Physics
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phflb...5.2638g&link_type=abstract
Physics of Fluids B (ISSN 0899-8221), vol. 5, no. 7, pt. 2, p. 2638-2645.
Physics
27
Magnetic Storms, Solar Activity, Solar Corona, Solar Terrestrial Interactions, Stellar Mass Ejection, Geomagnetism, Magnetic Field Configurations, Solar Cycles
Scientific paper
The phenomenon of coronal mass ejections (CME) is examined with reference to recent work in this field. In particular, attention is given to CMEs close to the sun, CMEs in interplanetary space, solar cycle variations of CMEs, and magnetic field topology and the problem of magnetic flux balance in interplanetary space. It is demonstrated that transient ejections of material from the sun are the cause of almost all large nonrecurrent geomagnetic substorms, as originally suggested by Chapman and his colleagues.
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