Temporal behaviour of the thermal model of hard X-ray bursts
โ Scribed by Alexander L. MacKinnon
- Publisher
- Springer
- Year
- 1985
- Tongue
- English
- Weight
- 557 KB
- Volume
- 98
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
A simple, analytic model is presented of a hot (> 108 K), thermal hard X-ray source, continuously heated, bounded by ion-acoustic conduction fronts, and expanding in a loop. The model is used to investigate the assumption, made in some published comparisons of this model with data, that the 'rise time' of the X-ray emission is approximately given by the loop length divided by the ion-sound speed appropriate to the peak temperature. It is found that a freely-expanding source does not behave in this way; instead, the rise time is symptomatic of the timescale for primary energy release. If the energy release rate does not fall significantly before the source fills the loop, however, then this assumption may be approximately satisfied, if a condition on the temporal behaviour of the energy release is satisfied.
Finally, some remarks on the relative timing of temperature and emission measure peaks are made, and possible further applications mentioned of the results presented herein.
๐ SIMILAR VOLUMES
A morphological study is made for the hard X-ray images (25-50 keV) of nine impulsive bursts observed by Hinotori. Most of them revealed single sources, either extended or compact, during the whole duration of the bursts. The sources of all of four spike bursts in the present sample are compact. Aft
The time histories of the emission at 10, 30, and 100 keV averaged over the loop from small and large loop thermal models of hard X-ray emission are studied. The small (15 000 km) loop cases show a characteristic delay in the peak of the 100 keV emission relative to the 30 keV emission of about 1.5