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Geoscientific Instrumentation, Methods and Data Systems An interactive open-access journal of the European Geosciences Union
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Preprints
https://doi.org/10.5194/gi-2020-7
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/gi-2020-7
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Submitted as: review article 24 Jun 2020

Submitted as: review article | 24 Jun 2020

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This preprint is currently under review for the journal GI.

Overview of Main Radiation Transport Codes

Nikolaos Schetakis1,2, Rodrigo Crespo3, José Luis Vázquez-Poletti3, Mariano Sastre1,4, Luis Vázquez3,5, and Alessio Di Iorio1 Nikolaos Schetakis et al.
  • 1ALMA Sistemi SRL, Guidonia (Rome), 00012, Italy
  • 2School of Electrical and Computer Engineering, Technical University of Crete, Chania, Crete, 73100, Greece
  • 3Facultad de Informática, Universidad Complutense de Madrid, Madrid, 28040, Spain
  • 4Departamento de Física de la Tierra y Astrofísica, Universidad Complutense de Madrid, Madrid, 28040, Spain
  • 5Instituto de Matemática Interdisciplinar (IMI) Universidad Complutense de Madrid, Madrid, 28040, Spain

Abstract. Accurate predictions of expected radiation dose levels in Mars are made with space radiation transport codes, and various space agencies and institutions typically rely on a particular code that has been developed within their own national space agencies. We present these codes that are related to the simulation of the radiation on different scenarios on Mars surface. All of them have similar fields of applications but differ in several aspects, including energy range and types of projectiles considered, as well as the models of nuclear reactions considered.

Nikolaos Schetakis et al.

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Nikolaos Schetakis et al.

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