Abstract
It is shown that the solar flare electron spectra in a large energy range fit well with a power law in energy. This is used as a basis to discuss the possible division of solar flares into various groups, and also to compare the spectra of electrons in interplanetary space and at the flare site.
| Original language | English |
|---|---|
| Pages (from-to) | 209-211 |
| Number of pages | 3 |
| Journal | Solar Physics |
| Volume | 142 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 1 Nov 1992 |
| Externally published | Yes |
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