Interpretation of Solar Hard X-ray Burst Polarisation Measurements
โ Scribed by BROWN, J. C.; MCCLYMONT, A. N.; MCLEAN, I. S.
- Book ID
- 109689342
- Publisher
- Nature Publishing Group
- Year
- 1974
- Tongue
- English
- Weight
- 227 KB
- Volume
- 247
- Category
- Article
- ISSN
- 0028-0836
- DOI
- 10.1038/247448a0
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๐ SIMILAR VOLUMES
A simple trap model of solar hard X-ray bursts is discussed in which nonthermal electrons trapped in a magnetic bottle precipitate into the lower chromosphere through the resonant scattering by whistlers. In -such a model, the X-ray spectra produced from trapped and precipitating electrons have 9 di
Observationally solar X bursts fall into three different categories: soft X bursts (E ,< I 0 keV), deka-keV bursts (10-150 keV), and very hard X bursts or deci-MeV bursts (200-1000 keV). The first kind is quasi-thermal, the last kind is non-thermal. The real existence of the third kind of burst look