ISSN:
1572-9672
Keywords:
Sun
;
Transition zone
;
Explosive events
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract It is suggested that the energy input for explosive events in the transition zone comes from precipitating ions, typically of energies of a few×102 keV/nucleon, accelerated in the high corona. The energetics of the process are discussed, together with implications for coronal heating.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00777844
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