Energy input for explosive events in the transition zone |
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| Authors: | G M Simnett |
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| Institution: | (1) School of Physics and Space Research, University of Birmingham, Edgbaston, B15 2TT Birmingham, UK |
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| 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. |
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| Keywords: | Sun Transition zone Explosive events |
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