2022
Geant4 simulation of the residual background in the ATHENA wide field imager from protons deflected by the charged particle diverter
GALGÓCZI, Gábor; Jean-Paul Bernhard RIFFALD SOUZA BREUER; Valentina FIORETTI; Jakub ZLÁMAL; Norbert WERNER et al.Základní údaje
Originální název
Geant4 simulation of the residual background in the ATHENA wide field imager from protons deflected by the charged particle diverter
Autoři
GALGÓCZI, Gábor; Jean-Paul Bernhard RIFFALD SOUZA BREUER; Valentina FIORETTI; Jakub ZLÁMAL; Norbert WERNER; Vojtěch ČALKOVSKÝ; Nathalie BOUDIN; Ivo FERREIRA; Matteo GUAINAZZI; Andreas VON KIENLIN; Simone LOTTI; Teresa MINEO; Silvano MOLENDI a Emanuele PERINATI
Vydání
Washington, Proceedings of SPIE, Volume 12181: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray, od s. 1-9, 9 s. 2022
Nakladatel
SPIE
Další údaje
Jazyk
angličtina
Typ výsledku
Stať ve sborníku
Obor
10308 Astronomy
Stát vydavatele
Spojené státy
Utajení
není předmětem státního či obchodního tajemství
Forma vydání
elektronická verze "online"
Označené pro přenos do RIV
Ano
Kód RIV
RIV/00216224:14310/22:00127120
Organizační jednotka
Přírodovědecká fakulta
ISBN
978-1-5106-5343-6
ISSN
UT WoS
EID Scopus
Klíčová slova anglicky
ATHENA; X-ray; soft proton scattering; Geant4; residual background
Příznaky
Mezinárodní význam, Recenzováno
Změněno: 19. 1. 2023 16:43, Mgr. Marie Novosadová Šípková, DiS.
Anotace
V originále
X-ray telescopes opened up a new window into the high-energy universe. However, the last generation of these telescopes encountered an unexpected problem: their optics focused not only x-rays but low-energy (so called soft) protons as well. These protons are very hard to model and can not be distinguished from x-rays. For example, 40% of XMM-Newton observations is significantly contaminated by soft proton induced background flares. In order to minimize the background from such low-energy protons the advanced telescope for high energy astrophysics (ATHENA) satellite introduced a novel concept, the so called charged particle diverter (CPD). It is an array of magnets in a Hallbach design, which deflects protons below 76 keV before they would hit the wide field imager (WFI) detector. In this work, we investigate the effect of scattering of the deflected protons with the CPD walls and the inner surfaces of the WFI detector assembly. Such scattered protons can loose energy, change direction and still hit the WFI. In order to adopt the most realistic instrument model, we imported the CAD model of both the CPD and the WFI focal plane assembly. Soft protons corresponding to ≈2.5 hours of exposure to the L1 solar wind are simulated in this work. The inhomogeneous magnetic field of the CPD is included in the simulation. We present a preliminary estimate of the WFI residual background induced by soft proton secondary scattering, in the case of the optical blocking filter present in the field of view. A first investigation of the volumes responsible for scattering the protons back into the field of view is reported.
Návaznosti
| EF19_073/0016943, projekt VaV |
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| GX21-13491X, projekt VaV |
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| MUNI/I/0003/2020, interní kód MU |
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