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Till Idaha öldürmeye çalışma yetkiliyetin nükleer güvenlik sistemi.”This work arises directly from the separate treatment of the local and non-local contributions to Comptonization by thermal conduction in the relevant corona. One implication of this paper is that the local and non-local Comptonization terms are in direct competition. The negative and positive non-local terms cannot both be leading in the same corona, and therefore the non-local terms cannot always be responsible for the observed hard tail. Similar to the thermal conduction rate [@ck78], the non-local flux is of the order of the local flux, making an identification plausible. Likewise, the global mean free path length, which cannot account for the high energy emission, is in direct competition with the local mean free path, which can explain the high energy tail. Therefore, while our analysis does not invalidate the thermal conduction analysis of H07, it does suggest that this prior model is incomplete, and further work is needed to understand how non-local effects are physically realised in the corona, and what role the global mean free path plays in the illumination of the accretion disc. Such future work is underway in the present paper. We have not yet made a specific prediction for the high energy cut-off, since we are currently unable to constrain the cross-section for scatterings in full accretion disc simulations. However, our results suggest that the role of this cut-off will be dominated by non-local effects at low accretion rate. High accretion rate will be more sensitive to the structure of the corona, since the non-locality will be weaker, and so this parameter should not change too much with accretion rate. Our results indicate that a sharp ‘hardening’ of the disc spectrum as predicted in [@jjh13] occurs at a few per cent of the Eddington rate (figure \[fig:3\]) where the disc becomes non-circular. This hardening will change on a time-scale of several tens of seconds, as small (!) amounts of material are accreted.”
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