R Alfvén, H. (1981), Cosmic Plasma, Springer, New York.
Bernstein, I. B., E. A. Frieman, R. M. Kulsrud, and M. N. Rosenbluth (1960), Development of ion-sound instability, Phys. Fluids, 3, 136.
Borrini, G. J., T. Gosling, S. J. Bame, E. C. Feldman, and J. M. Wilcox (1981), Solar wind helium and hydrogen structure near the heliospheric current sheet: A signal of coronal streamers at 1 AU, J. Geophys. Res., 86, 4565.
Chashey, I. V. (1997), The role of MHD wave interaction in solar wind formation, Astron. Z., 74, 3.
Crooker, N. U., S. W. Kahler, J. T. Gosling, D. E. Larson, R. P. Lepping, E. J. Smith, and J. J. de Keyser (2001), Scales of heliospheric current sheet coherence between 1 and 5 AU, J. Geophys. Res., 106, 15,963.
Doschek, G. A., and U. Feldman (2000), Extreme-ultraviolet spectral line widths in quiet-sun coronal plasmas at distances of 1.03 R
Israelevich, P. L., T. I. Gombosi, A. I. Ershkovich, K. C. Hansen, C. P. T. Groth, D. L. DeZeeuw, and K. G. Powell (2001), MHD simulation of the three-dimensional structure of the heliospheric current sheet, Astron. Astrophys., 376, 288.
Koutchmy, S., and M. Livshits (1992), Coronal streamers, Space Sci. Rev., 61, 393.
Laval, G., R. Pellat, and M. Vullemin (1966), Dynamics of the geomagnetic tail, in: Plasma Physics and Controlled Nuclear Fusion Research, 2, p. 259, Int. Assoc. Energy Agency, Vienna, Austria.
Lui, A. T. Y. (1987), Magnetotail Physics, Johns Hopkins Univ. Press, Baltimore, Md.
Minami, S., M. Morimoto, A. I. Podgorny, and I. M. Podgorny (2002), Numerical simulation of a heliospheric current sheet creation due to coronal expansion, paper presented at 8th Asian-Pacific Regional Meeting, Int. Astron. Union, Tokyo, Japan.
Parker, E. N. (1963), Interplanetary Dynamical Processes, Interscience, Hoboken, N.J.
Pisanko, Yu. V. (1985), Calculation of stationary magnetohydrodynamic flows in formation of solar wind, Geomagn. Aeron. (in Russian), 25, 17.
Pneuman, G. W., and R. A. Kopp (1971), Gas-magnetic field interactions in the solar corona, Sol. Phys., 18, 258.
Podgorny, A. I., and I. M. Podgorny (1995), Current sheet creation by super-Alfvénic jet in dipolar field, Sol. Phys., 161, 165.
Podgorny, A. I., and I. M. Podgorny (1996), Electrodynamical model of the flare and solar flare prognosis, Astron. Soc. Pac. Conf. Ser., 95, 66.
Podgorny, I. M., A. I. Podgorny, S. Minami, and M. Morimoto (2004), An MHD model for a Heliospheric Current Sheet, Astronomy Report., 48, 433.
Seely, J. F., U. Feldman, U. Schuhle, K. Wilhelm, W. Curdt, and P. Lemaire (1997), Turbulent velocities and ion temperatures in the solar corona obtained from SUMER line widths, Astrophys. J., 484, L87.
Smith, E. J. (2001), The heliospheric current sheet, J. Geophys. Res., 106, 15,819.
Somov, B. V., and S. I. Syrovatsky (1971), Current sheet formation on field drag by solar wind, J. Exp. Theor. Phys. (in Russian), 61, 1864.
Usmanov, A. V. (1993), Interplanetary magnetic field structure and solar wind parameters as inferred from solar magnetic field observations and by using a numerical 2-D MHD model, Sol. Phys., 143, 345.
Usmanov, A. V. (1999), Magnetohydrodynamic models of solar wind, Dr. Sci. thesis (in Russian), St. Petersburg University, St. Petersburg, Russia.
