Zobrazeno 1 - 10
of 341
pro vyhledávání: '"Kuznetsov, V. D."'
Autor:
Kuznetsov, V . D., Osin, A. I.
The evolutionarity conditions for the MHD shock waves are considered within the framework of the 8-moment approximation for collisionless plasma with heat fluxes. In the general case, evolutionarity diagrams are obtained depending on the relative mag
Externí odkaz:
http://arxiv.org/abs/2310.10620
Autor:
Pezzi, O., Pecora, F., Roux, J. le, Engelbrecht, N. E., Greco, A., Servidio, S., Malova, H. V., Khabarova, O. V., Malandraki, O., Bruno, R., Matthaeus, W. H., Li, G., Zelenyi, L. M., Kislov, R. A., Obridko, V. N., Kuznetsov, V. D.
Publikováno v:
Space Sci. Rev. 217, 39 (2021)
Our understanding of processes occurring in the heliosphere historically began with reduced dimensionality - one-dimensional (1D) and two-dimensional (2D) sketches and models, which aimed to illustrate views on large-scale structures in the solar win
Externí odkaz:
http://arxiv.org/abs/2101.05007
Autor:
Kuznetsov, V. D., Osin, A. I.
The research is aimed at the study of the properties of solutions for parallel MHD shock waves in collisionless plasma with heat fluxes, using 8-moment MHD approximation. Restrictions have been established on the upstream shock parameters preserving
Externí odkaz:
http://arxiv.org/abs/2003.09928
Autor:
Khabarova, O. V., Obridko, V. N., Kislov, R. A., Malova, H. V., Bemporad, A., Zelenyi, L. M., Kuznetsov, V. D., Kharshiladze, A. F.
Publikováno v:
Plasma Physics Reports, 2018, Vol. 44, No. 9, pp. 840 -853
An extensive analysis of Ulysses observations of the solar wind speed V from 1990 to 2008 is undertaken. It is shown that the evolution of V with heliocentric distance r depends substantially on both the heliolatitude and the solar activity cycle. De
Externí odkaz:
http://arxiv.org/abs/1806.09604
Publikováno v:
Mechanics & Advanced Technologies; 2024, Vol. 8 Issue 2, p172-177, 6p
Publikováno v:
Journ. Magn. Magn. Mater. 368 (2014) 338-341
Magnetic properties of DNA liquid-crystal dispersions are experimentally investigated by SQUID magnetometer. The magnetic susceptibility of pure DNA and DNA doped by La, and Gd is measured in the region 4.2-300 K. The total magnetic moment is represe
Externí odkaz:
http://arxiv.org/abs/1309.4281
The RESIK instrument on {\em CORONAS-F} spacecraft observed several sulphur X-ray lines in three of its four channels covering the wavelength range 3.8-6.1 \AA\ during solar flares. The fluxes are analyzed to give the sulphur abundance. Data are chos
Externí odkaz:
http://arxiv.org/abs/1203.5888
The abundance of chlorine is determined from X-ray spectra obtained with the RESIK instrument on {\em CORONAS-F} during solar flares between 2002 and 2003. Using weak lines of He-like Cl, \ion{Cl}{16}, between 4.44 and 4.50 \AA, and with temperatures
Externí odkaz:
http://arxiv.org/abs/1106.1387
Observations of He-like and H-like Ar (Ar XVII and Ar XVIII) lines at 3.949 Angstroms and 3.733 Angstroms respectively with the RESIK X-ray spectrometer on the CORONAS-F spacecraft, together with temperatures and emission measures from the two channe
Externí odkaz:
http://arxiv.org/abs/1007.3574
The solar X-ray continuum emission at five wavelengths between 3.495 Angstroms and 4.220 Angstroms for 19 flares in a seven-month period in 2002--2003 was observed by the RESIK crystal spectrometer on CORONAS-F. In this wavelength region, free--free
Externí odkaz:
http://arxiv.org/abs/1001.2412