Halo coronal mass ejections and geomagnetic storms

Details Halo coronal mass ejections and geomagnetic storms Halo coronal mass ejections and geomagnetic storms

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ep%26s...61..595g&link_type=abstract

Earth, Planets and Space, Volume 61, p. 595-597.

Physics

Scientific paper

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.

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