Geodesic
Two-particle kinetic model of the solar wind in approximation of frozenin magnetic field
Vestnik Tomskogo gosudarstvennogo universiteta. Matematika i mehanika, no. 1 (2007), pp. 72-78 Cet article a éte moissonné depuis la source Math-Net.Ru

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The suggested kinetic model of the solar plasma flow is based on the equation for two-particle probability distribution of electron and proton velocities, Maxwell equations, and the assumptions about a Parker type frozen-in magnetic field. The dependences derived for speed, density, and flux of plasma are consistent with bservational data for the solar wind. The restrictions to the presented model that result from the analysis of the drift equation for charged particles in the interplanetary magnetic field are discussed. 
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N. R. Min'kova. Two-particle kinetic model of the solar wind in approximation of frozenin magnetic field. Vestnik Tomskogo gosudarstvennogo universiteta. Matematika i mehanika, no. 1 (2007), pp. 72-78. http://geodesic.mathdoc.fr/item/VTGU_2007_1_a10/

[1] Lemaire J., Scherer M., “Kinetic models of the solar wind”, J. Geophys. Res., 76 (1971), 7479–7490 | DOI

[2] Vasenin Y.M., Minkova N.R., “Two-particle quasi-neutral kinetic model of collisionless solar wind”, J. Phys. A: Math. and General., 36 (2003), 6215–6220 | DOI | MR | Zbl

[3] Pierrard V., Issautier K., Meyer-Vernet N., Lemaire J., “Collisionless model of the solar wind in a spiral magnetic field”, Geophys. Res. Lett., 28:2 (2001), 223–226 | DOI

[4] Vasenin Y.M., Shamin A.V., Minkova N.R., “Solar wind kinetic model depending on rotation and magnetic field of the Sun”, 11th Int. Workshop on the Physics of Non-Ideal Plasmas (Valencia, Spain, 2003), Abstracts Book, 2003, 177

[5] Minkova N.R., “The kinetic model of the solar wind influenced by the given magnetic field”, Solar variability and its magnetic origin (IAUS 233), Proc. of the Int. Astronomical Union Symp. and Coll., Cambridge University Press, 2006, 311–312

[6] Parker E.N., “Dynamics of the interplanetary gas and magnetic fields”, Astrophys. J., 128 (1958), 664–676 | DOI

[7] Minkova N.R., “O zadanii vmorozhennogo magnitnogo polya v kineticheskikh modelyakh solnechnogo vetra”, Modelirovanie neravnovesnykh sistem-2006, Materialy IX Vserossiiskogo seminara, Krasnoyarsk, 2006, 121–122

[8] Wang Y.-M., Sheeley N.R., Jr., “Solar implications of Ulysses interplanetary field measurements”, Astrophys. J. Lett., 447 (1995), L143–L146 | DOI

[9] Koehnlein W., “Radial gependence of solar wind parameters in the ecliptic (1.1R61 AU)”, Solar Physics, 169 (1996), 209–213 | DOI

[10] Fisher R., Guhathakurta M., “Physical properties of the polar coronal rays and holes as observed with SPARTAN 201-01 coronograph”, Astrophys. J., 447 (1995), L139 | DOI

[11] Esser R., Habbal S., Coles W.A., Hollweg J.V., “Hot protons in the inner corona and their effect on the flow properties of the solar wind”, J. Geophys. Res, 102 (1997), 7063–7069 | DOI