Смекни!
smekni.com

Физические основы прогнозирования возмущений в околоземной среде по характеристикам Солнца (стр. 2 из 2)

8. Gosling J.T., Borrini G., Asbridge J.R. et al. Coronal streamers in the solar wind at 1 a.u. // J. Geophys. Res. 1981. V. 82. P. 5438.

9. Hundhausen A.J. Sizes and locations of coronal mass ejections: SMM observations from 1980 and 1984 - 1989 // J. Geophys. Res. 1993. V. 98. P. 13177.

10. Korzhov N.P. Large-scale three dimensional structure of the interplanetary magnetic field // Solar Phys. 1977. V. 55. P. 505.

11. Mendoza, B., Perez-Enriquez R. Association of coronal mass ejections with the heliomagnetic current sheet // J. Geophys. Res. 1993. V. 98. P. 9365.

12. Svalgaard L., Wilcox J.M., Duvall T.L. A model combining the solar and sector structured polar magnetic field // Solar Phys. 1974. V. 37. P.157.

13. Wilcox J.M., Hundhausen A.J. Comparison of heliospheric current sheet structure obtained from potential magnetic field computations and from observed polarization coronal brightness // J. Geophys. Res. 1983. V. 88. P. 8095. ИСЗФ СО РАН, Иркутск