Thin target γ-ray line production during the 1991 June 1 flare

Details Thin target γ-ray line production during the 1991 June 1 flare Thin target γ-ray line production during the 1991 June 1 flare

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..374..153t&link_type=abstract

High energy solar physics. AIP Conference Proceedings, Volume 374, pp. 153-161 (1996).

Physics

8

Solar Electromagnetic Emission

Scientific paper

We present a time dependent analysis of the γ-ray line spectra recorded by the PHEBUS instrument on board GRANAT during the 1991 June 1 flare. For each studied spectrum we determine the electron bremsstrahlung continuum and the γ-ray line fluences Φ1.1-1.8 and φ4.1-7.6, in the 1.1-1.8 MeV and 4.1-7.6 MeV bands respectively, as well as their ratio R=φ1.1-1.8/φ4.1-7.6. We find that the power law index of the bremsstrahlung continuum in the 0.6-10 MeV band is 2.6+/-0.1 and that it remains constant with time. The characteristic value of R, estimated for the spectrum accumulated over the whole event duration is about 4 but, surprisingly, R increases from a value of ~3 to a value of ~7 during the decay phase of the event. In order to interpret these findings we have compared the measured values of R with those obtained by using calculations of deexcitation γ-ray line spectra performed for different interacting particle spectra and compositions. We show that the high value of R and its large variation with time are inconsistent with a thick target γ-ray line source and that a thin target model is the appropriate one. This is consistent with an earlier study of the 1991 June 1 event which indicates that the observed nuclear line emission is produced in a coronal source. We finally argue that the increase of R with time strongly suggests an impulsive flare composition for the accelerated particles and the further enrichment of the heavy nuclei abundances as the flare progresses. For thin target interactions such an enrichment is most probably due to the acceleration process itself.

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