11 th Geant 4 Space Users Workshop Hiroshima

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11 th Geant 4 Space User’s Workshop Hiroshima, 26 -28 Aug 2015 Geant 4

11 th Geant 4 Space User’s Workshop Hiroshima, 26 -28 Aug 2015 Geant 4 at INTA Status Report - 2015 S. Ibarmia, P. Gallego, C. Martínez

Areas where Geant 4 is applied Since 2004 the INTA Space Environments & Effects

Areas where Geant 4 is applied Since 2004 the INTA Space Environments & Effects group has worked to include Geant 4 as base radiation simulation analysis tool. As a result , Geant 4 is currently supporting activities in the following areas: Space radiation engineering ð At S/C level § § Shielding analysis, radiation level spec. TID, DDD, fluxes, background noise, etc, ð At instrument/payload level § § § Supporting design optimization Shielding & effects estimation Radiation sensor calibration and design Qualification of EEE components irradiation ð Irradiation simulation. Dosimetry estimation ð Effective damage at sub-component level R&D ð Participation in ESA funded R&D specific activities related Geant 4 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

Geant 4 supported projects ESA Programs ð ð ð Solar Orbiter – PHI instrument

Geant 4 supported projects ESA Programs ð ð ð Solar Orbiter – PHI instrument Bepi. Colombo – MIXS instrument (ended) Exo. Mars – RLS instrument Plato (new) Athena (new) AIM / COPINS (new) National Nano/Micro missions ð Nanosat-1 B ð OPTOS ð Xat. Cobeo (ended) & Humsat-D ð Nanosat-2, Micro. Sat (planned) Other R&D ð ESA ITT -> CIRSOS 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

ESA Solar Orbiter - PHI Polarimetric & Helioseismic Imager Development of a polarimetric telescope

ESA Solar Orbiter - PHI Polarimetric & Helioseismic Imager Development of a polarimetric telescope to study helioseismicity ð Heritage from IMAX/Sun. Rise ð Launch foreseen for 2018+ ð State-of-the-art technologies § Li. NBO 3 etalons to banpass (m. Ang) solar Fe. I line (6173 ang) Geant 4 activities ð Space engineering. Full S/C simulation § § Full CAD to Geant 4 modeling Radiation levels for all PHI components ð Support: simulation of p+ & HI test CAD Designs GEANT 4 Models (CDR) § § Li. Nb. O 3 Etalons (5000 V, roughness <20 nm ) Dose profiling for all optical elements 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

ESA Bepi. Colombo - MIXS Mercury Imager X-ray Spectrometer INTA is resposible of the

ESA Bepi. Colombo - MIXS Mercury Imager X-ray Spectrometer INTA is resposible of the development of MIXS Focal Plane and E-Box ð Status: FM completed and delivered to ESA Geant 4 activities Bepi. Colombo MPO G 4 Model ð Space engineering. Full S/C simulation § § Shielding analysis Radiation levels for INTA MIXS components ð X-ray simulation § § § MIXS FM MIXS G 4 Model Calibration sources Mercury X-ray fluorescence X-ray focusing (optics grating MCP ) ð Simulation of the electron diverter (@optics) 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

ESA Exomars 2018 - RLS Raman Laser Spectrometer INTA is responsible of the development

ESA Exomars 2018 - RLS Raman Laser Spectrometer INTA is responsible of the development of the entire instrument ð Launch foreseen for 2018+ ð Chemical composition analyser based on laserinduced raman spectroscopy Geant 4 activity ð Space engineering. Instrument simulation § § § Shielding analysis Radiation levels at RLS components Proton & RHU propagation for RLS components ð Irradiation test simulation § Proton and HI tests: Lasers, diffracction gratings and optical lens 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

ESA PLATO Optical telescope array Detection of terrestrial exoplanets in the habitable zone of

ESA PLATO Optical telescope array Detection of terrestrial exoplanets in the habitable zone of solar-type stars INTA is responsible of the development of all the telescopes FPA ð Launch foreseen for 2024 Geant 4 activity ð Phase A/B: § § § Worst-case shielding analysis Radiation levels at critical components Main concern at this stage: Principal CCDs sensitive to TID ~5 krad!! Weight budget on its limit for extra shielding PLATO Telescope Geant 4 Model 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

ESA ATHENA Next generation X-ray observatory ð Mapping hot gas structures and determining their

ESA ATHENA Next generation X-ray observatory ð Mapping hot gas structures and determining their physical properties ð Searching for supermassive black holes ð INTA will be probably responsible of part of the FPA assembly and cryogenics system ð Launch foreseen for 2028 – Halo orbit L 2 Geant 4 activities ð TBD. Contracts under bidding process ð Challenges for Geant 4: § § § Simulation of background effects. Activation Focusing of unwanted low-energy particles Simulation of Silicon Pore Optics ð Much to learn from Astro-H Geant 4 work 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

ESA AIM / COPINS AIM: Asteroid Impact Mission ð Part of the Asteroid Impact

ESA AIM / COPINS AIM: Asteroid Impact Mission ð Part of the Asteroid Impact & Deflection Assessment mission (AIDA). ð Launch foreseen for 2020 ð Study the Didymos binary asteroid system ð INTA has been selected fot a feasibility study – COPINS (Cube. Sat Opportunity Payloads) § Responsible for two Cube. SATs Geant 4 activities ð TBD. Overall radiation level and shielding assessments 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

INTA Nanosat-1 B Nanosat 1 B mission ð Second sattelite of the nanosat series

INTA Nanosat-1 B Nanosat 1 B mission ð Second sattelite of the nanosat series ð Launched in summer 2009, sun-synchronous, 600 km ð Radiation payloads § LDT (results to be published) § § Geant 4 model of NS 1 B (80 -85% mass, 100’s vols, high fidelity) § A photodiode-based TNID sensor (Dark current) Particle flux measurements (Photocurrent) High sensitivity Rad. FET TID sensors § § § Direct readout data ~150 rad/year Compensated with annealing ~200 rad/year Geant 4 + NS 1 B Model ~240 ± 20 rad/year Geant 4 activities ð Space engineering. § § Shielding analysis Radiation levels at EEE, OWLS, LDT and Rad. FETs ð Simulation of LDT calibration tests under proton (PSI) Location of LDT and Rad. FET 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

INTA Nanosat-1 B Simulation of LDT calibration campaigns LDT Developed by INTA Optoelectronics Lab

INTA Nanosat-1 B Simulation of LDT calibration campaigns LDT Developed by INTA Optoelectronics Lab Measurement results vs. Simulation under publication and Ph. D thesis Geant 4 model, 70 Me. V proton irradiation and energy thresholds for <DT detectors. 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

OPTOS, Xat. Cobeo, Hum. SAT-D OPTOS ð 3 U Cube. SAT – Technological demonstrator

OPTOS, Xat. Cobeo, Hum. SAT-D OPTOS ð 3 U Cube. SAT – Technological demonstrator ð Launched on November 2013 ð Radiation payloads: High sensitivity Rad. FET sensor Xat. Cobeo mission ð 3 U Cube. SAT – University of Vigo & INTA ð Launched on Feb 2012 (VEGA maiden flight) ð Radiation payloads: High sensitivity TNID sensor Hum. SAT-D mission ð Evolution of Xat. Cobeo. Same 1 U platform ð Launched on November 2013 ð Radiation payloads: High sensitivity TNID sensor ð S/C full Geant 4 modeling for shielding analysis & radiation levels estimation Geant 4 activity ð Validation of environment models, margins analysis ð Results under final publication process! 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

R&D: CIRSOS Collaborative Iterative Radiation Shielding Optimisation System (CIRSOS) The CIRSOS system is an

R&D: CIRSOS Collaborative Iterative Radiation Shielding Optimisation System (CIRSOS) The CIRSOS system is an ESA funded R&D project aimed to develop a full radiation simulation framework, in order to help S/C and P/L engineers, through a SW system that: ð Efficiently supports collaborative and iterative radiation analyses ð Provides interfaces with industrial radiation design tools ð Allows end-to-end radiation simulation, starting from the definition of the high energy particle environment, performing particle propagation through complex 3 D geometrical models (via Geant 4) and ending with deep dielectric charging effects modelling (via SPIS) Se e Fr id ay ta lk !! Some of the most relevant advantages of CIRSOS for the radiation community include: § § § § A user-friendly GUI to manage the entire system A database controlled geometry managing. Material properties built-in databases High-energy radiation and charging simulation capabilities (independent or coupled) Parametric Geant 4 analyses Interface to SPENVIS, OMERE, FASTRAD and ESABASE 2 Parallel simulation on multiple host / multiple processor Built-in post-processing tools, bilt-in geometry visualization tools 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015

Summary & Future Summary ð INTA is applying Geant 4 as standard radiation tool

Summary & Future Summary ð INTA is applying Geant 4 as standard radiation tool § Many different programs supported § Establishing G 4 as the standard methodology for radiation analysis ð Main scenarios of successful application § Engineering support to ESA instruments § Engineering support to INTA missions § Payload design and calibration of radiation sensors § Other Geant 4 R&D focused on the improvement and/or development of new engineering tools 11 th Geant 4 Space Users’ Workshop Hiroshima, 26 -28 Aug 2015