| タイトル | A multi-wavelength analysis of the February 6/7, 1997 coronal mass ejection |
| 著者（英） | Kosugi, T.; Thompson, B. J.; Nitta, N.; Gopalswamy, N.; Kundu, M. R.; Plunkett, S. P.; Hudson, H. S.; Gurman, J. B.; Burkpile, J. T.; Howard, R. A.; Hanaoka, Y.; Lepping, R. P. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 1997-09-01 |
| 言語 | eng |
| 内容記述 | The coronal mass ejection (CME) event on 6 to 7 February 1997 that originate from the southwest quadrant of the sun are analyzed. The CME is accelerated from a projected speed of 170 km/s to about 650 km/s at 25 solar radii. The CME is an arcade eruption followed by bright prominence core structures. The CME was accompanied by an arcade formation. The X-ray and extreme ultraviolet observations suggest that the reconnection proceeded from the northwest and the southeast end of a filament channel. The CME event caused interplanetary effects that produced a medium size geomagnetic storm on earth. Issues relating to the origin and propagation of geo-effective solar disturbances are addressed. |
| NASA分類 | Solar Physics |
| 権利 | No Copyright, Distribution within the U.S. granted by agreement |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/540368 |
|
