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. Geant4 simulation of the residual background in the ATHENA wide field imager from protons deflected by the charged particle diverter. Online. In Jan-Willem A. den Herder, Shouleh Nikzad, Kazuhiro Nakazawa. Proceedings of SPIE, Volume 12181: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray. Washington: SPIE, 2022, s. 1-9. ISBN 978-1-5106-5343-6. Dostupné z: https://dx.doi.org/10.1117/12.2629994.
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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 (348 Maďarsko, domácí), Jean-Paul Bernhard RIFFALD SOUZA BREUER (76 Brazílie, domácí), Valentina FIORETTI, Jakub ZLÁMAL, Norbert WERNER (703 Slovensko, domácí), 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
Originální 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"
WWW URL URL
Kód RIV RIV/00216224:14310/22:00127120
Organizační jednotka Přírodovědecká fakulta
ISBN 978-1-5106-5343-6
ISSN 0277-786X
Doi http://dx.doi.org/10.1117/12.2629994
UT WoS 000865607100098
Klíčová slova anglicky ATHENA; X-ray; soft proton scattering; Geant4; residual background
Štítky rivok
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnila: Mgr. Marie Šípková, DiS., učo 437722. Změněno: 19. 1. 2023 16:43.
Anotace
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 VaVNázev: Interní grantová agentura Masarykovy univerzity
GX21-13491X, projekt VaVNázev: Zkoumání žhavého vesmíru a porozumění kosmické zpětné vazbě (Akronym: EHU)
Investor: Grantová agentura ČR, Exploring the Hot Universe and Understanding Comic Feedback
MUNI/I/0003/2020, interní kód MUNázev: MUNI Award in Science and Humanities 3 (Akronym: Space-Based High-Energy Astrophysics)
Investor: Masarykova univerzita, MUNI Award in Science and Humanities 3, MASH - MUNI Award in Science and Humanities
VytisknoutZobrazeno: 27. 5. 2024 17:48