Abstract
Abstract
In this letter, I show that the discrepancies in the geoeffectiveness of halo coronal mass ejections (CMEs) reported in the literature arise due to the varied definitions of halo CMEs used by different authors. In particular, I show that the low geoeffectiveness rate is a direct consequence of including partial halo CMEs. The geoeffectiveness of partial halo CMEs is lower because they are of low speed and likely to make a glancing impact on Earth.
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Geology
Reference17 articles.
1. Gonzalez, W. D., J. A. Joselyn, Y. Kamide, H. W. Kroehl, G. Rostoker, B. T. Tsurutani, and V. M. Vasyliunas, What is a geomagnetic storm?, J. Geophys. Res., 99, 5771, 1994.
2. Gopalswamy, N., A global picture of CMEs in the inner heliosphere, in The Sun and the Heliosphere as an Integrated System, edited by G. Poletto and S. T. Suess, chap. 8, p. 201, Kluwer Acad., Boston, 2004.
3. Gopalswamy, N., S. Yashiro, Y. Liu, G. Michalek, A. Vourlidas, M. L. Kaiser, and R. A. Howard, Coronal mass ejections and other extreme characteristics of the 2003 October-November solar eruptions, J. Geophys. Res., 110, A09S15, doi:10.1029/2004JA010958, 2005.
4. Gopalswamy, N., S. Yashiro, and S. Akiyama, Geoeffectiveness of halo coronal mass ejections, J. Geophys. Res., 112, A06112, doi: 10.1029/2006JA012149, 2007.
5. Gopalswamy, N., S. Akiyama, S. Yashiro, G. Michalek, and R. P. Lepping, Solar sources and geospace consequences of interplanetary magnetic clouds observed during solar cycle 23, J. Atm. Sol. Terr. Phys., 70, 245, doi:10.1016/j.jastp.2007.08.070, 2008.
Cited by
25 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献