太陽圏電流シート
出典: フリー百科事典『ウィキペディア（Wikipedia）』 (2022/05/14 07:14 UTC 版)
外部リンク
- The Heliospheric Current Sheet
- A Star With Two North Poles (features animation)
- The interplanetary magnetic field
- 3-Dimensional View of the Heliospheric Current Sheet
- NASA Astrophysics Data System article references (Online full text articles)
- ^ A Star with two North Poles, April 22, 2003, Science @ NASA
- ^ Riley, Pete; Linker, J. A.; Miki?, Z., "Modeling the heliospheric current sheet: Solar cycle variations", (2002) Journal of Geophysical Research (Space Physics), Volume 107, Issue A7, pp. SSH 8-1, CiteID 1136, DOI 10.1029/2001JA000299. (Full text Archived 2009年8月14日, at the Wayback Machine.)
- ^ Artist's Conception of the Heliospheric Current Sheet（2006年9月1日時点のアーカイブ）
- ^ a b c Israelevich, P. L., et al., "MHD simulation of the three-dimensional structure of the heliospheric current sheet" (2001) Astronomy and Astrophysics, v.376, p.288-291
- ^ Parker, E. N., "Dynamics of the Interplanetary Gas and Magnetic Fields", (1958) Astrophysical Journal, vol. 128, p.664
- ^ "Current Sheet Magnetic Model for the Solar Corona", K. H. Schatten, Cosmic Electrodynamics, 2, 232-245, 1971.
- ^ Rosenberg, R. L. and P. J. Coleman, Jr., Heliographic latitude dependence of the dominant polarity of the interplanetary magnetic field, J. Geophys. Res., 74 (24), 5611-5622, 1969.
- ^ Wilcox, J. M.; Scherrer, P. H.; Hoeksema, J. T., "The origin of the warped heliospheric current sheet" (1980)
- ^ Mursula, K.; Hiltula, T., "Bashful ballerina: Southward shifted heliospheric current sheet" (2003), Geophysical Research Letters, Volume 30, Issue 22, pp. SSC 2-1
- ^ Louise K. Harra, Keith O. Mason, Space Science 2004, Imperial College Press, ISBN 1860943616
- ^ Smith, E (1999-07). “The Sun, Solar Wind, and Magnetic Field”. Proceedings of the International School of Physics Enrico FERMI Varenna, Italy.
- ^ John M. Wilcox and Norman F. Ness, "Quasi-Stationary Corotating Structure in the Interplanetary Medium" (1965) Journal of Geophysical Research, 70, 5793.
- ^ Alfvén, H., Carlqvist, P (1978). “Interstellar clouds, the formation of stars”. Astrophysics and Space Science (Springer) 55 (2): 487-509. doi:10.1007/BF00642272.
- ^ 太陽風は彗星の「塵の尾」にも影響を及ぼす、アストロアーツ、2018年11月12日、2019年1月8日閲覧
[前の解説]
「太陽圏電流シート」の続きの解説一覧
- 1 太陽圏電流シートとは
- 2 太陽圏電流シートの概要
- 3 外部リンク
- 太陽圏電流シートのページへのリンク
