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Overview of the main radiation transport codes

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dc.contributor.authorSchetakis, Nikolaos
dc.contributor.authorCrespo, Rodrigo
dc.contributor.authorLuis Vazquez-Poletti, Jose
dc.contributor.authorSastre Marugán, Mariano
dc.contributor.authorVazquez, Luis
dc.contributor.authorDi Iorio, Alessio
dc.date.accessioned2023-06-17T08:56:04Z
dc.date.available2023-06-17T08:56:04Z
dc.date.issued2020-10-27
dc.description© Author(s). This research has been carried out in the framework of the IN-TIME project, which is funded by the European Commission under the Horizon 2020 Marie Skłodowska-Curie actions Research and Innovation Staff Exchange (RISE; grant agreement no. 823934). The authors are thankful to the institutions and individual members who participated in the project. Through other research projects, the Spanish Government (Ministerio de Economía, Industria y Competitividad and Ministerio de Ciencia e Innovación) additionally supported Luis Vázquez (ESP2016-79135-R), Mariano Sastre (PCIN-2014-013-C07-04, PCIN-2016-080, CGL2016-78702- C2-2-R and PID2019-105306RB-I00) and JLVP (RTI2018-096465- B-I00, EDGECLOUD). José Luis Vázquez-Poletti was also supported by the Madrid Regional Government (project EDGEDATA, S2018/TCS-4499). We would like to thank the associate editor and two anonymous reviewers for their thoughtful comments and efforts towards improving our paper.
dc.description.abstractAccurate predictions of expected radiation dose levels on Mars are often provided by specific radiation transport codes that have been adapted to space conditions. Unsurprisingly, several of the main space agencies and institutions involved in space research and technology tend to work with their own in-house radiation codes. We present the codes that are related to the simulation of the radiation on Mars' surface under different scenarios. All of these codes have similar fields of application, but they differ with respect to several aspects, including the energy range and types of projectiles considered as well as the models of nuclear reactions considered.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUnión Europea. Horizonte 2020
dc.description.sponsorshipMinisterio de Economía y Competitividad (MINECO)/Ministerio de Ciencia e Innovación (MICCIN)
dc.description.sponsorshipComunidad de Madrid
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/63255
dc.identifier.doi10.5194/gi-9-407-2020
dc.identifier.issn2193-0856
dc.identifier.officialurlhttp://dx.doi.org/10.5194/gi-9-407-2020
dc.identifier.relatedurlhttps://gi.copernicus.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/7566
dc.issue.number2
dc.journal.titleGeoscientific instrumentation methods and data systems
dc.language.isoeng
dc.page.final415
dc.page.initial407
dc.publisherCopernicus Gesellschaft Mbh
dc.relation.projectIDIN TIME (823934)
dc.relation.projectID(ESP2016-79135-R; PCIN-2014-013-C07-04; PCIN-2016-080; CGL2016-78702- C2-2-R; PID2019-105306RB-I00; RTI2018-096465- B-I00)
dc.relation.projectIDEDGEDATA-CM (S2018/TCS-4499)
dc.rightsAtribución 3.0 España
dc.rights.accessRightsopen access
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/es/
dc.subject.cdu550.3
dc.subject.keywordHetc-Heds
dc.subject.keywordHzetrn
dc.subject.keywordFluka
dc.subject.keywordNeutrons
dc.subject.keywordSpectra
dc.subject.keywordShield
dc.subject.keywordGeosciences
dc.subject.keywordMultidisciplinary
dc.subject.keywordMeteorology & Atmospheric Sciences
dc.subject.ucmGeofísica
dc.subject.ucmMeteorología (Física)
dc.subject.unesco2507 Geofísica
dc.titleOverview of the main radiation transport codes
dc.typejournal article
dc.volume.number9
dspace.entity.typePublication
relation.isAuthorOfPublicationcf5cf9ad-8e0e-4c40-966d-58da28c01b49
relation.isAuthorOfPublication.latestForDiscoverycf5cf9ad-8e0e-4c40-966d-58da28c01b49

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