Coronal mass ejections, flares, and geomagnetic storms

Details Coronal mass ejections, flares, and geomagnetic storms Coronal mass ejections, flares, and geomagnetic storms

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jgr...10320553l&link_type=abstract

Journal of Geophysical Research, Volume 103, Issue A9, p. 20553-20560

Astronomy and Astrophysics

Astrophysics

10

Interplanetary Physics: Interplanetary Shocks, Magnetospheric Physics: Solar Wind/Magnetosphere Interactions, Magnetospheric Physics: Storms And Substorms, Solar Physics, Astrophysics, And Astronomy: Flares

Scientific paper

We investigate the role of the coronal mass ejections (CMEs) (by using soft X ray solar emission as proxy data) in producing the nonrecurrent geomagnetic storms in the period 1969-1974. The linkage between these phenomena is confirmed: however, it turns out that CMEs associated with chromospheric flares, accompanied by type 4 radio emission, are the most effective in perturbing the geomagnetic field.

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