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- W2061880304 abstract "Coronal mass ejections (CMEs) are playing increasingly important roles in models developed to understand solar-terrestrial physics. A CME is characterized by a disruption or change in a helmet streamer, one of the radiant petals so prominent in solar eclipse pictures. This remarkable phenomenon, discovered in the 1970s, was long regarded a consequence of energetic processes occurring lower in the atmosphere, exemplified by solar flares. Now it appears that the roles are reversed—CMEs, not flares, are the driving process. In the revised picture, flares are frequent, but not necessary, consequences of CMEs; they follow instead of initiate events. CMEs are also geophysically effective. A recent statistical analysis shows they cause nearly 90% of large geomagnetic storms." @default.
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- W2061880304 date "1991-01-01" @default.
- W2061880304 modified "2023-10-17" @default.
- W2061880304 title "Geophysics news 1990: Heliosphere" @default.
- W2061880304 doi "https://doi.org/10.1029/90eo00069" @default.
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