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History and development of coronal mass ejections as a key player in solar terrestrial relationship

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Figure

Fig. 1 a The 1909 May 12 solar eruption photographed by G. E. Hale in H-alpha. A filament erupted from a sunspot group located at S13E15, which was a good location for an eruption to have direct impact on Earth (from Hale 1931)
Fig. 2 Particle (a) and magnetometer (b) data from Pioneer-V show-ing the reduction in cosmic ray intensity by 28 % (Forbush decrease) associated with an interplanetary magnetic field enhancement
Fig. 4 80 MHz flux density (August 11). The source. The a Evolution of K-coronal intensity at a heliocentric distance of 1.5 Rʘ above the east limb (dashed line) compared with the evolution of solid curve)
Fig. 5 The height-time history of various substructures of a white-light coronal transient observed on 1973 January 11 by OSO-7
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