"K. B. Kaportseva"'
Autor:
K. B. Kaportseva, Yu. S. Shugay
Publikováno v:
Cosmic Research. 59:268-279
Abstract This paper analyzes the results of modeling coronal mass ejection (CME) propagation in 2010–2011 obtained using input data from different sources: CME catalogs SEEDS and CACTus, and predictions of the velocity of quasi-stationary solar win
Autor:
K. B. Kaportseva, Yu. S. Shugay
Publikováno v:
Geomagnetism and Aeronomy. 61:158-168
The results of the forecasting of quasi-stationary and transient solar wind streams velocity for a period from May to December 2010 are presented. The velocity of quasi-stationary solar wind streams on the near-Earth orbit was calculated with the emp
Autor:
Igor Veselovsky, K. B. Kaportseva
Publikováno v:
Geomagnetism and Aeronomy. 59:257-264
The results from a statistical analysis of solar wind data obtained near the Earth’s orbit by the DSCOVR spacecraft for the period of one year starting August 2016 are discussed. The distribution of the solar wind temperature T for this period was
Autor:
D. G. Rodkin, Igor Veselovsky, K. B. Kaportseva, Vladimir Slemzin, A. T. Lukashenko, Yu. S. Shugay
Publikováno v:
Cosmic Research. 57:18-28
The paper considers the classification of solar wind streams in magnetohydrodynamic parameters (MHD-types); combinations of proton speed, density, temperature, and magnetic field strength, in addition to the classical solar wind separation into high-
Publikováno v:
Solar System Research. 53:56-67
At the present time, there is no generally accepted classification of the solar wind flows. There are various approaches to this problem depending on the goal of the study. In our paper, we propose the binary classification of the solar wind types by
Publikováno v:
Physics of Atomic Nuclei. 81:766-770
A binary classification of solar wind types is given according to three main hydrodynamic parameters—the proton speed, the proton temperature, and the proton density. Boundaries between the fast–hot–dense, fast–hot–rarefied, fast–cold–d
Autor:
K. B. Kaportseva, Yu. S. Shugay
Publikováno v:
Cosmic Research. 59:537-537