Abstract
The method to estimate the low cutoff energy of non-thermal electrons in solar microwave and hard X-ray bursts is discussed in this paper. At first, for a given radiation mechanism, the ratio between two frequency (or energy) channels is calculated with different value of the cutoff to fit the observational data. Secondly, the cross point of the spectral profiles at different time for a given burst may provide the information of the low or high cutoff energy of non-thermal electrons. Two events on June 3 and 10, 2000 are studied with data of OVSA and YOHKOH.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 663-666 |
| Number of pages | 4 |
| Journal | European Space Agency, (Special Publication) ESA SP |
| Issue number | 535 |
| State | Published - 2003 |
| Event | Proceedings of the ISCS 2003; Solar Variability as an Input to the Earth's Environment - Tatranska Lomnica, Czech Republic Duration: Jun 23 2003 → Jun 28 2003 |
All Science Journal Classification (ASJC) codes
- Aerospace Engineering
- Space and Planetary Science
Keywords
- Hard X-ray
- Microwave
- Solar