Atmospheric albedo contributes 10% to 100% of GRM effective area depending on Earth orientation and GRB angle, with dominance at 8-20 keV when direct response vanishes, requiring inclusion in calibration.
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Study on the detector energy response of SVOM/GRM
Atmospheric albedo contributes 10% to 100% of GRM effective area depending on Earth orientation and GRB angle, with dominance at 8-20 keV when direct response vanishes, requiring inclusion in calibration.