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Modelling the interaction of the Astro Bio Cube Sat with the Van Allen’s Belt radiative field using Monte Carlo transport codes
Purpose The AstroBio Cube Satellite (ABCS) will deploy within the inner Van Allen belt on the Vega C Maiden Flight launch opportunity of the European Space Agency. At this altitude, ABCS will experience radiation doses orders of magnitude greater than in low earth orbit, where CubeSats usually opera...
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Published in: | Radiation detection technology and methods 2022-06, Vol.6 (2), p.262-279 |
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creator | Burgio, N. Cretara, L. Corcione, M. Frullini, M. Iannascoli, L. Nascetti, A. Santagata, A. Palmerini, G. Quintino, A. Brucato, J. R. Meneghin, A. Paglialunga, D. |
description | Purpose
The AstroBio Cube Satellite (ABCS) will deploy within the inner Van Allen belt on the Vega C Maiden Flight launch opportunity of the European Space Agency. At this altitude, ABCS will experience radiation doses orders of magnitude greater than in low earth orbit, where CubeSats usually operate. The paper aims to estimate the irradiation effect on the ABCS payload in the orbital condition, their possible mitigation designing shielding solutions and performs a preliminary representativity simulation study on the ABCS irradiation with fission neutron at the TAPIRO (TAratura Pila Rapida Potenza 0) nuclear research reactor facility at ENEA.
Methods
We quantify the contributions of geomagnetically trapped particles (electron and proton), Galactic Cosmic Rays (GCR ions), Solar energetic particle within the ABCS orbit using the ESA’s SPace ENVironment information system. FLUKA (Fluktuierende Kaskade—Fluctuating Cascade) code models the ABCS interaction with the orbital source.
Results
We found a shielding solution of the weight of 300 g constituted by subsequent layers of tungsten, resins, and aluminium that decreases on average the 20% overall dose rate relative to the shielding offered by the only satellite’s structure. Finally, simulations of neutron irradiation of the whole ABCS structure within the TAPIRO’s thermal column cavity show that a relatively short irradiation time is requested to reach the same level of 1 MeV neutron Silicon equivalent damage of the orbital source.
Conclusions
The finding deserves the planning of a future experimental approach to confirm the TAPIRO’s performance and establish an irradiation protocol for testing aerospatial electronic components. |
doi_str_mv | 10.1007/s41605-022-00321-9 |
format | article |
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The AstroBio Cube Satellite (ABCS) will deploy within the inner Van Allen belt on the Vega C Maiden Flight launch opportunity of the European Space Agency. At this altitude, ABCS will experience radiation doses orders of magnitude greater than in low earth orbit, where CubeSats usually operate. The paper aims to estimate the irradiation effect on the ABCS payload in the orbital condition, their possible mitigation designing shielding solutions and performs a preliminary representativity simulation study on the ABCS irradiation with fission neutron at the TAPIRO (TAratura Pila Rapida Potenza 0) nuclear research reactor facility at ENEA.
Methods
We quantify the contributions of geomagnetically trapped particles (electron and proton), Galactic Cosmic Rays (GCR ions), Solar energetic particle within the ABCS orbit using the ESA’s SPace ENVironment information system. FLUKA (Fluktuierende Kaskade—Fluctuating Cascade) code models the ABCS interaction with the orbital source.
Results
We found a shielding solution of the weight of 300 g constituted by subsequent layers of tungsten, resins, and aluminium that decreases on average the 20% overall dose rate relative to the shielding offered by the only satellite’s structure. Finally, simulations of neutron irradiation of the whole ABCS structure within the TAPIRO’s thermal column cavity show that a relatively short irradiation time is requested to reach the same level of 1 MeV neutron Silicon equivalent damage of the orbital source.
Conclusions
The finding deserves the planning of a future experimental approach to confirm the TAPIRO’s performance and establish an irradiation protocol for testing aerospatial electronic components.</description><identifier>ISSN: 2509-9930</identifier><identifier>EISSN: 2509-9949</identifier><identifier>DOI: 10.1007/s41605-022-00321-9</identifier><language>eng</language><publisher>Singapore: Springer Nature Singapore</publisher><subject>Beam Physics ; Hadrons ; Heavy Ions ; Nuclear Energy ; Nuclear Physics ; Original Paper ; Particle Acceleration and Detection ; Physics ; Physics and Astronomy</subject><ispartof>Radiation detection technology and methods, 2022-06, Vol.6 (2), p.262-279</ispartof><rights>The Author(s) 2022</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c335t-4c531f76dc235eabedd6b735a58b1ef63e5f3b36e99140983860e770b6b6d76e3</citedby><cites>FETCH-LOGICAL-c335t-4c531f76dc235eabedd6b735a58b1ef63e5f3b36e99140983860e770b6b6d76e3</cites><orcidid>0000-0001-8982-2593 ; 0000-0002-4738-5521 ; 0000-0002-9721-0690 ; 0000-0002-7471-2858 ; 0000-0003-4678-0068 ; 0000-0003-1665-6664 ; 0000-0001-8976-8750 ; 0000-0002-6113-6898 ; 0000-0003-1275-323X ; 0000-0001-8138-7494 ; 0000-0002-2356-914X ; 0000-0003-4099-7506</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27903,27904</link.rule.ids></links><search><creatorcontrib>Burgio, N.</creatorcontrib><creatorcontrib>Cretara, L.</creatorcontrib><creatorcontrib>Corcione, M.</creatorcontrib><creatorcontrib>Frullini, M.</creatorcontrib><creatorcontrib>Iannascoli, L.</creatorcontrib><creatorcontrib>Nascetti, A.</creatorcontrib><creatorcontrib>Santagata, A.</creatorcontrib><creatorcontrib>Palmerini, G.</creatorcontrib><creatorcontrib>Quintino, A.</creatorcontrib><creatorcontrib>Brucato, J. R.</creatorcontrib><creatorcontrib>Meneghin, A.</creatorcontrib><creatorcontrib>Paglialunga, D.</creatorcontrib><title>Modelling the interaction of the Astro Bio Cube Sat with the Van Allen’s Belt radiative field using Monte Carlo transport codes</title><title>Radiation detection technology and methods</title><addtitle>Radiat Detect Technol Methods</addtitle><description>Purpose
The AstroBio Cube Satellite (ABCS) will deploy within the inner Van Allen belt on the Vega C Maiden Flight launch opportunity of the European Space Agency. At this altitude, ABCS will experience radiation doses orders of magnitude greater than in low earth orbit, where CubeSats usually operate. The paper aims to estimate the irradiation effect on the ABCS payload in the orbital condition, their possible mitigation designing shielding solutions and performs a preliminary representativity simulation study on the ABCS irradiation with fission neutron at the TAPIRO (TAratura Pila Rapida Potenza 0) nuclear research reactor facility at ENEA.
Methods
We quantify the contributions of geomagnetically trapped particles (electron and proton), Galactic Cosmic Rays (GCR ions), Solar energetic particle within the ABCS orbit using the ESA’s SPace ENVironment information system. FLUKA (Fluktuierende Kaskade—Fluctuating Cascade) code models the ABCS interaction with the orbital source.
Results
We found a shielding solution of the weight of 300 g constituted by subsequent layers of tungsten, resins, and aluminium that decreases on average the 20% overall dose rate relative to the shielding offered by the only satellite’s structure. Finally, simulations of neutron irradiation of the whole ABCS structure within the TAPIRO’s thermal column cavity show that a relatively short irradiation time is requested to reach the same level of 1 MeV neutron Silicon equivalent damage of the orbital source.
Conclusions
The finding deserves the planning of a future experimental approach to confirm the TAPIRO’s performance and establish an irradiation protocol for testing aerospatial electronic components.</description><subject>Beam Physics</subject><subject>Hadrons</subject><subject>Heavy Ions</subject><subject>Nuclear Energy</subject><subject>Nuclear Physics</subject><subject>Original Paper</subject><subject>Particle Acceleration and Detection</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><issn>2509-9930</issn><issn>2509-9949</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNp9kE1OwzAQhSMEElXpBVj5AoFJHNvxso34k1qx4GdrOcmkdWXiynZB7OAYXI-TkLaIJasZzcx7b_QlyXkGFxmAuAxFxoGlkOcpAM2zVB4lo5yBTKUs5PFfT-E0mYSwBoBc0KIEMUo-F65Fa02_JHGFxPQRvW6icT1x3X40DdE7MjOOVNsayYOO5M3E1X73rHsytRb774-vQGZoI_G6NTqaVySdQduSbdh5L9xgTCrtrSPR6z5snI-kGbLDWXLSaRtw8lvHydP11WN1m87vb-6q6TxtKGUxLRpGs07wtskpQ11j2_JaUKZZWWfYcYqsozXlKGVWgCxpyQGFgJrXvBUc6TjJD76NdyF47NTGmxft31UGasdRHTiqgaPac1RyENGDKAzH_RK9Wrut74c__1P9AHW-d8k</recordid><startdate>20220601</startdate><enddate>20220601</enddate><creator>Burgio, N.</creator><creator>Cretara, L.</creator><creator>Corcione, M.</creator><creator>Frullini, M.</creator><creator>Iannascoli, L.</creator><creator>Nascetti, A.</creator><creator>Santagata, A.</creator><creator>Palmerini, G.</creator><creator>Quintino, A.</creator><creator>Brucato, J. R.</creator><creator>Meneghin, A.</creator><creator>Paglialunga, D.</creator><general>Springer Nature Singapore</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0001-8982-2593</orcidid><orcidid>https://orcid.org/0000-0002-4738-5521</orcidid><orcidid>https://orcid.org/0000-0002-9721-0690</orcidid><orcidid>https://orcid.org/0000-0002-7471-2858</orcidid><orcidid>https://orcid.org/0000-0003-4678-0068</orcidid><orcidid>https://orcid.org/0000-0003-1665-6664</orcidid><orcidid>https://orcid.org/0000-0001-8976-8750</orcidid><orcidid>https://orcid.org/0000-0002-6113-6898</orcidid><orcidid>https://orcid.org/0000-0003-1275-323X</orcidid><orcidid>https://orcid.org/0000-0001-8138-7494</orcidid><orcidid>https://orcid.org/0000-0002-2356-914X</orcidid><orcidid>https://orcid.org/0000-0003-4099-7506</orcidid></search><sort><creationdate>20220601</creationdate><title>Modelling the interaction of the Astro Bio Cube Sat with the Van Allen’s Belt radiative field using Monte Carlo transport codes</title><author>Burgio, N. ; Cretara, L. ; Corcione, M. ; Frullini, M. ; Iannascoli, L. ; Nascetti, A. ; Santagata, A. ; Palmerini, G. ; Quintino, A. ; Brucato, J. R. ; Meneghin, A. ; Paglialunga, D.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c335t-4c531f76dc235eabedd6b735a58b1ef63e5f3b36e99140983860e770b6b6d76e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Beam Physics</topic><topic>Hadrons</topic><topic>Heavy Ions</topic><topic>Nuclear Energy</topic><topic>Nuclear Physics</topic><topic>Original Paper</topic><topic>Particle Acceleration and Detection</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Burgio, N.</creatorcontrib><creatorcontrib>Cretara, L.</creatorcontrib><creatorcontrib>Corcione, M.</creatorcontrib><creatorcontrib>Frullini, M.</creatorcontrib><creatorcontrib>Iannascoli, L.</creatorcontrib><creatorcontrib>Nascetti, A.</creatorcontrib><creatorcontrib>Santagata, A.</creatorcontrib><creatorcontrib>Palmerini, G.</creatorcontrib><creatorcontrib>Quintino, A.</creatorcontrib><creatorcontrib>Brucato, J. R.</creatorcontrib><creatorcontrib>Meneghin, A.</creatorcontrib><creatorcontrib>Paglialunga, D.</creatorcontrib><collection>Springer Nature OA Free Journals</collection><collection>CrossRef</collection><jtitle>Radiation detection technology and methods</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Burgio, N.</au><au>Cretara, L.</au><au>Corcione, M.</au><au>Frullini, M.</au><au>Iannascoli, L.</au><au>Nascetti, A.</au><au>Santagata, A.</au><au>Palmerini, G.</au><au>Quintino, A.</au><au>Brucato, J. R.</au><au>Meneghin, A.</au><au>Paglialunga, D.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Modelling the interaction of the Astro Bio Cube Sat with the Van Allen’s Belt radiative field using Monte Carlo transport codes</atitle><jtitle>Radiation detection technology and methods</jtitle><stitle>Radiat Detect Technol Methods</stitle><date>2022-06-01</date><risdate>2022</risdate><volume>6</volume><issue>2</issue><spage>262</spage><epage>279</epage><pages>262-279</pages><issn>2509-9930</issn><eissn>2509-9949</eissn><abstract>Purpose
The AstroBio Cube Satellite (ABCS) will deploy within the inner Van Allen belt on the Vega C Maiden Flight launch opportunity of the European Space Agency. At this altitude, ABCS will experience radiation doses orders of magnitude greater than in low earth orbit, where CubeSats usually operate. The paper aims to estimate the irradiation effect on the ABCS payload in the orbital condition, their possible mitigation designing shielding solutions and performs a preliminary representativity simulation study on the ABCS irradiation with fission neutron at the TAPIRO (TAratura Pila Rapida Potenza 0) nuclear research reactor facility at ENEA.
Methods
We quantify the contributions of geomagnetically trapped particles (electron and proton), Galactic Cosmic Rays (GCR ions), Solar energetic particle within the ABCS orbit using the ESA’s SPace ENVironment information system. FLUKA (Fluktuierende Kaskade—Fluctuating Cascade) code models the ABCS interaction with the orbital source.
Results
We found a shielding solution of the weight of 300 g constituted by subsequent layers of tungsten, resins, and aluminium that decreases on average the 20% overall dose rate relative to the shielding offered by the only satellite’s structure. Finally, simulations of neutron irradiation of the whole ABCS structure within the TAPIRO’s thermal column cavity show that a relatively short irradiation time is requested to reach the same level of 1 MeV neutron Silicon equivalent damage of the orbital source.
Conclusions
The finding deserves the planning of a future experimental approach to confirm the TAPIRO’s performance and establish an irradiation protocol for testing aerospatial electronic components.</abstract><cop>Singapore</cop><pub>Springer Nature Singapore</pub><doi>10.1007/s41605-022-00321-9</doi><tpages>18</tpages><orcidid>https://orcid.org/0000-0001-8982-2593</orcidid><orcidid>https://orcid.org/0000-0002-4738-5521</orcidid><orcidid>https://orcid.org/0000-0002-9721-0690</orcidid><orcidid>https://orcid.org/0000-0002-7471-2858</orcidid><orcidid>https://orcid.org/0000-0003-4678-0068</orcidid><orcidid>https://orcid.org/0000-0003-1665-6664</orcidid><orcidid>https://orcid.org/0000-0001-8976-8750</orcidid><orcidid>https://orcid.org/0000-0002-6113-6898</orcidid><orcidid>https://orcid.org/0000-0003-1275-323X</orcidid><orcidid>https://orcid.org/0000-0001-8138-7494</orcidid><orcidid>https://orcid.org/0000-0002-2356-914X</orcidid><orcidid>https://orcid.org/0000-0003-4099-7506</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Beam Physics Hadrons Heavy Ions Nuclear Energy Nuclear Physics Original Paper Particle Acceleration and Detection Physics Physics and Astronomy |
title | Modelling the interaction of the Astro Bio Cube Sat with the Van Allen’s Belt radiative field using Monte Carlo transport codes |
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