НОВИЙ ПІДХІД ДО РЕКОНСТРУКЦІЇ ЗОБРАЖЕНЬ У РЕНТГЕНІВСЬКОМУ ТА ГАММА-ДОМЕНАХ

This study examines the consequences of high-energy radiation interactions from X-ray sources with extended astrophysical objects. A comparative analysis is conducted between the spectra of primary radiation sources and those of irradiated absorbing and scattering regions. The limitations of current diagnostic methods are identified, and strategies for enhancing both the sensitivity and informational value of the resulting data are proposed. Signal-to-noise ratios are derived for a gamma-ray detector prototype developed by the authors, under various geometric configurations of emitting and scattering structures. Necessary modifications to the radiation transport equations are suggested, along with instrumental techniques for identifying and registering previously unrecognized astrophysical entities.