Informace o publikaci

Instrument response generation using high-resolution 3D voxilization of GRBAlpha and VZLUSAT-2 satellites with MEGAlib

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BREUER Jean-Paul YOKOTA Masato FUKAZAWA Yasushi TAKAHASHI Hiromitsu WERNER Norbert ŘÍPA Jakub DAFČÍKOVÁ Marianna MÜNZ Filip OHNO Masanori CSÁK Balázs MÉSZÁROS László PÁL András FRAJT Marcel HUDEC Jan KAPUŠ Jakub REZENOV Maksim DÁNIEL Vladimír DUDÁŠ Juraj SVOBODA Petr CHANG Hsiang-Kuang CHANG Hao-Min HU Chin-Ping LIN Chih-Hsun LIU Tsung-Che SEN Kaustubha TSAO Che-Chih WU Chih-En

Rok publikování 2026
Druh Stať ve sborníku
Konference Proc. SPIE 14146, Space Telescopes and Instrumentation 2026: Ultraviolet to Gamma Ray
Fakulta / Pracoviště MU

Přírodovědecká fakulta

Citace
www https://www.spiedigitallibrary.org/conference-proceedings-of-spie/14146/3102333/Instrument-response-generation-using-high-resolution-3D-voxilization-of-GRBAlpha/10.1117/12.3102333.full
Doi https://doi.org/10.1117/12.3102333
Klíčová slova Instrument response; MEGAlib; Cubesats; Gamma-ray bursts; GRBAlpha; VZLUSAT-2; CAD; Voxelization
Popis Pathfinder gamma-ray burst (GRB) detecting CubeSat missions such as GRBAlpha and VZLUSAT-2 have demonstrated the successful application of scintillator detectors with silicon photomultipliers in low Earth orbit (LEO). To produce more comprehensive scientific analysis of the data, the effective area of the detector needs to be characterised at different energies. A large part of this process requires a thorough understanding of the detectors response matrices as a function of the satellite mass model typically performed through Geant4 and MEGAlib simulations. We use a novel voxelization and binning methodology to turn complex 3D geometries into MEGAlib-compatible versions, and we validate these experiments by showing that the simulation results with Geant4 agree within an order of 10%. We use MEGAlib simulations from various angles around the spacecraft to generate instrumental response matrices for both simple and complex geometries, in the case of GRBAlpha and VZLUSAT-2, respectively.
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