Abstract
The dynamic spectral characteristics of the thermal model for solar hard X-ray bursts recently proposed by Brown et al. (1979) (BMS) are investigated. It is pointed out that this model, in which a single source is heated impulsively and cooled by anomalous conduction across an ion-acoustic turbulent thermal front, predicts that the total source emission measure should rise as the temperature falls. This prediction, which is common to all conductively cooled single-source models, is contrary to observations of many simple spike bursts. It is proposed, therefore, that the hard X-ray source may consist of a distribution of many small impulsively-heated kernels, each cooled by anomalous conduction, with lifetimes shorter than current burst data temporal resolution. In this case the dynamic spectra of bursts are governed by the dynamic evolution of the kernel production process, such as magnetic-field dissipation in the tearing mode. An integral equation is formulated, the solution of which yields information on this kernel production process, from dynamic burst spectra, for any kernel model.
With a BMS-type kernel model in one-dimensional form, the derived instantaneous spectra are limited in hardness to spectral indices γ ≳ 4 for any kernel production process, due to the nature of the conductive cooling. Ion-acoustic conductive cooling in three dimensions, however, increases the limiting spectral hardness to γ ≳ 3. Other forms of anomalous conduction yield similar results but could permit bursts as hard as γ ≳ 2, consistent with the hardest observed.
The contribution to the X-ray spectrum from the escaping tail of high-energy kernel electrons in the BMS model is calculated in various limits. If this tail dissipates purely collisionally, for example, its thick-target bremsstrahlung can significantly modify the kernel spectrum at the high-energy end. The energetics of this dynamic dissipation model for thermal hard X-ray bursts also are briefly discussed.
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Now at: Department of Mathematics, University of Waikato, Hamilton, New Zealand.
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Brown, J.C., Craig, I.J.D. & Karpen, J.T. Dynamic spectral characteristics of thermal models for solar hard X-ray bursts. Sol Phys 67, 143–162 (1980). https://doi.org/10.1007/BF00146690
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DOI: https://doi.org/10.1007/BF00146690